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<article xmlns:xlink="http://www.w3.org/1999/xlink" xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:oasis="http://docs.oasis-open.org/ns/oasis-exchange/table" xml:lang="en" dtd-version="3.0" article-type="research-article"><?xmltex \bartext{Research article}?>
  <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 Publications</publisher-name>
    <publisher-loc>Göttingen, Germany</publisher-loc>
  </publisher></journal-meta>
    <article-meta>
      <article-id pub-id-type="doi">10.5194/bg-19-3317-2022</article-id><title-group><article-title>Monitoring post-fire recovery of various vegetation biomes using
multi-wavelength satellite remote sensing</article-title><alt-title>Monitoring post-fire recovery of various vegetation biomes</alt-title>
      </title-group><?xmltex \runningtitle{Monitoring post-fire recovery of various vegetation biomes}?><?xmltex \runningauthor{E.~Bousquet et al.}?>
      <contrib-group>
        <contrib contrib-type="author" corresp="yes" rid="aff1">
          <name><surname>Bousquet</surname><given-names>Emma</given-names></name>
          <email>emma.bousquet@cerema.fr</email>
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Mialon</surname><given-names>Arnaud</given-names></name>
          
        <ext-link>https://orcid.org/0000-0001-7970-0701</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Rodriguez-Fernandez</surname><given-names>Nemesio</given-names></name>
          
        <ext-link>https://orcid.org/0000-0003-3796-149X</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2">
          <name><surname>Mermoz</surname><given-names>Stéphane</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Kerr</surname><given-names>Yann</given-names></name>
          
        <ext-link>https://orcid.org/0000-0001-6352-1717</ext-link></contrib>
        <aff id="aff1"><label>1</label><institution>Centre d'Etudes Spatiales de la Biosphère (CESBIO), Université
de Toulouse (CNES/CNRS/INRAE/IRD/UPS),<?xmltex \hack{\break}?> 18 av. Edouard Belin, bpi 2801, 31401
Toulouse CEDEX 9, France</institution>
        </aff>
        <aff id="aff2"><label>2</label><institution>GlobEO, 31400 Toulouse, France</institution>
        </aff>
      </contrib-group>
      <author-notes><corresp id="corr1">Emma Bousquet (emma.bousquet@cerema.fr)</corresp></author-notes><pub-date><day>15</day><month>July</month><year>2022</year></pub-date>
      
      <volume>19</volume>
      <issue>13</issue>
      <fpage>3317</fpage><lpage>3336</lpage>
      <history>
        <date date-type="received"><day>27</day><month>October</month><year>2021</year></date>
           <date date-type="rev-request"><day>11</day><month>November</month><year>2021</year></date>
           <date date-type="rev-recd"><day>27</day><month>May</month><year>2022</year></date>
           <date date-type="accepted"><day>23</day><month>June</month><year>2022</year></date>
      </history>
      <permissions>
        <copyright-statement>Copyright: © 2022 Emma Bousquet et al.</copyright-statement>
        <copyright-year>2022</copyright-year>
      <license license-type="open-access"><license-p>This work is licensed under the Creative Commons Attribution 4.0 International License. To view a copy of this licence, visit <ext-link ext-link-type="uri" xlink:href="https://creativecommons.org/licenses/by/4.0/">https://creativecommons.org/licenses/by/4.0/</ext-link></license-p></license></permissions><self-uri xlink:href="https://bg.copernicus.org/articles/19/3317/2022/bg-19-3317-2022.html">This article is available from https://bg.copernicus.org/articles/19/3317/2022/bg-19-3317-2022.html</self-uri><self-uri xlink:href="https://bg.copernicus.org/articles/19/3317/2022/bg-19-3317-2022.pdf">The full text article is available as a PDF file from https://bg.copernicus.org/articles/19/3317/2022/bg-19-3317-2022.pdf</self-uri>
      <abstract><title>Abstract</title>

      <p id="d1e127">Anthropogenic climate change is now considered to be one
of the main factors causing an increase in both the frequency and severity of
wildfires. These fires are prone to release substantial quantities of
CO<inline-formula><mml:math id="M1" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> into the atmosphere and to endanger natural ecosystems and
biodiversity. Depending on the ecosystem and climate regime, fires have
distinct triggering factors and impacts. To better analyse this phenomenon,
we investigated post-fire vegetation anomalies over different biomes, from
2012 to 2020. The study was performed using several remotely sensed
quantities ranging from visible–infrared vegetation indices (the enhanced
vegetation index (EVI)) to vegetation opacities obtained at several passive-microwave wavelengths (X-band, C-band, and L-band vegetation optical depth
(X-VOD, C-VOD, and L-VOD)), ranging from 2 to 20 cm. It was found that C-
and X-VOD are mostly sensitive to fire impact on low-vegetation areas (grass
and shrublands) or on tree leaves, while L-VOD depicts the fire
impact on tree trunks and branches better. As a consequence, L-VOD is probably a
better way of assessing fire impact on biomass. The study shows that L-VOD
can be used to monitor fire-affected areas as well as post-fire recovery,
especially over densely vegetated areas.</p>
  </abstract>
    </article-meta>
  </front>
<body>
      

<sec id="Ch1.S1" sec-type="intro">
  <label>1</label><title>Introduction</title>
      <p id="d1e148">Fires are a natural part of many ecosystems, being historically triggered by
lightning strikes (de Groot et al., 2013). Nevertheless, most wildfires are
now ignited by human activities (95 % in the Mediterranean basin, 85 %
in Asia and South America; FAO, 2006). In recent years, and in spite of
various efforts, wildfires were proven to increase both in frequency and in
severity worldwide, largely due to anthropogenic climate change and human
pressure (Weber and Stocks, 1998; Jin et al., 2012). The 2020 fire season
became historically significant in southern Australia and in the western United States,
linked with extreme vegetation dryness (Higuera and Abatzoglou, 2020).
