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  <front>
    <journal-meta>
<journal-id journal-id-type="publisher">BG</journal-id>
<journal-title-group>
<journal-title>Biogeosciences</journal-title>
<abbrev-journal-title abbrev-type="publisher">BG</abbrev-journal-title>
<abbrev-journal-title abbrev-type="nlm-ta">Biogeosciences</abbrev-journal-title>
</journal-title-group>
<issn pub-type="epub">1726-4189</issn>
<publisher><publisher-name>Copernicus GmbH</publisher-name>
<publisher-loc>Göttingen, Germany</publisher-loc>
</publisher>
</journal-meta>

    <article-meta>
      <article-id pub-id-type="doi">10.5194/bg-12-4161-2015</article-id><title-group><article-title>The role of photo- and thermal degradation for <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> and CO fluxes in an arid ecosystem</article-title>
      </title-group><?xmltex \runningtitle{Photo- and thermal degradation in an arid ecosystem}?><?xmltex \runningauthor{H.~van Asperen et~al.}?>
      <contrib-group>
        <contrib contrib-type="author" corresp="yes" rid="aff1">
          <name><surname>van Asperen</surname><given-names>H.</given-names></name>
          <email>v_asperen@iup.physik.uni-bremen.de</email>
        <ext-link>https://orcid.org/0000-0002-9639-4547</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Warneke</surname><given-names>T.</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2">
          <name><surname>Sabbatini</surname><given-names>S.</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2 aff3">
          <name><surname>Nicolini</surname><given-names>G.</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2">
          <name><surname>Papale</surname><given-names>D.</given-names></name>
          
        <ext-link>https://orcid.org/0000-0001-5170-8648</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Notholt</surname><given-names>J.</given-names></name>
          
        </contrib>
        <aff id="aff1"><label>1</label><institution>Institute of Environmental Physics, University of Bremen, Otto-Hahn-Allee 1, Bremen, 28359, Germany</institution>
        </aff>
        <aff id="aff2"><label>2</label><institution>Department for Innovation in Biological, Agro-food and Forest Systems (DIBAF), University of Tuscia, via S. Camillo de Lellis s.n.c., 01100 Viterbo, Italy</institution>
        </aff>
        <aff id="aff3"><label>3</label><institution>Euro Mediterranean Centre on Climate Change (CMCC) – Impacts on Agriculture, Forests and Ecosystem Services (IAFES), via A. Pacinotti 5, 01100 Viterbo, Italy</institution>
        </aff>
      </contrib-group>
      <author-notes><corresp id="corr1">H. van Asperen (v_asperen@iup.physik.uni-bremen.de)</corresp></author-notes><pub-date><day>14</day><month>July</month><year>2015</year></pub-date>
      
      <volume>12</volume>
      <issue>13</issue>
      <fpage>4161</fpage><lpage>4174</lpage>
      <history>
        <date date-type="received"><day>12</day><month>January</month><year>2015</year></date>
           <date date-type="rev-request"><day>04</day><month>February</month><year>2015</year></date>
           <date date-type="rev-recd"><day>19</day><month>June</month><year>2015</year></date>
           <date date-type="accepted"><day>23</day><month>June</month><year>2015</year></date>
      </history>
      <permissions>
<license license-type="open-access">
<license-p>This work is licensed under a Creative Commons Attribution 3.0 Unported License. To view a copy of this license, visit <ext-link ext-link-type="uri" xlink:href="http://creativecommons.org/licenses/by/3.0/">http://creativecommons.org/licenses/by/3.0/</ext-link></license-p>
</license>
</permissions><self-uri xlink:href="https://bg.copernicus.org/articles/12/4161/2015/bg-12-4161-2015.html">This article is available from https://bg.copernicus.org/articles/12/4161/2015/bg-12-4161-2015.html</self-uri>
<self-uri xlink:href="https://bg.copernicus.org/articles/12/4161/2015/bg-12-4161-2015.pdf">The full text article is available as a PDF file from https://bg.copernicus.org/articles/12/4161/2015/bg-12-4161-2015.pdf</self-uri>


      <abstract>
    <p>Recent studies have suggested the potential importance of abiotic
degradation in arid ecosystems. In this study, the role of photo- and
thermal degradation in ecosystem CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> and CO exchange
is assessed. A field experiment was performed in Italy using
an FTIR-spectrometer (Fourier Transform Infrared) coupled to a flux gradient system and to flux
chambers. In a laboratory experiment, field samples were exposed to
different temperatures and radiation intensities.</p>
    <p>No photodegradation-induced CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> and CO fluxes of in literature suggested magnitudes were
found in the field nor in the laboratory study. In the laboratory, we measured CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> and
CO fluxes that were derived from thermal degradation. In the field experiment,
CO uptake and emission have been measured and are proposed to be a result of biological uptake and
abiotic thermal degradation-production.</p>
    <p>We suggest that previous studies, addressing direct photodegradation,
have overestimated the role of photodegradation and observed fluxes
might be due to thermal degradation, which is an indirect effect of
radiation. The potential importance of abiotic decomposition in the
form of thermal degradation, especially for arid regions, should be
considered in future studies.</p>
  </abstract>
    </article-meta>
  </front>
<body>
      

<sec id="Ch1.S1" sec-type="intro">
  <title>Introduction</title>
      <p><inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> is the main carbon species being exchanged between
biosphere and atmosphere and the most important anthropogenic
greenhouse gas. <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula> is a less abundant non-greenhouse gas but
considered important in the climate debate due to its oxidation
process with atmospheric <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msup><mml:mi mathvariant="normal">OH</mml:mi><mml:mo>-</mml:mo></mml:msup></mml:mrow></mml:math></inline-formula> <xref ref-type="bibr" rid="bib1.bibx30" id="paren.1"/>. Yearly,
terrestrial ecosystems exchange approximately 120 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">Pg</mml:mi></mml:math></inline-formula>
of carbon with the atmosphere <xref ref-type="bibr" rid="bib1.bibx30" id="paren.2"/>.</p>
      <p>Arid ecosystems account for approximately 40 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">%</mml:mi></mml:math></inline-formula> of land area
and 20 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">%</mml:mi></mml:math></inline-formula> of the soil carbon pool but are still an unknown
factor in climate models <xref ref-type="bibr" rid="bib1.bibx22" id="paren.3"/>. In recent studies, the
possible importance of abiotic degradation for arid regions, such as
photo- and thermal degradation, has been recognized
<xref ref-type="bibr" rid="bib1.bibx2 bib1.bibx18 bib1.bibx26" id="paren.4"/>.</p>
<sec id="Ch1.S1.SS1">
  <?xmltex \opttitle{Ecosystem {$\chem{CO_{2}}$} fluxes; photo- and thermal degradation}?><title>Ecosystem <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> fluxes; photo- and thermal degradation</title>
      <p>Photodegradation is the direct breakdown of organic matter by radiation.
Photodegradation is known to be an important pathway in aquatic ecosystems
<xref ref-type="bibr" rid="bib1.bibx39" id="paren.5"/>. Recently, the possible importance of
photodegradation in terrestrial ecosystems has been suggested
<xref ref-type="bibr" rid="bib1.bibx2 bib1.bibx4 bib1.bibx13 bib1.bibx26" id="paren.6"/>. Photodegradation can play an important role in
arid ecosystems, where microbial decomposition is restricted
<xref ref-type="bibr" rid="bib1.bibx2 bib1.bibx4 bib1.bibx24 bib1.bibx25 bib1.bibx33" id="paren.7"/>.
<xref ref-type="bibr" rid="bib1.bibx26" id="text.8"/> estimated that in arid ecosystems
19 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">%</mml:mi></mml:math></inline-formula> of the annual <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> flux is induced by photodegradation
and, in dry summer conditions, even 92 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">%</mml:mi></mml:math></inline-formula> of daytime <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>
emissions can be attributed to this process.</p>
      <p>Photodegradation is attributed to UV as well as visible radiation
<xref ref-type="bibr" rid="bib1.bibx2 bib1.bibx4 bib1.bibx5" id="paren.9"/>. The biochemical
mechanisms behind photodegradation-induced carbon fluxes are not clear; it is
proposed that solar radiative energy breaks down the bonds of carboxyl,
directly producing <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> and other gas species
<xref ref-type="bibr" rid="bib1.bibx24" id="paren.10"/>. It has been hypothesized that rates of
photodegradation depend on plant and litter tissue type: lignin, one of the
most recalcitrant tissue in plant material (to microbial decomposition), is
expected to be most sensitive to photodegradation <xref ref-type="bibr" rid="bib1.bibx1 bib1.bibx18" id="paren.11"/>. However, while studies reporting photodegradation are
multiple, recent studies, aiming to further investigate the process, were
unable to observe the effects of photodegradation
<xref ref-type="bibr" rid="bib1.bibx20 bib1.bibx23 bib1.bibx34" id="paren.12"/>. A reason for this
discrepancy has not yet been found <xref ref-type="bibr" rid="bib1.bibx20 bib1.bibx23 bib1.bibx32 bib1.bibx34" id="paren.13"/>. It is important to notice that
in literature, the term photodegradation is sometimes also used for the
indirect effects of radiation on decomposition. One example is microbial
facilitation: radiation breaks down organic compounds into smaller molecules,
which are then more easily degradable for microbes. For a review on studies done
on photodegradation, please see King et al. (2012).</p>
      <p>A less studied abiotic degradation pathway is thermal degradation, the
temperature-dependent degradation of carbon in the absence of radiation
and possibly oxygen <xref ref-type="bibr" rid="bib1.bibx10 bib1.bibx24 bib1.bibx27" id="paren.14"/>. However, photodegradation is considered the
more dominant abiotic <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> producing process
<xref ref-type="bibr" rid="bib1.bibx24" id="paren.15"/>. Besides <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula> and
<inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> are also reported as products of photo- and thermal degradation
<xref ref-type="bibr" rid="bib1.bibx10 bib1.bibx24 bib1.bibx27 bib1.bibx31 bib1.bibx35" id="paren.16"/>.</p>
</sec>
<sec id="Ch1.S1.SS2">
  <?xmltex \opttitle{Ecosystem {$\chem{CO}$} fluxes; photo- and thermal degradation}?><title>Ecosystem <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula> fluxes; photo- and thermal degradation</title>
      <p>The role of <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula> in soils and ecosystems is not well
understood. Soils are known for being sources as well as sinks of
<inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula> <xref ref-type="bibr" rid="bib1.bibx7" id="paren.17"/>. Most likely, the main cause for soil
<inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula> uptake is the oxidation of <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula> to <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> or
<inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> by soil bacteria or soil enzymes <xref ref-type="bibr" rid="bib1.bibx3 bib1.bibx7 bib1.bibx17 bib1.bibx29 bib1.bibx36 bib1.bibx38" id="paren.18"/>. Soil
<inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula> consumption is found to be dependent on atmospheric
<inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula> concentrations and the consumption rate is usually expressed
in deposition velocity: the uptake rate divided by the
<inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula> concentration <xref ref-type="bibr" rid="bib1.bibx9 bib1.bibx21" id="paren.19"/>.</p>
      <p>Soil <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula> emissions have also been reported and are thought to be
of non-biological origin <xref ref-type="bibr" rid="bib1.bibx8 bib1.bibx9" id="paren.20"/>. For
example, soil <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula> emissions were found in peatlands
<xref ref-type="bibr" rid="bib1.bibx14" id="paren.21"/> and in arid soils
<xref ref-type="bibr" rid="bib1.bibx9" id="paren.22"/>. Living plants are also known to emit a small
amount of <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula> <xref ref-type="bibr" rid="bib1.bibx6 bib1.bibx19 bib1.bibx31" id="paren.23"/>. However, senescent plant material has been shown to
emit 5 to 10 times more than photosynthesising leaf material <xref ref-type="bibr" rid="bib1.bibx10 bib1.bibx27 bib1.bibx31" id="paren.24"/>. These fluxes, mostly determined in laboratory
studies, were attributed to thermal degradation and, to a larger extent,
photodegradation <xref ref-type="bibr" rid="bib1.bibx10 bib1.bibx24 bib1.bibx27" id="paren.25"/>.</p>
</sec>
<sec id="Ch1.S1.SS3">
  <title>Measurement of photo- and thermal degradation</title>
      <p>Studying photodegradation is difficult due to the multiple (indirect)
effects radiation has on total biological decomposition. For
example, UV-radiation is known to inhibit microbial processes, to
change (senescent) tissue chemistry and to alter the dominating microbial and fungal
communities, thereby affecting microbial decomposition rates in both
directions <xref ref-type="bibr" rid="bib1.bibx12 bib1.bibx28 bib1.bibx37 bib1.bibx39" id="paren.26"/>.
Differentiating photodegradation-induced fluxes
from biological sources in field experiments can be achieved by the comparison
of different flux measurement techniques such as eddy covariance (EC)
measurements vs. flux chamber measurements and/or soil gradient
measurements, in that one method does not receive solar radiation