Summer 2021 saw an unprecedented number of fires around the Mediterranean
Sea, in Siberia, and in North America (CAMS, 2021). In tropical rainforests,
the Amazon in particular, wildfires have become increasingly prevalent over
the past decades due not only to more frequent droughts and periodic El Niño
events (Aragão et al., 2018; Chen et al., 2013; Cochrane, 2003) but
also to selective logging and deforestation that lead to forest desiccation
and reduce rainfall (Asner et al., 2010).</p>
      <p id="d1e151">Wildfire likelihood factors were categorized into climatic (e.g. precipitation, temperature, air humidity, wind speed), topographic, in situ,
historical, and anthropogenic factors (Mhawej et al., 2015). Drought, i.e. the concomitant increase in air dryness and decrease in soil moisture, was
identified as the most significant fire likelihood factor (Ray et al.,
2005). Indirectly, drought also causes vegetation drying, leaf shedding, and
branch losses, which increase forest flammability (Nepstad et al., 2001;
Chuvieco et al., 2012). Surveying the soil moisture (SM) and the vegetation
water content (VWC) could then be a good indicator for fire risk detection,
and passive-microwave remote sensing is a useful tool for that. Indeed, the
SM deficit monitored with AMSR-E (Advanced Microwave Scanning Radiometer for EOS (Earth Observing System)) was previously proven to be a major factor for the evolution of extreme fire events in Siberia (Forkel et al.,
2012). GRACE-assimilated (Gravity Recovery and Climate Experiment) SM was also exploited for fire risk assessment in
the United States (Jensen et al., 2018; Farahmand et al., 2020). SMOS (Soil Moisture and Ocean Salinity) SM
anomalies have been found to explain singular fire episodes in the
north-western Iberian Peninsula (Chaparro et al., 2016) and in Canada
(Ambadan et al., 2020). SMOS SM has been used as an alternative source of
moisture information in the McArthur Forest Fire Danger Index (FFDI; Holgate
et al., 2017). Finally, AMSR-E vegetation optical depth (VOD) was
successfully used in data-driven fire models (Forkel et al., 2017;
Kuhn-Régnier et al., 2021).</p>
      <p id="d1e154">In addition to endangering populations, wildlife, and ecosystems and to
releasing overwhelming quantities of CO<inline-formula><mml:math id="M2" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> into the atmosphere (CAMS, 2021),
wildfires have several negative effects on soil and vegetation properties.
They cause deterioration of soil structure and porosity, ash entrapment,
removal of organic matter and nutrients, decrease of microbial and
invertebrate communities, etc. (Certini, 2005). Plant cover removal also
increases soil water repellency and runoff, which can lead to floods and
erosion (Shakesby and Doerr, 2005). Post-fire vegetation regeneration highly
depends on the ecosystem and on the fire severity (Chu and Guo, 2013). In
humid tropical forests, the Amazon in particular, wildfires can
significantly reduce above-ground biomass (AGB) for decades by amplifying
tree mortality (Barlow et al., 2003; Silva et al., 2018; de Faria et al.,
2021). Conversely, some ecosystems can recover much faster. For instance,
some coniferous trees (e.g. jack pine, black spruce) evolved to become fire
resistant and to use the flames as a means for spreading their seeds, as the
heat causes the opening of cones (Weber and Stocks, 1998). Some eucalyptus
communities of south-east Australia are also able to survive fire by
activating dormant vegetative buds to produce regrowth (Heath et al., 2016).
In savannas, recurrent seasonal fires help maintain the structure,
species composition, and biological diversity (Menaut et al., 1990). In
forests, prescribed burning enables the reduction of hazardous accumulations of
fuel and thus mitigates the severity of wildfires (Sackett, 1975). Fires
can even be necessary for canopy regeneration: a decline in sequoia
population was observed when fires were suppressed in California (Parsons
and DeBenedetti, 1979). Vegetation can thus recover from fire, and if plants
succeed in promptly recolonizing the burned area, the pre-fire level of most
properties can be recovered and even enhanced (Certini, 2005).</p>
      <p id="d1e166">It is essential to monitor post-fire vegetation conditions, and satellite
remote sensing proved its ability to achieve this goal in addition to
field campaigns (Chu and Guo, 2013). Indicators and metrics based on
multispectral satellite imagery (visible and infrared) are the most
frequently used, such as the normalized difference vegetation index (NDVI),
the enhanced vegetation index (EVI), and the normalized burn ratio (NBR)
(Pérez-Cabello et al., 2021). Despite a quick saturation over dense
forests, they still provide a good proxy for green vegetation regrowth.