<xref ref-type="bibr" rid="bib1.bibx26" id="paren.27"/>. This approach requires that the
areas or footprints sensed by the different techniques are fully
homogeneous, which is not often the case and hard to validate. To study the effects of photodegradation (in field or laboratory),
radiation filters can also be used to expose samples to different types or amounts of radiation <xref ref-type="bibr" rid="bib1.bibx4 bib1.bibx24 bib1.bibx25" id="paren.28"/>.</p>
      <p>Studying the role of thermal degradation-induced carbon fluxes is
challenging, especially for <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> due to the accompanying
effect temperature has on microbial decomposition. To study thermal
degradation-induced <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> production, microbial decomposition
should be absent, which can only be achieved in laboratory studies <xref ref-type="bibr" rid="bib1.bibx24" id="paren.29"/>.</p>
      <p>Previous field and laboratory studies on the role of direct or indirect abiotic degradation
report very contrasting results <xref ref-type="bibr" rid="bib1.bibx18 bib1.bibx20 bib1.bibx23 bib1.bibx24 bib1.bibx26 bib1.bibx34" id="paren.30"/>. More specific studies are thus
needed to better understand this process and its role in the carbon
cycle. In this study, we present the results of field and laboratory
measurements aimed to evaluate the role of direct photodegradation and
thermal degradation in an arid ecosystem.</p>
</sec>
</sec>
<sec id="Ch1.S2">
  <title>Materials and methods</title>
<sec id="Ch1.S2.SS1">
  <title>Study site</title>
      <p>We performed a field experiment in a grassland (IT-Ro4, harvested
cropland, approximately 250 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">m</mml:mi></mml:math></inline-formula> by 450 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">m</mml:mi></mml:math></inline-formula>, lat
42.37<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N, long 11.92<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E, 147 <inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="normal">m</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mi mathvariant="normal">a</mml:mi><mml:mo>.</mml:mo><mml:mi mathvariant="normal">s</mml:mi><mml:mo>.</mml:mo><mml:mi mathvariant="normal">l</mml:mi><mml:mo>.</mml:mo></mml:mrow></mml:math></inline-formula>), in
the province of Viterbo, Italy. The climate is Mediterranean, with
a typical drought period covering approximately 2 months during summer
(July–August). Mean annual temperature is 14 <inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C and annual
rainfall is 755 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">mm</mml:mi></mml:math></inline-formula>. Such climatic characteristics make the
site suitable for abiotic degradation studies. The underlying material
is tuff, soil texture is clay loam and soils are classified as Eutric
Cambisol. Yearly, the field site is ploughed to a depth of 20 or
50 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">cm</mml:mi></mml:math></inline-formula>. Just before the experiment, oat and vetch were
cultivated. During the experiment, vegetation was not managed and was
a mix of invasive species such as <italic>Amaranthus retroflexus</italic>, <italic>Chenopodium</italic> spp., <italic>Conyza canadensis</italic>, <italic>Artemisia vulgaris</italic>, <italic>Cirsium</italic> spp., <italic>Mercurialis annua</italic> and <italic>Polygonum</italic> spp. The field study was conducted in
July–September 2013. At the beginning of the experiment, most
vegetation was dried out, however, patches of active vegetation were
observed. Temperature and rainfall during measurements were
representative for the period (hot and dry) (Fig  2), however, the preceding
spring had been cold and rainy in respect to the average.</p>
      <p>IT-Ro4 is an experimental site managed by the University of Tuscia
(Viterbo). Continuous EC measurements of scalars and energy fluxes are
performed (LI-7500 open path analyzer, Licor, Lincoln, Nebraska, USA;
Windmaster Pro sonic anenomemeter, Gill, Hampshire, UK) along with
meteorological and environmental measurements (CNR-1, Kipp &amp; Zonen,
Delft, the Netherlands; soil water content, CS616, Campbell
Scientific, North Logan, USA; soil temperature, CS107, Campbell
scientific, North Logan, USA; soil heat flux, HFT3 Soil Heat Flux
Plate, Campbell scientific, North Logan, USA).</p>
</sec>
<sec id="Ch1.S2.SS2">
  <title>Instrumentation and set up</title>
      <p>The analyzer used in this study is based on a Fourier Transform Infrared
(FTIR)-spectrometer (Spectronus, Ecotech), for details on the FTIR-analyzer,
see <xref ref-type="bibr" rid="bib1.bibx15" id="text.31"/>. An FTIR is capable of measuring air
concentrations of <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">N</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mi mathvariant="normal">O</mml:mi></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula> and
<inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> simultaneously. Before being measured, air samples
were dried by a nafion dryer and by a column of magnesium perchlorate.
Measurements were corrected for pressure and temperature fluctuations and for
cross-sensitivities <xref ref-type="bibr" rid="bib1.bibx16" id="paren.32"/>. Background measurements and
a calibration routine using two standard gas cylinders were performed weekly.
We designed an external manifold box which allowed us to connect the FTIR to
a flux gradient (FG) setup and to two flux chambers (FC), simultaneously. Both
methods provide air concentration data as well as flux data. In this paper,
only <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula> flux data are presented.</p>
</sec>
<sec id="Ch1.S2.SS3">
  <title>Concentration and flux measurements</title>
      <p>FG measurements were performed once per hour and performed at the same
location as the EC tower. More information about the FG system can be found
in the Appendix. For FC measurements, six soil collars
(50 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">cm</mml:mi></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 50 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">cm</mml:mi></mml:math></inline-formula>) were inserted to 10 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">cm</mml:mi></mml:math></inline-formula> depth
a week before the start of the experiment. Positions of soil collars were
checked for being undisturbed and representative. The two flux chambers (open
dynamic chambers,
50 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">cm</mml:mi></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 50 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">cm</mml:mi></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 50 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">cm</mml:mi></mml:math></inline-formula>, produced by
Karlsruhe Institute of Technology, Germany) consisted of a stainless steel
frame, UV-transparent acrylic sides (Acryl Glass XT solar, 3mm,
UV-transparent) and a vent tube, and were tightened by the use of clamps and
rubber air strips. Transparency of the acrylic material was measured and
reported to be <inline-formula><mml:math display="inline"><mml:mi mathvariant="italic">&gt;</mml:mi></mml:math></inline-formula> 90 % in the UV and visible wavelength band
(280–700 nm). Two fans per flux chamber were continuously running, insuring
well-mixed headspace air. Automatic chamber closure (once per hour) was made
possible by use of a pneumatic system regulated by the valve manifold box.
Air flow from the flux chambers to the FTIR was initiated by a membrane pump
placed behind the measurement cell, set to 1 <inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="normal">L</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msup><mml:mi mathvariant="normal">min</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula>. Air flow
was measured every 2 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">min</mml:mi></mml:math></inline-formula> continuously for 20 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">min</mml:mi></mml:math></inline-formula> in flow
mode. Chamber opening and closure was after 4 and 18 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">min</mml:mi></mml:math></inline-formula>,
respectively. Sampling lines from the chambers were of equal size and
material and were tested for leaks regularly. Chamber temperatures were
recorded by temperature loggers (Voltcraft DL-1181THP). Fluxes were derived
from concentration increases after chamber closure, by use of linear
regression. Gas fluxes were calculated by:

                <disp-formula id="Ch1.E1" content-type="numbered"><mml:math display="block"><mml:mrow><mml:mi>F</mml:mi><mml:mo>=</mml:mo><mml:mfrac><mml:mrow><mml:mi>V</mml:mi><mml:mi>P</mml:mi></mml:mrow><mml:mrow><mml:mi>R</mml:mi><mml:mi>S</mml:mi><mml:mi>T</mml:mi></mml:mrow></mml:mfrac><mml:mfrac><mml:mrow><mml:mi mathvariant="italic">δ</mml:mi><mml:mi>C</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="italic">δ</mml:mi><mml:mi>t</mml:mi></mml:mrow></mml:mfrac><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>

          wherein <inline-formula><mml:math display="inline"><mml:mi>V</mml:mi></mml:math></inline-formula> is the volume of the chamber (m<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msup></mml:math></inline-formula>), <inline-formula><mml:math display="inline"><mml:mi>P</mml:mi></mml:math></inline-formula> the chamber air
pressure (Pa), <inline-formula><mml:math display="inline"><mml:mi>R</mml:mi></mml:math></inline-formula> the gas constant
(8.314 <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">m</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msup><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mi mathvariant="normal">Pa</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msup><mml:mi mathvariant="normal">K</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msup><mml:mi mathvariant="normal">mol</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula>), <inline-formula><mml:math display="inline"><mml:mi>S</mml:mi></mml:math></inline-formula> the chamber surface area
(m<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:math></inline-formula>), <inline-formula><mml:math display="inline"><mml:mi>T</mml:mi></mml:math></inline-formula> the chamber air temperature (K) and <inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="italic">δ</mml:mi><mml:mi>C</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="italic">δ</mml:mi><mml:mi>t</mml:mi></mml:mrow></mml:math></inline-formula> is
the gas concentration change over time (mol <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">mol</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msup><mml:mi mathvariant="normal">s</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula>). For flux calculations, only the
concentration increases between 2 and 10 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">min</mml:mi></mml:math></inline-formula> after closure
were used. Concentration increases were checked for non-linear trends
and, if found, not used. Flux standard deviations were derived from the
propagated standard deviations of the regression slope.</p>
      <p>When homogeneity in footprint can be assured, micrometeorological and
FC methods can be compared and used to study the role of
photodegradation. Flux chambers can be shielded from incoming
radiation, preventing photodegradation-induced carbon production,
while micrometeorological methods capture all fluxes. Comparing the
two methods therefore gives an indication of the presence and
the magnitude of photodegradation-induced carbon fluxes <xref ref-type="bibr" rid="bib1.bibx26" id="paren.33"/>.
The use of this method was planned for our field experiment, but could not be
applied due to lack of conformity between flux methods footprints, because of sparse
photosynthetically active vegetation present in the footprint of the FG technique,
causing the methods to be incomparable.</p>
      <p>To study photodegradation, two different flux chambers, one with and one
without solar radiation exposure were used. During this experiment, the flux
chambers were measuring six fixed chamber locations; chambers were manually
moved every few days. One flux chamber was made opaque by the use of light
excluding aluminum foil (on 5 August). On the days before
(28 July–5 August), all positions were compared by measuring the locations
with transparent chambers. On 3–5 August, the same locations were measured
(with transparent chambers) as on 5–8 August, when one of the two chambers
was covered. Both locations showed very similar <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula>
flux patterns. Unfortunately, on 8 August, a leak formed in the opaque
chamber system, therefore direct comparison between the two treatments is
limited to 3 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">days</mml:mi></mml:math></inline-formula>. Flux measurements made by the opaque chamber after
8 August are not shown. With blank measurements, the flux chambers were
tested for internal <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> and/or <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula> production. No <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>
production was found. Minor <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula> production was found during the day,
negligible in comparison to field <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula> production: values presented in
this paper are not corrected for this.</p>
      <p>Studying thermal degradation-induced <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> production in the
field is not possible due to the simultaneous temperature response of
biological <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> production. For <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula>, no temperature-dependent biological <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula> production is expected, wherefore
measurement of thermal degradation-induced <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula> production in
the field is possible. To study the role of thermal degradation in field
<inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula> exchange, chamber temperature sensors were installed,
measuring air temperature every minute.</p>
</sec>
<sec id="Ch1.S2.SS4">
  <title>Laboratory experiment</title>
      <p>Two different laboratory experiments were performed to study photo- and
thermal degradation. Grass samples (senescent above ground grass material,
mix of species as described in Methodology, pieces between 20–80 cm, not
ground) for the laboratory experiment were taken from the field site. Mixed
soil material samples were taken from the upper 3 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">cm</mml:mi></mml:math></inline-formula> of the soil,
soil samples were not sieved. Both sample types were dried at
35 <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula> for 72 h, to assure microbial activity to be negligible
<xref ref-type="bibr" rid="bib1.bibx24" id="paren.34"/>.</p>
      <p>Photodegradation of senescent grass material was studied with a system
consisting of a metal cylinder, inner diameter <inline-formula><mml:math display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 6.5 cm,
height <inline-formula><mml:math display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 25 cm, area <inline-formula><mml:math display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 33 cm<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:math></inline-formula>, with an acrylic cap, which could
be closed by screws. Transmittance of cap was measured and was 0.2 (250 nm), 6.1
(260 nm), 35.9 (270 nm), 73.9 (280 nm), 89.6 (290 nm) and approximately
94 % for larger wavelengths. The cylinder was placed beneath a UV-A and
UV-B source (manufacture instrument: Isitec GmbH, Bremerhaven; UV-A lamp:
Philips TL 60W/10R (peak emission at 375 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">nm</mml:mi></mml:math></inline-formula>), UV-B lamp: Philips TL
40W/12RS (peak emission at 310 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">nm</mml:mi></mml:math></inline-formula>)). Radiation intensities at the
sample location were quantified by use of an OceanOptics USB 2000
spectrometer with an optical fibre patch cord (P200-2-UV/VIS) and by an
ILT1700 research radiometer with accompanying optical filters and are
reported as comparison to natural radiation measured with the same
instruments (determined in summer in Northern Germany, midday, no clouds,
pointed at sun). Instrument radiation in the UV-A wavelength band
360–400 nm was measured to be 1.6 times higher than natural radiation, with
the peak emission being at 375 nm (2.9 times natural radiation). Instrument
radiation in the wavelength band 200–320 nm was measured to be 2.9 times
higher than natural radiation, with the peak emission being between 290 and
310 nm (7.7 times natural radiation). During the experiment, different
samples (empty cylinder, 2 gram-sample and 4 gram-sample) were exposed to
different types/amounts of radiation (no radiation, UV-A and/or UV-B
radiation). Grass in the cylinders was positioned so that at least 80 % of
the surface bottom was covered with grass material. During the experiments,
air was continuously circulated from the cylinder to the FTIR and measured
once per minute; emissions were derived from the measured concentration
changes. Cylinder temperatures were monitored by an internal temperature
probe (GTH 175/PT, Greisinger Electronics) and remained constant over the
experiments (21, sd <inline-formula><mml:math display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 0.15 <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula>). Every treatment was
performed for 30 min and was duplicated.</p>
      <p>To study thermal degradation, a glass flask (inner diameter <inline-formula><mml:math display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 6.7 cm,
height <inline-formula><mml:math display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 6 cm) was placed in a closed loop with the FTIR. For this
experiment, only glass and stainless steel materials were used. 4 grass
samples of 2 grams and 4 soil samples of 30 grams were taken. The grass
sample was distributed equally in the flask. The soil sample was not sieved
and filled approximately 1 cm (height) of the glass flask. The samples were
heated in temperature steps of 5<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> (20–65 <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula>) by use
of a controlled temperature water bath. Temperature time steps were 20 min. During the experiments, air was circulated from the glass flask to
the FTIR and measured once per minute. After approximately 3 min, a
stabilization in the <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula> production could be observed. Emissions were
derived from the measured concentration changes. Glass flask air temperatures
were manually measured to check if water bath temperature was representative
for grass and soil material temperatures; after 5 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">min</mml:mi></mml:math></inline-formula>, the glass
flask air temperature had reached the same temperature as the water. All
experiments were performed in duplicate and in dark conditions.</p>
      <p>In the results sections, the given regression coefficients from
polynomial fits are the explained sum of squares divided by the total
sum of squares.</p>
</sec>
</sec>
<sec id="Ch1.S3">
  <title>Results</title>
      <p>During the field campaign (3 August–11 September 2013), total precipitation
was 15 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">mm</mml:mi></mml:math></inline-formula> and air temperatures ranged between 13 and
43 <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula> (see Fig. 2). Soil water content, measured at
10 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">cm</mml:mi></mml:math></inline-formula> depth was 18 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">%</mml:mi></mml:math></inline-formula> (VWC) and decreased less than
1 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">%</mml:mi></mml:math></inline-formula> over the experiment.</p>
<sec id="Ch1.S3.SS1">
  <title>Flux measurements</title>
      <p>FG <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> fluxes are shown in the Appendix. FG <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula> uptake (up to
1 <inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="normal">nmol</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msup><mml:mi mathvariant="normal">m</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msup><mml:mi mathvariant="normal">s</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula>) and emission (on average
2 <inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="normal">nmol</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msup><mml:mi mathvariant="normal">m</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msup><mml:mi mathvariant="normal">s</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula>) at night were measured (Fig  1). During the
day, large (<inline-formula><mml:math display="inline"><mml:mrow><mml:mo>≥</mml:mo><mml:mn>10</mml:mn></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="normal">nmol</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msup><mml:mi mathvariant="normal">m</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msup><mml:mi mathvariant="normal">s</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula>) <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula> emissions were
recorded (Fig. 1). Based on the 31 days of FG measurements, on average net
150 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">µ</mml:mi></mml:math></inline-formula>mol CO <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">m</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula> per day was estimated to be emitted. FC <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>
and FC <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula> fluxes of the transparent flux chamber can be seen in
Fig. 2, rain events and incoming solar radiation are indicated. FC
<inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> fluxes showed a diurnal pattern with small emissions at night
(1 <inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="normal">µ</mml:mi><mml:mi mathvariant="normal">mol</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msup><mml:mi mathvariant="normal">m</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msup><mml:mi mathvariant="normal">s</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula>) and higher emissions during the day (up
to 8 <inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="normal">µ</mml:mi><mml:mi mathvariant="normal">mol</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msup><mml:mi mathvariant="normal">m</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msup><mml:mi mathvariant="normal">s</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula>). Large rain events on 20 and 27 August
(6.6 and 2 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">mm</mml:mi></mml:math></inline-formula>) caused a short increase in chamber <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> fluxes.
Locations without organic surface material (indicated as bare soils in Fig
 2) showed slightly lower <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula> fluxes.</p>
      <p>At night, <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula> uptake of maximum 0.8 <inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="normal">nmol</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msup><mml:mi mathvariant="normal">m</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msup><mml:mi mathvariant="normal">s</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula> was
observed. During the day, emissions up to 3 <inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="normal">nmol</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msup><mml:mi mathvariant="normal">m</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msup><mml:mi mathvariant="normal">s</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula> were
observed. Over the course of the experiment, nightly <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula> uptake was
continuously decreasing. The rain events caused a clear increase in nightly
<inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula> uptake, after which the decreasing continued (Figs. 1 and  2).
Based on 36 days of FC measurements,  on average net
30 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">µ</mml:mi></mml:math></inline-formula>mol CO <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">m</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula> per day was estimated to be emitted.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F1"><caption><p>Flux Gradient <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula> measurements over 8 days in August. A large
rain event took place on 20 August.</p></caption>
          <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://bg.copernicus.org/articles/12/4161/2015/bg-12-4161-2015-f01.pdf"/>

        </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F2" specific-use="star"><caption><p><bold>(a, b)</bold> Chamber <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula> fluxes  (errorbars with SD of flux are included but not visible due to
low value) during field experiment, different colors are different
locations. The two bare soil locations (soils without organic surface material) are  both presented with green diamonds. Rain events
(open diamonds) are indicated. Presented data are from transparent flux chamber measurements; <bold>(c)</bold> Air temperature
(<inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula>) (red circles) and radiation (W m<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>) (black line).</p></caption>
          <?xmltex \igopts{width=483.69685pt}?><graphic xlink:href="https://bg.copernicus.org/articles/12/4161/2015/bg-12-4161-2015-f02.pdf"/>