Microwave data have also shown a good potential to monitor post-fire
recovery. L-band SAR (synthetic-aperture radar) was used to assess forest regrowth in South-East Asia
(Mermoz and Le Toan, 2016) and to estimate the tree survival in eucalyptus
forests of Western Australia (Fernandez-Carrillo et al., 2019). C-band VOD
was used to analyse the Amazon canopy dynamics during the 2019 fire season
(Zhang et al., 2021). Authors found a lower magnitude of canopy damage and a
longer recovery period for C-VOD than for optical-based indices (NDVI, EVI,
NBR). Indeed, the optical-based indices only represent the canopy greenness,
whereas microwave measurements are more sensitive to woody components
(Guglielmetti et al., 2007; Frappart et al., 2020). Microwave VODs are also
sensitive to VWC and can help to monitor the biomass status (Fan et al.,
2018; Konings et al., 2019).</p>
      <p id="d1e170">With the arrival of L-band radiometers such as the SMOS satellite, it is now possible to infer surface soil
moisture, biomass (i.e. fuel), and its water content at deeper sensing depth.
The rationale for this study is to investigate how L-band radiometry responds
to fire events in various ecosystems and climates. The SMOS satellite has
been operating for over 12 years now, and we have access to a large catalogue
of major fires. This study also presents for the first time L-VOD used in
conjunction with other sensors, from visible-infrared (EVI) to microwave X-
and C-VOD, for the study of post-fire vegetation recovery. The
complementarity of these vegetation variables along with climate variables
(air temperature (<inline-formula><mml:math id="M3" display="inline"><mml:mi>T</mml:mi></mml:math></inline-formula>), precipitation (<inline-formula><mml:math id="M4" display="inline"><mml:mi>P</mml:mi></mml:math></inline-formula>), soil moisture (SM), and terrestrial
water storage (TWS)) was used to identify the fire likelihood factors and
the immediate and long-term fire impact on vegetation. To evaluate the
long-term impact and recovery, the study focused on areas with unique fire
events, thereby excluding areas with regular seasonal fires (e.g. the
Sahel) where the vegetation cannot fully recover before the following fire
event. We first observed three particular cases of large fires and then
extended the analysis to different biomes.</p>
</sec>
<sec id="Ch1.S2">
  <label>2</label><title>Data</title>
<sec id="Ch1.S2.SS1">
  <label>2.1</label><title>Fires</title>
      <p id="d1e202">Fires were obtained from the National Aeronautics and Space Administration
(NASA) Moderate Resolution Imaging Spectroradiometer (MODIS) active fire
product (MOD14A1_M). The product is a quantification of the
number of fires observed within a 1000 km<inline-formula><mml:math id="M5" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:math></inline-formula> area over a month.
A fire must cover at least <inline-formula><mml:math id="M6" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 1000 m<inline-formula><mml:math id="M7" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:math></inline-formula> to be
detected and must not be covered by clouds, heavy smoke, or tree canopy
(Giglio et al., 2020). The active fire product is based on the 1 km fire
channels at 3.9 and 11 <inline-formula><mml:math id="M8" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi></mml:mrow></mml:math></inline-formula>m of the MODIS Terra and Aqua satellites (Justice
et al., 2006). It is distributed at 0.1<inline-formula><mml:math id="M9" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> resolution and at a monthly timescale by the NASA Earth Observations (NEO) portal.</p><?xmltex \hack{\newpage}?>
</sec>
<sec id="Ch1.S2.SS2">
  <label>2.2</label><title>Precipitation</title>
      <p id="d1e256">Precipitation (<inline-formula><mml:math id="M10" display="inline"><mml:mi>P</mml:mi></mml:math></inline-formula>) data come from the Precipitation Estimation from Remotely
Sensed Information using Artificial Neural Networks–Climate Data Record
(PERSIANN-CDR). The precipitation estimate uses the PERSIANN algorithm on
GridSat-B1 infrared satellite data and training of the artificial neural
network on the National Centers for Environmental Prediction (NCEP) hourly
precipitation data (Ashouri et al., 2015). The dataset is distributed by the
National Oceanic and Atmospheric Administration (NOAA) at a daily timescale and at 0.25<inline-formula><mml:math id="M11" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> resolution in the latitude band 60<inline-formula><mml:math id="M12" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> S–60<inline-formula><mml:math id="M13" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N.</p>
</sec>
<sec id="Ch1.S2.SS3">
  <label>2.3</label><title>Soil moisture</title>
      <p id="d1e301">The soil moisture (SM) dataset comes from the SMOS satellite, launched by
the European Space Agency (ESA) in 2009 (Kerr et al., 2001). It performs
passive measurements of the thermal emission of Earth at the L band (1.4 GHz, 21 cm). L-band VOD and SM are derived from SMOS brightness temperatures
using the L-band Microwave Emission of the Biosphere (L-MEB) radiative
transfer model (Wigneron et al., 2007; Kerr et al., 2012). L-band SM is the
volume of water per volume of soil (m<inline-formula><mml:math id="M14" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msup></mml:math></inline-formula> m<inline-formula><mml:math id="M15" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>) in the top surface
soil layer (<inline-formula><mml:math id="M16" display="inline"><mml:mo lspace="0mm">∼</mml:mo></mml:math></inline-formula> 5 cm). The footprint size is <inline-formula><mml:math id="M17" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 43 km on average (Kerr et al., 2010). We considered the ESA Level 2 SM dataset
in version 7.2 (L2 v720) resampled to the global cylindrical Equal-Area
Scalable Earth (EASE) Grid version 2.0 (Brodzik et al., 2012) at 625 km<inline-formula><mml:math id="M18" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:math></inline-formula> spatial sampling (25 km <inline-formula><mml:math id="M19" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 25 km at 30<inline-formula><mml:math id="M20" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> of
latitude). Ascending (06:00) and descending (18:00) overpasses were averaged,
from June 2010 to December 2020.</p>
</sec>
<sec id="Ch1.S2.SS4">
  <label>2.4</label><title>Terrestrial water storage</title>
      <p id="d1e373">Terrestrial water storage (TWS) anomalies from the Gravity Recovery and
Climate Experiment (GRACE) satellite were also considered. We used the monthly
GRACE/GRACE-FO (Follow-On) Level 3 product provided through the Gravity
Information Service (GravIS) web portal of the German Research Centre for
Geosciences (GFZ) at 1<inline-formula><mml:math id="M21" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> latitude–longitude grids (Boergens et al., 2019).
TWS anomalies (cm) represent the water mass anomalies from snow, surface
water, soil moisture, and deep groundwater. They are derived from
measurements of temporal changes in Earth's gravity field. Data were
lacking for 35 months  in the 10-year dataset. One-time gaps were filled by
linear interpolation; consecutive missing months were not considered
(September–November 2016, July 2017–May 2018, and August–October 2018; 17 months in
total).</p>
</sec>
<sec id="Ch1.S2.SS5">
  <label>2.5</label><title>Temperature</title>
      <p id="d1e394">Temperature (<inline-formula><mml:math id="M22" display="inline"><mml:mi>T</mml:mi></mml:math></inline-formula>) data come from the land surface temperature (LST) dataset
from the MODIS Terra satellite (NASA). Daytime and nighttime measurements were
averaged (MOD11C3 Version 6 product in the Climate Modeling Grid (CMG),
LST_Day_CMG, and LST_Night_CMG; Wan et al., 2015). These datasets are obtained
using MODIS thermal infrared bands from 3 to 15 <inline-formula><mml:math id="M23" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi></mml:mrow></mml:math></inline-formula>m and distributed by
the NASA Land Processes Distributed Active Archive Center (LP DAAC) at a monthly
timescale and at 0.05<inline-formula><mml:math id="M24" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> resolution.</p>
</sec>
<sec id="Ch1.S2.SS6">
  <label>2.6</label><title>Vegetation optical depth</title>
      <p id="d1e429">Vegetation optical depth (VOD) is a remotely sensed indicator related to AGB
and to VWC (Kerr and Njoku, 1990; Jackson and Schmugge, 1991; Jones et al.,
2011; Rahmoune et al., 2014; Vittucci et al., 2016; Rodriguez-Fernandez et
al., 2018; Mialon et al., 2020). No clear approach exists for disentangling
the contributions of AGB and VWC in the VOD because of the co-sensitivity of
microwave observables to both quantities (Konings et al., 2019). The lower
frequencies have better capabilities of penetrating deeper within the canopy
(Ulaby et al., 1981). At the L band, VOD is sensitive to coarse woody elements,
such as trunks, stems, and branches. At the C and X bands, VOD is more sensitive
to thin stems and leaves (Guglielmetti et al., 2007). L-VOD is then more
sensitive than higher-frequency VODs to high AGB values and is a good proxy
for dense vegetation (Rodriguez-Fernandez et al., 2018). In this paper,
L-VOD comes from the SMOS Level 2 dataset in version 7.2 (L2 v720) measured at
1.4 GHz (<inline-formula><mml:math id="M25" display="inline"><mml:mrow><mml:mi mathvariant="italic">λ</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">21</mml:mn></mml:mrow></mml:math></inline-formula> cm), resampled to EASE-Grid 2.0 at 625 km<inline-formula><mml:math id="M26" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:math></inline-formula> resolution (25 km <inline-formula><mml:math id="M27" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 25 km at 30<inline-formula><mml:math id="M28" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> of
latitude). In the SMOS retrieval algorithm, the vegetation attenuation is
taken into account by the <inline-formula><mml:math id="M29" display="inline"><mml:mi mathvariant="italic">τ</mml:mi></mml:math></inline-formula> parameter of the <inline-formula><mml:math id="M30" display="inline"><mml:mrow><mml:mi mathvariant="italic">τ</mml:mi><mml:mo>-</mml:mo><mml:mi mathvariant="italic">ω</mml:mi></mml:mrow></mml:math></inline-formula>
model (Mo et al., 1982), which corresponds to the L-VOD. Data from June 2010
to December 2020 were considered, and ascending (06:00) and descending (18:00)
overpasses were averaged. C- and X-VOD from the Japan Aerospace Exploration
Agency (JAXA) Global Change Observation Mission (GCOM) Advanced Microwave
Scanning Radiometer 2 (AMSR2) dataset were also considered (Imaoka et al.,
2010). C- and X-VOD are measured at 6.9 GHz (<inline-formula><mml:math id="M31" display="inline"><mml:mrow><mml:mi mathvariant="italic">λ</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">4.3</mml:mn></mml:mrow></mml:math></inline-formula> cm) and 10.7 GHz (<inline-formula><mml:math id="M32" display="inline"><mml:mrow><mml:mi mathvariant="italic">λ</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">2.8</mml:mn></mml:mrow></mml:math></inline-formula> cm) respectively. The C2 band (7.3 GHz, <inline-formula><mml:math id="M33" display="inline"><mml:mrow><mml:mi mathvariant="italic">λ</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">4.1</mml:mn></mml:mrow></mml:math></inline-formula> cm) was not discussed in this paper, as the data were mostly redundant