        </fig>

</sec>
<sec id="Ch1.S3.SS2">
  <title>Photo- and thermal degradation</title>
      <p>Photodegradation was studied by comparing opaque and transparent
chamber measurements of 3 days (5–8 August) and by analysis of
transparent FC data of a period in August (period with fixed location,
stable weather conditions and no precipitation). Analysis of different periods (different locations with similar conditions) showed
similar patterns.</p>
      <p>Possible photo- and/or thermal degradation-induced <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> fluxes
are not shown or evaluated here: FG <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> fluxes were too small
for dependency analysis and <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> chamber fluxes mostly showed
uptake, indicating a different process than photo- or
thermal degradation.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F3" specific-use="star"><caption><p>Transparent and opaque flux chamber <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> fluxes (left) and
<inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula> fluxes
(right) vs. air temperature <bold>(a, b)</bold> and chamber
temperature after 6 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">min</mml:mi></mml:math></inline-formula> closure <bold>(c, d)</bold>. Regression
coefficients of polynomial fits are given in the legends.</p></caption>
          <?xmltex \igopts{width=426.791339pt}?><graphic xlink:href="https://bg.copernicus.org/articles/12/4161/2015/bg-12-4161-2015-f03.pdf"/>

        </fig>

<sec id="Ch1.S3.SS2.SSS1">
  <?xmltex \opttitle{{$\chem{CO_{2}}$} fluxes}?><title><inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> fluxes</title>
      <p>Figure 3 shows the <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> fluxes (of transparent and opaque
chamber) vs. air temperatures (Fig. 3a) and chamber temperatures
(after 6 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">min</mml:mi></mml:math></inline-formula> closure, Fig. 3c). FC measurements showed very
weak dependency on soil temperatures at 10 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">cm</mml:mi></mml:math></inline-formula> (data not
shown). Blocking radiation showed no distinguished impact on measured
<inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> fluxes. Chamber <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> fluxes correlate well with air
temperatures and less with chamber temperatures (Fig. 3a and c). Chamber
coverage had an effect on chamber temperatures; during daytime hours,
the opaque chamber temperature differed up to 10 <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula> from the
transparent chamber temperature.</p>
</sec>
<sec id="Ch1.S3.SS2.SSS2">
  <?xmltex \opttitle{{$\chem{CO}$} fluxes}?><title><inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula> fluxes</title>
      <p>A clear effect of chamber coverage on <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula> fluxes was visible;
transparent chamber fluxes were higher during the
day. FC <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula> fluxes correlate better with chamber temperatures
than with air temperatures (Fig. 3b and d).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F4" specific-use="star"><caption><p>Transparent flux chamber <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula> fluxes for 15–19 August
vs. air temperature <bold>(a)</bold>, chamber temperature after
6 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">min</mml:mi></mml:math></inline-formula> closure <bold>(b)</bold> and solar radiation
<bold>(c)</bold>. Regression coefficients of polynomial fits are given
in the legends.</p></caption>
            <?xmltex \igopts{height=426.791339pt}?><graphic xlink:href="https://bg.copernicus.org/articles/12/4161/2015/bg-12-4161-2015-f04.pdf"/>

          </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F5"><caption><p>Fitted <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula> fluxes for 15–19 August (black line) for measured
field <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula> fluxes (purple diamonds)(<inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi>R</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mo>=</mml:mo><mml:mn>0.85</mml:mn></mml:mrow></mml:math></inline-formula>). The cumulative fitted
<inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula> flux is a sum of fitted
<inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula> uptake (with <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>Q</mml:mi><mml:mn>10</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 1.8, based on literature
<xref ref-type="bibr" rid="bib1.bibx36" id="paren.35"/> and fitted <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula> production (with <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>Q</mml:mi><mml:mn>10</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 2.1)
based on chamber temperature (after 6 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">min</mml:mi></mml:math></inline-formula> closure).</p></caption>
            <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://bg.copernicus.org/articles/12/4161/2015/bg-12-4161-2015-f05.pdf"/>

          </fig>

      <p>Figure 4 shows <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula> fluxes in the transparent chamber vs. air
temperatures (Fig. 4a), chamber temperatures (after 6 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">min</mml:mi></mml:math></inline-formula>
closure, Fig. 4b) and amount of solar radiation (Fig. 4c) for a period in
August.  Again, <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula> fluxes relate best to chamber temperatures,
and less to air temperatures and amount of incoming radiation (Fig. 4).</p>
      <p>A temperature dependent biological <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula> uptake curve was fitted over
chamber temperature data from (cold) night conditions (when abiotic fluxes
are assumed to be minimal) and extrapolated to warmer temperatures. For
biological <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula> uptake, a <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>Q</mml:mi><mml:mn>10</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>-value from literature of 1.8 was chosen <xref ref-type="bibr" rid="bib1.bibx36" id="paren.36"/>. An
abiotic thermal degradation <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>Q</mml:mi><mml:mn>10</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>-curve was fitted, also based on chamber
temperature data, with a fitted <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>Q</mml:mi><mml:mn>10</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>-value of 2.1. The sum of both
processes agrees well the observed field <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula> fluxes (<inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi>R</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mo>=</mml:mo><mml:mn>0.85</mml:mn></mml:mrow></mml:math></inline-formula>,
Fig. 5).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F6"><caption><p><bold>(a)</bold> Average <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> production of grass and soil
material (nmol <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">min</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msup><mml:mi mathvariant="normal">gr</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula>) over different
temperatures in the laboratory experiment; <bold>(b)</bold> average
<inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula> production of grass and soil material
(nmol <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">min</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msup><mml:mi mathvariant="normal">gr</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula>) over different temperatures in
the laboratory experiment, with fitted <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>Q</mml:mi><mml:mn>10</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>-value.</p></caption>
            <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://bg.copernicus.org/articles/12/4161/2015/bg-12-4161-2015-f06.pdf"/>