with the C1 band (6.9 GHz). We used the daily L3 V001 VOD products, from July 2012 to December 2020, processed with the land parameter retrieval model
(LPRM) algorithm (Owe et al., 2008) and distributed by NASA on a regular
grid at 25 km <inline-formula><mml:math id="M34" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 25 km resolution. Ascending (13:30) and
descending (01:30) overpasses (LPRM_AMSR2_A_SOILM3 and LPRM_AMSR2_D_SOILM3) were averaged.</p>
</sec>
<sec id="Ch1.S2.SS7">
  <label>2.7</label><title>Enhanced vegetation index</title>
      <p id="d1e540">VOD values were compared with the visible–near-infrared-based enhanced
vegetation index (EVI) from MODIS (NASA) MOD13C2 and MYD13C2 Version 6 for
the Aqua and Terra Satellites respectively, distributed at 5600 m resolution
(Didan, 2015). EVI represents canopy greenness, with an improved sensitivity
over high-AGB regions compared to NDVI. It is obtained by combining
measurements at red (<inline-formula><mml:math id="M35" display="inline"><mml:mrow><mml:mi mathvariant="italic">λ</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0.6</mml:mn></mml:mrow></mml:math></inline-formula>–0.7 <inline-formula><mml:math id="M36" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi></mml:mrow></mml:math></inline-formula>m, <inline-formula><mml:math id="M37" display="inline"><mml:mi>f</mml:mi></mml:math></inline-formula> <inline-formula><mml:math id="M38" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 460 THz) and near-infrared wavelengths (<inline-formula><mml:math id="M39" display="inline"><mml:mrow><mml:mi mathvariant="italic">λ</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0.7</mml:mn></mml:mrow></mml:math></inline-formula>–1.1 <inline-formula><mml:math id="M40" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi></mml:mrow></mml:math></inline-formula>m, <inline-formula><mml:math id="M41" display="inline"><mml:mi>f</mml:mi></mml:math></inline-formula> <inline-formula><mml:math id="M42" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 330 THz).</p>
</sec>
<sec id="Ch1.S2.SS8">
  <label>2.8</label><title>Auxiliary data</title>
<sec id="Ch1.S2.SS8.SSS1">
  <label>2.8.1</label><title>Year of gross forest cover loss event</title>
      <p id="d1e627">The year of gross forest cover loss event map (the so-called lossyear
product) from Hansen et al. (2013) was used to observe the forest loss rate
and year within a SMOS pixel, for the three major fires studied (Fig. 2).
This map represents the first year of detected tree loss during the period
2000–2020, defined as a stand-replacement disturbance or a change from a
forest to non-forest state. This dataset is based on Landsat images and is
distributed at <inline-formula><mml:math id="M43" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 30 m resolution with <inline-formula><mml:math id="M44" display="inline"><mml:mrow><mml:mn mathvariant="normal">10</mml:mn><mml:mo>×</mml:mo><mml:mn mathvariant="normal">10</mml:mn></mml:mrow></mml:math></inline-formula> square degree
tiles at <uri>https://glad.earthengine.app/view/global-forest-change</uri> (last access: 1 October 2021). Each year
of the period 2010–2020 was extracted from the forest loss product and
averaged into SMOS EASE-Grid 2.0 so as to obtain a yearly percentage of
forest loss.</p>
</sec>
<sec id="Ch1.S2.SS8.SSS2">
  <label>2.8.2</label><title>Land cover</title>
      <p id="d1e660">A land surface climatology map based on 10 years (2001–2010) of the MODIS
MCD12Q1 product at 500 m resolution (Broxton et al., 2014) was used to
filter the data and to distinguish four different vegetation types (see
Sect. 3). This land cover map identifies 17 ecosystems based on the
IGBP (International Geosphere-Biosphere Programme) class labels.</p>
</sec>
<sec id="Ch1.S2.SS8.SSS3">
  <label>2.8.3</label><title>Above-ground biomass</title>
      <p id="d1e671">The global map of AGB (Mg ha<inline-formula><mml:math id="M45" 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>) from Santoro et al. (2021) was used to
distinguish sparse from dense forests (see Sect. 3.3). This map is
distributed through the ESA Climate Change Initiative (CCI) Biomass at 100 m
resolution. It combines a large pool of spaceborne remote sensing
observations from two SAR missions (Envisat and
ALOS (Advanced Land Observing Satellite)) and uses optical (Landsat) and lidar (ICESat (Ice, Cloud, and land Elevation) GLAS (Geoscience Laser Altimeter System)) data to support
the model calibration procedure. The ESA CCI Biomass map representative of
2010 was used here because it provides AGB information prior to the
studied fire events (2011–2020).</p>
</sec>
<sec id="Ch1.S2.SS8.SSS4">
  <label>2.8.4</label><title>Snow and ice</title>
      <p id="d1e694">The Interactive Multisensor Snow and Ice Mapping System (IMS) database was
used to mask areas covered with snow or ice (see Sect. 3.1). We used the IMS
Daily Northern Hemisphere Snow and Ice Analysis at 4 km resolution, version 1 (Helfrich et al., 2007), provided by the National Snow and Ice Data Center
(NSIDC).</p>
</sec>
<sec id="Ch1.S2.SS8.SSS5">
  <label>2.8.5</label><title>Flooding</title>
      <p id="d1e706">Flooded areas were filtered out (see Sect. 3.1) based on the Global
Inundation Estimate from Multiple Satellites (GIEMS-2) dataset (Prigent et
al., 2019). It provides long-term monthly estimates of surface water extent,
including open water, wetlands, and rice paddies. The methodology combines
passive- and active-microwave, visible, and near-infrared observations
(SSM/I (Special Sensor Microwave/Imager), ERS (European Remote Sensing), AVHRR (Advanced Very High Resolution Radiometer)). The water fraction is delivered globally from 1992 to
2015, on an equal area grid of 0.25<inline-formula><mml:math id="M46" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M47" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 0.25<inline-formula><mml:math id="M48" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> at the Equator
(<inline-formula><mml:math id="M49" display="inline"><mml:mo lspace="0mm">∼</mml:mo></mml:math></inline-formula> 28 km <inline-formula><mml:math id="M50" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 28 km). Flooded areas were detected with a
climatology over the 1992–2015 period.</p>
</sec>
<sec id="Ch1.S2.SS8.SSS6">
  <label>2.8.6</label><title>Topography</title>
      <p id="d1e756">Strong topographies were also filtered out for this study (see Sect. 3.1).
They were flagged using a mask created for the SMOS retrieval (Mialon et
al., 2008) based on a digital elevation model (DEM) provided by the Shuttle
Radar Topography Mission (SRTM), a joint project between the National
Aeronautics and Space Administration (NASA) and the National
Geospatial-Intelligence Agency (NGA), conducted in 2000 (Jarvis et al.,
2006).</p>
</sec>
</sec>
</sec>
<sec id="Ch1.S3">
  <label>3</label><title>Methods</title>
      <p id="d1e769">First, we investigated three various regions which recently experienced
severe fires. These areas consist in (i) a eucalyptus open forest in a
human-affected environment, under dry El Niño conditions in Australia;
(ii) a mixed area of needleleaf forests, woody savannas, and human activities
under a Mediterranean climate in California; and (iii) a remote primary
rainforest in a tropical wet climate in Amazonia (see Sect. 3.2). Second,
the study was extended to the ecosystem scale, for five vegetation types, by
selecting the major fires of the last decade (see Sect. 3.3). The rationale
was to capture significant and unique events occurring over an area large
enough to be observed with the SMOS satellite without any ambiguity. Four
climate variables related to the fire risk were considered: precipitation,
SM, TWS, and temperature. Wind is another predominant fire likelihood factor
(Albini, 1993) but was not studied here due to the lack of reliable data at
the required spatiotemporal scale. Vegetation status before, during, and
after fire was monitored with four vegetation variables: EVI, X-VOD, C-VOD,
and L-VOD.</p><?xmltex \hack{\newpage}?>
<sec id="Ch1.S3.SS1">
  <label>3.1</label><title>Data preprocessing</title>
      <p id="d1e780">Data from June 2010 to December 2020 were considered (10.5 years), except
for C- and X-VOD from AMSR2 which were only available from July 2012.