          </fig>

</sec>
<sec id="Ch1.S3.SS2.SSS3">
  <title>Laboratory experiment</title>
      <p>In the laboratory, exposure of senescent plant material from the field site
to high intensity UV-radiation did not result in increased <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> or
<inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula> fluxes in comparison to measurements performed in dark conditions
(data shown in Appendix).</p>
      <p>Grass and soil material samples exposed to different temperatures, under dark
conditions, showed significant <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> production during lower
temperatures (<inline-formula><mml:math display="inline"><mml:mrow><mml:mo>&lt;</mml:mo><mml:mn>40</mml:mn></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula>) and displayed small <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>
emissions at higher temperatures (<inline-formula><mml:math display="inline"><mml:mrow><mml:mo>&gt;</mml:mo><mml:mn>55</mml:mn></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula>) (Fig. 6a). For
<inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula>, clear thermal production was found, exponentially increasing with
higher temperatures (Fig. 6b). A <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>Q</mml:mi><mml:mn>10</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>-value of 2.14 for senescent grass
material and 2.00 for soil material was found to fit best to the observed
laboratory thermal degradation <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula> fluxes (Fig. 6b).</p><?xmltex \hack{\newpage}?>
</sec>
</sec>
</sec>
<sec id="Ch1.S4">
  <title>Discussion</title>
<sec id="Ch1.S4.SS1">
  <?xmltex \opttitle{{$\chem{CO_{2}}$} fluxes}?><title><inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> fluxes</title>
      <p>EC and FG measurements showed that the arid grassland was not yet in a dormant
state; significant <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> uptake was observed during the day (Appendix Fig. B1).
FC <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> measurements, performed on locations without photosynthetic
active vegetation, solely showed positive <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> fluxes, with peak
emissions during the day up to 8 <inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="normal">µ</mml:mi><mml:mi mathvariant="normal">mol</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msup><mml:mi mathvariant="normal">m</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msup><mml:mi mathvariant="normal">s</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula>. Figure 3a
shows that <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> fluxes mostly relate to air temperatures, and
poorly relate to soil temperatures (not shown). Expected is that most
<inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> production takes place close to the surface where the temperature
follows air temperatures closer than it follows soil temperatures at
10 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">cm</mml:mi></mml:math></inline-formula> depth. In the ecosystem, the rain events resulted in an
increase in <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> production for several days, showing the typical
water-dependent response of arid ecosystem respiration (Fig. 2 and B1).</p>
</sec>
<sec id="Ch1.S4.SSx1" specific-use="unnumbered">
  <title>Photo- and thermal degradation</title>
      <p>In the thermal degradation laboratory experiment, <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> production from
senescent plant and soil material was observed during lower temperatures
(20–40 <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula>), indicating remaining biological activity, even
after drying. Above 50 <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula>, an increasing <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>
production was observed with increasing temperatures, therefore expected to
be (partly) of non-biological origin. Possible abiotic <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> production
of approximately 3 <inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="normal">nmol</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msup><mml:mi mathvariant="normal">min</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msup><mml:mi mathvariant="normal">gr</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula> for senescent grass
material was observed. Extrapolating the thermal production rates of the
senescent grass material to field conditions (assuming 200 gr of senescent
plant material per m<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:math></inline-formula> at 55 <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula>), would result in a minor
flux of 0.01 <inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="normal">µ</mml:mi><mml:mi mathvariant="normal">mol</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msup><mml:mi mathvariant="normal">m</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msup><mml:mi mathvariant="normal">s</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula>, in comparison to observed field
fluxes of <inline-formula><mml:math display="inline"><mml:mrow><mml:mo>&gt;</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="normal">µ</mml:mi><mml:mi mathvariant="normal">mol</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msup><mml:mi mathvariant="normal">m</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msup><mml:mi mathvariant="normal">s</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula>. Based on the observations in
the laboratory, it is expected that the soil material also produces thermal
degradation-induced <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> fluxes. However, considering the relative
cold and wet conditions of the subsurface soil material in the
field, compared to laboratory conditions and to surface temperatures, it is
expected that soil thermal degradation fluxes are minor in comparison to soil
biological fluxes.</p>
      <p>Other studies have observed thermal degradation-induced
<inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> fluxes with higher rates
(approximately 125 <inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="normal">nmol</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msup><mml:mi mathvariant="normal">gr</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msup><mml:mi mathvariant="normal">min</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula> for C3-grass at
55 <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula>),
but also at lower temperatures <xref ref-type="bibr" rid="bib1.bibx24" id="paren.37"/>. We can not
verify this observation for our field material. Based on our
observations, we propose that under natural conditions, when
soil surface temperatures and especially soil subsurface temperatures
rarely exceed 55 <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula>, thermal degradation-induced
<inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> fluxes do not play an important role in comparison to
biological production, even in arid regions such as our study area.</p>
      <p>We observed that chamber design can strongly influence chamber
temperatures: during midday, the opaque and transparent chamber temperatures could differ up to
10 <inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C. As observed in the laboratory experiment,
unnatural high temperatures might lead to abiotic thermal
<inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> production. A research methodology aimed at measuring
photodegradation can unintentionally result in high surface
temperature levels, which could lead to unrepresentative high abiotic
<inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> production estimates.</p>
      <p>The simultaneous use of opaque and transparent chambers was employed to study
the effect of radiation on carbon fluxes in the field. Blocking radiation had
no visible effect on field chamber <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> fluxes (Fig. 3a and c).
<inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> flux measurements performed on bare soil locations (soils without
organic surface material) seemed lower than other locations; senescent
surface material seemed to contribute to total <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> fluxes (Fig. 2a).
However, only 3 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">days</mml:mi></mml:math></inline-formula> of bare soil measurements are available and no
opaque chamber measurements on bare soil are present, therefore comparison is
restricted.</p>
      <p>The flux chambers, which were used to assess photodegradation, had a
transparency of 90 % or higher in the UV-B, UV-A and visible wavelength
band. For our field experiment, we can therefore conclude that no large
direct photodegradation fluxes (as suggested by Rutledge et al., 2010 of
1 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">µ</mml:mi></mml:math></inline-formula>mol m<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> s<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>) have been induced by natural sunlight
intensities. In the laboratory experiment, field site grass samples received
above natural-intensity UV-radiation. In this experiment, no direct
photodegradation fluxes were observed from field site grass material. While
the laboratory experiment presented here does not prove that there are no
photodegradation fluxes at all, the results from the laboratory experiment
support the conclusion from the field experiment that direct
photodegradation fluxes in arid ecosystems are not as important as suggested
by a previous study <xref ref-type="bibr" rid="bib1.bibx26" id="paren.38"/>.</p>
      <p>The experiment was conducted on a field site situated in a Mediterranean
climate. Based on annual precipitation and on measured respiration values,
the ecosystem might seem too wet to be suitable to measure arid ecosystem
processes. However, the climate is known for the precipitation free summers
with high irradiation, causing the soil surface and surface materials to be
fully dried out in summer. Since photodegradation is taking place at the soil
surface, the ecosystem can be considered suitable for the assessment of this
arid ecosystem process. The absolute amounts of possible photodegradation
fluxes are not influenced by the respiration fluxes. The expected rates of
photodegradation fluxes (of 1 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">µ</mml:mi></mml:math></inline-formula>mol m<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> s<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>,
<xref ref-type="bibr" rid="bib1.bibx26" id="paren.39"/>) should have been detectable, even when
mixed with respiratory fluxes.</p>
      <p>Similar to what has been found by <xref ref-type="bibr" rid="bib1.bibx20 bib1.bibx23 bib1.bibx34" id="text.40"/>, we did not observe the effects of photodegradation in the field
nor in the laboratory: no direct photodegradation-induced
<inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> fluxes have been observed. This is in contrast to other
photodegradation studies, which have reported photodegradation fluxes in the
field <xref ref-type="bibr" rid="bib1.bibx26" id="paren.41"/> or in the laboratory
<xref ref-type="bibr" rid="bib1.bibx24" id="paren.42"/>. Potential explanations for this difference are:
(a) the used field methodology in the previous study was not suitable for
measuring direct abiotic degradation fluxes; (b) the role and significance of
photodegradation differs per material and per field site; (c) studies might
(partly) have misinterpreted thermal degradation fluxes as photodegradation
fluxes or (d) photodegradation fluxes were too small to be observed by the
presented method. We therefore do not question the existence of the
photodegradation process, but doubt its suggested large role in arid
ecosystems. However, as shown, the magnitude and the potential importance of
thermal degradation-induced <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> fluxes in arid ecosystems are still
unknown.</p>
</sec>
<sec id="Ch1.S4.SS2">
  <?xmltex \opttitle{{$\chem{CO}$} fluxes}?><title><inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula> fluxes</title>
      <p>During the measurement period, both <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula> uptake and emission have
been observed by the FG method (patches of green active vegetation
inside the footprint) as well as by the FC method (no photosynthetic active
vegetation contributing to the fluxes) (Figs. 1 and 2). <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula> exchange measurements from
FG and FC differed largely, most likely caused by the difference in footprint.</p>
      <p>During the night, uptake of up to 1 <inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="normal">nmol</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msup><mml:mi mathvariant="normal">m</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msup><mml:mi mathvariant="normal">s</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula> of <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula>
was observed, which is most likely caused by microbial oxidation to
<inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> or <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> <xref ref-type="bibr" rid="bib1.bibx3 bib1.bibx6 bib1.bibx7 bib1.bibx17 bib1.bibx29 bib1.bibx38 bib1.bibx36" id="paren.43"/>. The <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula> uptake was decreasing over time but a rain