Monthly averages of all datasets were computed and resampled to SMOS
EASE-Grid 2.0 (<inline-formula><mml:math id="M51" display="inline"><mml:mo lspace="0mm">∼</mml:mo></mml:math></inline-formula> 25 km resolution) with a weighted average
interpolation, using GDAL (Geospatial Data Abstraction Library) (GDAL/OGR contributors, 2020). SMOS data (SM and
L-VOD) were filtered from RFI (radio frequency interference) impacts by using a 20 % maximum threshold on
the RFI probability, provided by the SMOS Level 2 product. Only the centre part
of the swath was considered (less than 450 km away from the sub-satellite
track) so as to only use optimal retrievals. Microwave measurements were
also proven to be disturbed by strong topography (Mialon et al., 2008), snow
(Schwank et al., 2014), and standing water (Ye et al., 2015; Jones et al.,
2011; Bousquet et al., 2021). Hence, for all datasets, we removed strong-topography areas based on the SMOS topography mask, snow-covered months based on the
IMS database (20 % maximum snow coverage), water-contaminated areas based
on the land cover map (50 % maximum water fraction), and flooded ones
based on GIEMS-2 climatology (20 % maximum water fraction).</p>
</sec>
<sec id="Ch1.S3.SS2">
  <label>3.2</label><title>Case study: analysis of three major fires</title>
<sec id="Ch1.S3.SS2.SSS1">
  <label>3.2.1</label><title>Wildfires on the South Coast of New South Wales in Australia</title>
      <p id="d1e805">The first studied area is located on the South Coast of New South Wales in
Australia at 33.53–37.72<inline-formula><mml:math id="M52" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> S, 149.40–150.17<inline-formula><mml:math id="M53" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E (Fig. 1) and covers 13 SMOS pixels. The dominant vegetation type is eucalyptus open forest (McColl,
1969; DEWR, 2007). The climate is warm temperate with dry summers (Kottek et
al., 2006). The mean rainfall is <inline-formula><mml:math id="M54" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 1000 mm yr<inline-formula><mml:math id="M55" 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>, and
the mean temperature is <inline-formula><mml:math id="M56" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 15<inline-formula><mml:math id="M57" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> C (McColl, 1969). The
topography varies between 0 and 600 m above sea level. The 2019–2020
wildfires in Australia were influenced by the El Niño Southern Oscillation
(Dowdy, 2018). They became historically significant, as they were widespread
and extremely severe, in particular in New South Wales (Ehsani et al.,
2020). The tree cover loss map (Hansen et al., 2013) indicates a 25 %
forest loss in 2020 in the studied area (Fig. 2).</p>
</sec>
<sec id="Ch1.S3.SS2.SSS2">
  <label>3.2.2</label><title>Mendocino Complex Fire in California</title>
      <p id="d1e870">The second studied area is located in California, near Lakeport, at
38.96–39.46<inline-formula><mml:math id="M58" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N, 122.68–123.20<inline-formula><mml:math id="M59" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> W (Fig. 1). It corresponds to four SMOS pixels. The area
is covered with evergreen needleleaf forest and woody savannas (Broxton et
al., 2014) and is very urbanized. The climate is warm temperate (Kottek et
al., 2006), with dry, windy, and often hot weather conditions from spring
through late autumn that can produce severe wildfires (Crockett and
Westerling, 2018). The 2018 fire season was the most extreme on record in
northern California (now second to the 2020 fire season) in terms of number
of fatalities, destroyed structures, and burned areas (Brown et al., 2020).
The Mendocino Complex is the largest fire complex in state history and
burned nearly 1860 km<inline-formula><mml:math id="M60" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:math></inline-formula> of vegetation between July and September 2018.
It included two wildfires: the Ranch Fire in the north, which was the
largest single fire in state history and burned 1660 km<inline-formula><mml:math id="M61" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:math></inline-formula>, and the River
Fire in the west, which burned 198 km<inline-formula><mml:math id="M62" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:math></inline-formula> (BLM, 2018). The Mendocino
Complex caused a 34 % vegetation loss in this region (26 % in 2018 and
8 % in 2019, Fig. 2) and was predominantly classified as moderate
severity (62 %; BLM, 2018).</p>
</sec>
<sec id="Ch1.S3.SS2.SSS3">
  <label>3.2.3</label><title>Santarém wildfire in the Amazon</title>
      <p id="d1e926">The third studied area is located in the Amazon rainforest near the city of Santarém
(Brazil) at 3.14–2.75<inline-formula><mml:math id="M63" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> S, 53.95–54.13<inline-formula><mml:math id="M64" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> W (Fig. 1) and covers two SMOS
pixels. The evergreen broadleaf forest is dense (L-VOD <inline-formula><mml:math id="M65" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 1.02; AGB <inline-formula><mml:math id="M66" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 280 Mg ha<inline-formula><mml:math id="M67" 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> on average over the area). The climate is hot and humid, with
an annual mean temperature of 25<inline-formula><mml:math id="M68" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> C and mean precipitation of 1920 mm yr<inline-formula><mml:math id="M69" 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> (Berenguer et al., 2018). During the strong El Niño event in
December 2015, a severe drought caused large fires in this area, with no