event caused an enhanced uptake for some days (Figs. 1 and 2). Soil biota
being responsible for the <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula> uptake seems plausible since the effect
of drought (decreasing uptake over time) and the effect of the rain (enhanced
uptake) indicate a biological process. Nevertheless, with solely biological
<inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula> uptake taking place, one would expect higher uptake during warmer
temperatures and no <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula> emission. It is expected that an abiotic
process occurs simultaneously with the biotic uptake of <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula>, leading to
a buffering effect on CO uptake. For this reason, CO
deposition velocities could not be calculated.</p>
</sec>
<sec id="Ch1.S4.SSx2" specific-use="unnumbered">
  <title>Photo- and thermal degradation</title>
      <p>We propose that the observed <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula> emissions in the flux chambers are caused by thermal degradation.
FG measurements showed <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula> emissions during the day as well as
during the night, indicating that <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula> is not (solely) produced
by photodegradation (Fig. 1). By means of opaque chamber
measurements, lower <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula> fluxes, in comparison to
transparent chamber measurements, were detected. However, as described
before, FC temperatures were strongly affected by the blocking of
solar radiation. Analysis of <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula> fluxes showed a strong
correlation with FC temperatures, and no relationship with radiation
input, indicating that it was not the absence of
radiation, but the indirect effect on temperature that caused the lower <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula> emissions (Figs. 3 and 4).</p>
      <p>FC <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula> fluxes were ranging between <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>1 and
2.5 <inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="normal">nmol</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msup><mml:mi mathvariant="normal">m</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msup><mml:mi mathvariant="normal">s</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula> and only originated from soil or surface
litter, since photosynthetic active vegetation was absent. Measured <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula>
emissions are higher than reported for <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula> emissions from living plants
and similar to values found for senescent plant material
<xref ref-type="bibr" rid="bib1.bibx6 bib1.bibx10 bib1.bibx24 bib1.bibx27 bib1.bibx39" id="paren.44"/>.
However, the measurements are a cumulative signal of uptake and emission and
can therefore not be compared directly to other studies.</p>
      <p>In the laboratory experiment, where grass from the field site was exposed to
above natural intensity UV-radiation, no photodegradation-induced <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula>
fluxes were observed. However, significant thermal degradation-induced fluxes
from the senescent grass and soil material were measured, even measurable at
low temperatures (20 <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula>). At 50 <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula>, a thermal
<inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula> production rate of senescent grass material of
0.13 <inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="normal">nmol</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msup><mml:mi mathvariant="normal">min</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msup><mml:mi mathvariant="normal">gr</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula> was found. Extrapolating this
observation to field conditions (assuming 200 grams of senescent plant
material per m<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:math></inline-formula> at 50 <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula>), would result in a flux of
approximately 0.4 <inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="normal">nmol</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msup><mml:mi mathvariant="normal">m</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msup><mml:mi mathvariant="normal">s</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula>, which is approximately 5
times lower than the net measured field <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula> fluxes. Extrapolating the
thermally-induced <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula> production rate of the soil material to field
conditions would result in an estimated production of approximately 1
<inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="normal">nmol</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msup><mml:mi mathvariant="normal">m</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msup><mml:mi mathvariant="normal">s</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula> from the upper 3 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">cm</mml:mi></mml:math></inline-formula> of the soil during
a summer day. However, while this estimate indicates that abiotic thermal
soil CO production indeed might play a major role, for accurate estimates for
net soil <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula> uptake or emission, more information about biological
<inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula> uptake and about the soil profile is needed.</p>
      <p>The observed field chamber <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula> fluxes are suggested to be a cumulative
signal of biological uptake and abiotic thermal degradation. Both processes
were fitted over chamber temperatures. For the fitting of biological
<inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula> uptake, a <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>Q</mml:mi><mml:mn>10</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>-value of 1.8 was chosen
<xref ref-type="bibr" rid="bib1.bibx36" id="paren.45"/>. To match the cumulative measured <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula> fluxes
(purple diamonds in Fig. 5), a higher <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>Q</mml:mi><mml:mn>10</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>-value of 2.1 for the abiotic
thermal soil <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula> production was fitted (<inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi>R</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mo>=</mml:mo><mml:mn>0.85</mml:mn></mml:mrow></mml:math></inline-formula>).</p>
      <p>The laboratory measurements were used to experimentally determine
the <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>Q</mml:mi><mml:mn>10</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>-value of thermal degradation-induced <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula> fluxes.
<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>Q</mml:mi><mml:mn>10</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>-values of 2.14 for senescent grass and 2.00 for soil material were
measured. These values are similar to the <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>Q</mml:mi><mml:mn>10</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>-value which was fitted for
the thermal degradation process to match the cumulative field measurements,
as described in the previous paragraph (Fig. 5).</p>
      <p>The soil <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula> uptake process, taking place below the surface, is subject
to buffered chamber temperatures, and therefore the chosen <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>Q</mml:mi><mml:mn>10</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>-value
might be an underestimation. Also, the biological soil uptake is not expected
to follow the <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>Q</mml:mi><mml:mn>10</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>-temperature response at higher temperatures
(<inline-formula><mml:math display="inline"><mml:mrow><mml:mo>&gt;</mml:mo><mml:mn>35</mml:mn></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula>). Nevertheless, the difference in temperature
response (as a consequence of different <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>Q</mml:mi><mml:mn>10</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>-values or as a consequence
of buffered temperatures) causes biological <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula> uptake to be dominant
during colder (chamber) temperatures, and thermal degradation to be dominant
during warmer (chamber) temperatures. During our field experiment, thermal
degradation started to be dominant from approximately 25 <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula>
(chamber temperature) and followed an exponential curve with higher
temperatures (Fig. 5).</p>
      <p>The temperatures inside the chamber were higher than the temperatures outside
the chamber. Although this will result in higher fluxes inside the chamber
compared to the ecosystem around it, the correlation between temperatures
inside the chamber and the <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula> flux should be representative for the
ecosystem. The laboratory study shows a similar relationship between
temperature and <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula> flux. According to our results, the temperatures
outside the chamber are high enough to induce significant thermal degradation
fluxes. This is supported by the measured <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula> fluxes by the FG
technique. FG <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula> emissions were higher, likely due to its footprint
which contained relatively more dead vegetation (thermal degradation
material) since, for practical reasons, the chambers were placed over lower
dead vegetation. Also, the FG footprint contained active vegetation, which is
another possible <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula> emitting source <xref ref-type="bibr" rid="bib1.bibx6" id="paren.46"/>.</p>
      <p><?xmltex \hack{\newpage}?>Overall, the measurements show that the field site is
a net source of <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula> during the summer months, affecting the
atmospheric chemistry, at least at plant level, via OH<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>-</mml:mo></mml:msup></mml:math></inline-formula>
depletion. More field measurements on annual <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula> exchange are
needed to better understand the role of thermal degradation in
<inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> exchange in arid regions.</p>
</sec>
</sec>
<sec id="Ch1.S5" sec-type="conclusions">
  <title>Conclusions</title>
      <p>In our field and laboratory experiment, direct photodegradation-induced
<inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula> fluxes have not been observed. Based on laboratory
experiments, the production of thermal degradation-induced <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> is
expected, but only significant under unnaturally high temperatures. In the
laboratory, thermal degradation-induced <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula> fluxes were clearly
observed, also at relatively low temperatures (20 <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula>). In the
field, biological <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula> uptake as well as abiotic <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula> production
was observed; abiotic <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula> production is assumed to be mainly a product
of thermal degradation. The <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>Q</mml:mi><mml:mn>10</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>-value of the <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula> producing thermal
degradation process, as determined in the laboratory, agrees well with the
fitted <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>Q</mml:mi><mml:mn>10</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>-value for abiotic <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula> fluxes measured at the field
site.</p>
      <p>Not all litter types are reported to be sensitive to photodegradation, which
could explain why we did not measure photodegradation-induced fluxes. Also,
we realize that in field conditions, partitioning photodegradation from
thermal degradation or biological processes is challenging and minor
photodegradation fluxes might not be detectable. We therefore do not exclude
the existence of photodegradation. However, in our field experiment in an
arid ecosystem, we were not able to observe any direct
photodegradation-induced carbon fluxes, showing that direct photodegradation
does not play a major role in this arid ecosystem. Previous studies
suggesting the occurrence of major photodegradation fluxes might possibly
have neglected thermal degradation fluxes, which is an indirect effect of
radiation. The potential importance of abiotic decomposition in the form of
thermal degradation, especially for arid regions, should be considered and be
studied in more detail.</p><?xmltex \hack{\clearpage}?>
</sec>

      
      </body>
    <back><app-group>

<app id="App1.Ch1.S1">
  <title>Flux Gradient method</title>
      <p>FG measurements were performed once per hour. Air inlet heights were at 1.3
and 4.2 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">m</mml:mi></mml:math></inline-formula>. Air was sampled at 1 <inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="normal">L</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msup><mml:mi mathvariant="normal">min</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula>. Sampling lines
of stainless steel were used for the experiment. For 30 <inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="normal">min</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msup><mml:mi mathvariant="normal">h</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula>,
the airflows were led to air sampling bags, after that the bag inlet was
closed until analysis. Before the analysis, the FTIR measurement cell was
evacuated and flushed twice with measurement air before being filled. Per air
sample, a 3 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">min</mml:mi></mml:math></inline-formula>-spectra (static) measurement was taken. FG
measurements were performed at the same point as of the EC set-up
(measurement height at 3.5 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">m</mml:mi></mml:math></inline-formula>). During day time, footprint analysis
showed that 90 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">%</mml:mi></mml:math></inline-formula> of the source area of the EC signal came from the
grassland area within 150 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">m</mml:mi></mml:math></inline-formula>. Since the FG method is measuring at the
same location and height, it is expected that daytime FG fluxes mainly
originate from the grassland area as well. During nighttime, footprint
analysis showed fluxes mainly originating from outside the grassland. FG
<inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> fluxes agreed well with EC fluxes and ranged between <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>7 and
8 <inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="normal">µ</mml:mi><mml:mi mathvariant="normal">mol</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msup><mml:mi mathvariant="normal">m</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msup><mml:mi mathvariant="normal">s</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula> (Fig. B1) By using the FG method, fluxes can
be calculated by:

              <disp-formula id="App1.Ch1.E1" content-type="numbered"><mml:math display="block"><mml:mrow><mml:mi>F</mml:mi><mml:mo>=</mml:mo><mml:mi>K</mml:mi><mml:mfrac><mml:mrow><mml:mi mathvariant="italic">δ</mml:mi><mml:mi>C</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="italic">δ</mml:mi><mml:mi>z</mml:mi></mml:mrow></mml:mfrac><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>

        wherein <inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="italic">δ</mml:mi><mml:mi>C</mml:mi></mml:mrow></mml:math></inline-formula> is the difference in concentration of a gas species
(<inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="normal">mol</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msup><mml:mi mathvariant="normal">m</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula>) between the two inlet-heights (<inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="italic">δ</mml:mi><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> (m)) and <inline-formula><mml:math display="inline"><mml:mi>K</mml:mi></mml:math></inline-formula>
is the diffusion coefficient (<inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">m</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msup><mml:mi mathvariant="normal">s</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula>), and <inline-formula><mml:math display="inline"><mml:mi>F</mml:mi></mml:math></inline-formula> the flux
(<inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="normal">mol</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msup><mml:mi mathvariant="normal">m</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msup><mml:mi mathvariant="normal">s</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula>). <inline-formula><mml:math display="inline"><mml:mi>K</mml:mi></mml:math></inline-formula> can be parameterized using the data of
a sonic anemometer, based on the friction velocity (<inline-formula><mml:math display="inline"><mml:mi>u</mml:mi></mml:math></inline-formula>-star), the Von
Karman-constant, the effective height and the stability factor (<inline-formula><mml:math display="inline"><mml:mi mathvariant="italic">ζ</mml:mi></mml:math></inline-formula>)
<xref ref-type="bibr" rid="bib1.bibx11" id="paren.47"/>.</p>
</app>

<app id="App1.Ch1.S2">
  <title>Laboratory photodegradation experiment</title>
      <p>CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> and CO grass sample emission was measured under dark and UV-radiation
conditions and compared to blank measurements (Fig. B2). In comparison to
blank measurements, no positive influence of UV-radiation was found on CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>
and CO production. Observed emissions under UV-radiation were slightly
smaller than in dark conditions, which could be caused by the inhibiting
effect of UV-radiation on microbial decomposition <xref ref-type="bibr" rid="bib1.bibx23" id="paren.48"/>.
However, differences were not significant.
<xref ref-type="bibr" rid="bib1.bibx26" id="text.49"/> estimated photodegradation
fluxes of 1 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">µ</mml:mi></mml:math></inline-formula>mol CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> m<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> s<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> in sunny conditions
(60 000 nmol CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> m<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> min<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>). Considered are the following
assumptions: 80 % of field site surface is covered with dry organic matter.
80 % of laboratory surface is covered with dry organic matter. Expected is
that at least 50 % of photodegradation is caused by UV-radiation. The
laboratory samples received 2 times more UV-radiation than under natural
conditions. Sample rates are measured over 0.0033 m<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> (33 cm<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>).
Based on Rutledge (2010), the following emission magnitudes were therefore
expected in the laboratory experiment:
60 000 <inline-formula><mml:math display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 0.5 <inline-formula><mml:math display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 2 <inline-formula><mml:math display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 0.0033 <inline-formula><mml:math display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 200 nmol
CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> min<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> per sample. <xref ref-type="bibr" rid="bib1.bibx27" id="text.50"/> measured approximately
250 nmol CO m<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> min<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> (250 <inline-formula><mml:math display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 10<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">9</mml:mn></mml:msup></mml:math></inline-formula>
molecules cm<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> s<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>) of photodegradation fluxes under peak daytime
radiation. Considering the same assumptions, then CO emissions with a
magnitude of
250 <inline-formula><mml:math display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 0.5 <inline-formula><mml:math display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 2 <inline-formula><mml:math display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 0.0033 <inline-formula><mml:math display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 8.3 nmol m<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> min<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>
per sample were expected. Calculated expected productions rates are indicated in
Fig. B2.</p>

      <?xmltex \floatpos{t}?><fig id="App1.Ch1.F1"><caption><p>Comparison of Flux Gradient- and Eddy Covariance-<inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> flux
measurements over 8 days in August. There was a large rain event on 20 August.</p></caption>
        <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://bg.copernicus.org/articles/12/4161/2015/bg-12-4161-2015-f07.pdf"/>

      </fig>

      <?xmltex \floatpos{h}?><fig id="App1.Ch1.F2" position="anchor"><caption><p>Results of photodegradation laboratory experiment. Results are for 2
gram samples, placed in a 33 cm<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:math></inline-formula> cylinder. Upper figures: CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>
production under different treatments. Exp. prod. stands for expected
production based on comparison to Rutledge (2010). Right figure is zoom-in of
left figure. Lower figures: CO production under different treatments. Exp.
prod. stands for expected production based on comparison to Schade (1999).
Right figure is zoom-in of left figure.</p></caption>
        <?xmltex \hack{\hsize\textwidth}?>
        <?xmltex \igopts{width=426.791339pt}?><graphic xlink:href="https://bg.copernicus.org/articles/12/4161/2015/bg-12-4161-2015-f08.pdf"/>

      </fig>

<?xmltex \hack{\clearpage}?>
</app>
  </app-group><ack><title>Acknowledgements</title><p>We are grateful for the support of InGOS (European Community Seventh
Framework Programme (FP7/2007-2013)) for funding the field
experiment. Also, we would like to thank TTorch who supported the
author in an exchange stay at University of Tuscia (TTORCH ESF
Exchange Grant, part of the ESF “Tall Tower and Surface Research
Network for Verification of Climate Relevant Emissions of Human
Origin”-project). We would also like to thank the ESSReS Research
School, part of the Helmholtz Centre for Polar and Marine Research. We
thank Alessio Boschi, Michele Tomassucci and Sipko Bulthuis for their help during the
field experiment. Furthermore, we would like to thank Tommaso Chiti
for his help taking the soil samples, Stefano Ponziani for providing field data and
Annika Wieferich for her additional experiments in the laboratory. Thanks is also extended to the
two anonymous reviewers whose comments helped improve our manuscript.
<?xmltex \hack{\newline}?><?xmltex \hack{\newline}?>
The article processing charges for this open-access <?xmltex \hack{\newline}?> publication were covered by the University of Bremen.
<?xmltex \hack{\newline}?><?xmltex \hack{\newline}?>
Edited by: T. Keenan</p></ack><ref-list>
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