link to anthropic deforestation (Berenguer et al., 2018). They induced a
20 % forest loss in 2016 in the studied area (Fig. 2).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F1" specific-use="star"><?xmltex \currentcnt{1}?><?xmltex \def\figurename{Figure}?><label>Figure 1</label><caption><p id="d1e997">Global maps of SMOS L-VOD (left) and SM (right), with averages for
2011–2020. The red dots show the locations of the three areas of interest:
the Mendocino Complex in California, Santarém in Amazonia, and the South
Coast of New South Wales in Australia.</p></caption>
            <?xmltex \igopts{width=503.61378pt}?><graphic xlink:href="https://bg.copernicus.org/articles/19/3317/2022/bg-19-3317-2022-f01.png"/>

          </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F2" specific-use="star"><?xmltex \currentcnt{2}?><?xmltex \def\figurename{Figure}?><label>Figure 2</label><caption><p id="d1e1008">Yearly forest loss (%) attributed to the three burned areas
under study, from the Hansen et al. (2013) “lossyear” product.</p></caption>
            <?xmltex \igopts{width=503.61378pt}?><graphic xlink:href="https://bg.copernicus.org/articles/19/3317/2022/bg-19-3317-2022-f02.png"/>

          </fig>

</sec>
<sec id="Ch1.S3.SS2.SSS4">
  <label>3.2.4</label><title>Anomaly time series computation</title>
      <p id="d1e1025">Anomaly time series of EVI; X-, C-, and L-VOD; <inline-formula><mml:math id="M70" display="inline"><mml:mi>P</mml:mi></mml:math></inline-formula>; SM; TWS; and <inline-formula><mml:math id="M71" display="inline"><mml:mi>T</mml:mi></mml:math></inline-formula> were plotted
over the three studied sites. The anomaly (anom) time series of a variable <inline-formula><mml:math id="M72" display="inline"><mml:mi>x</mml:mi></mml:math></inline-formula> is the
difference between the original time series and the mean climatology, which
is the mean seasonal cycle of this variable. They are defined as
              <disp-formula id="Ch1.E1" content-type="numbered"><label>1</label><mml:math id="M73" display="block"><mml:mrow><mml:mi mathvariant="normal">anom</mml:mi><mml:mfenced close=")" open="("><mml:mrow><mml:mi>x</mml:mi><mml:mfenced open="(" close=")"><mml:mi>t</mml:mi></mml:mfenced></mml:mrow></mml:mfenced><mml:mo>=</mml:mo><mml:mi>x</mml:mi><mml:mfenced open="(" close=")"><mml:mi>t</mml:mi></mml:mfenced><mml:mo>-</mml:mo><mml:mi mathvariant="normal">climatology</mml:mi><mml:mfenced close=")" open="("><mml:mrow><mml:mi>x</mml:mi><mml:mfenced open="(" close=")"><mml:mi>m</mml:mi></mml:mfenced></mml:mrow></mml:mfenced></mml:mrow></mml:math></disp-formula>
            and
              <disp-formula id="Ch1.E2" content-type="numbered"><label>2</label><mml:math id="M74" display="block"><mml:mtable rowspacing="0.2ex" class="split" displaystyle="true" columnalign="right left"><mml:mtr><mml:mtd><mml:mrow><mml:mi mathvariant="normal">climatology</mml:mi><mml:mfenced open="(" close=")"><mml:mrow><mml:mi>x</mml:mi><mml:mfenced close=")" open="("><mml:mrow><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mi>m</mml:mi></mml:mrow></mml:mfenced></mml:mrow></mml:mfenced></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mn mathvariant="normal">1</mml:mn><mml:mrow><mml:msub><mml:mi>y</mml:mi><mml:mi>n</mml:mi></mml:msub></mml:mrow></mml:mfrac></mml:mstyle><mml:msubsup><mml:mo>∑</mml:mo><mml:mrow><mml:mi>y</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow><mml:mrow><mml:msub><mml:mi>y</mml:mi><mml:mi>n</mml:mi></mml:msub></mml:mrow></mml:msubsup><mml:mi>x</mml:mi><mml:mfenced open="(" close=")"><mml:mrow><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mi>m</mml:mi><mml:mo>+</mml:mo><mml:mfenced close=")" open="("><mml:mrow><mml:mi>y</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:mfenced><mml:mo>⋅</mml:mo><mml:mn mathvariant="normal">12</mml:mn></mml:mrow></mml:mfenced><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd><mml:mrow><?xmltex \igopts{width=5.690551pt}?><mml:mstyle background="https://bg.copernicus.org/articles/19/3317/2022/bg-19-3317-2022-g01.png"/><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mi>m</mml:mi></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:mo>=</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mo>-</mml:mo><mml:mn mathvariant="normal">12</mml:mn></mml:mrow></mml:mtd></mml:mtr></mml:mtable></mml:math></disp-formula>
            where <inline-formula><mml:math id="M75" display="inline"><mml:mi>t</mml:mi></mml:math></inline-formula> is the month number from January 2010 (6 to 132 in this study); <inline-formula><mml:math id="M76" display="inline"><mml:mi>m</mml:mi></mml:math></inline-formula> is
the month of the year, between 1 and 12, with <inline-formula><mml:math id="M77" display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>=</mml:mo></mml:mrow></mml:math></inline-formula> (<inline-formula><mml:math id="M78" display="inline"><mml:mrow><mml:mi>t</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:math></inline-formula> mod 12) <inline-formula><mml:math id="M79" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> 1; and <inline-formula><mml:math id="M80" display="inline"><mml:mi>y</mml:mi></mml:math></inline-formula>
is the year number, from 1 to <inline-formula><mml:math id="M81" display="inline"><mml:mrow><mml:msub><mml:mi>y</mml:mi><mml:mi>n</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, with <inline-formula><mml:math id="M82" display="inline"><mml:mrow><mml:msub><mml:mi>y</mml:mi><mml:mi>n</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn mathvariant="normal">11</mml:mn></mml:mrow></mml:math></inline-formula> here, as the
climatology is computed for the period 2010–2020. Plotting the anomaly time
series enables the removal of the natural seasonal cycle so as to observe only
the variations due to specific events. The average pre-fire variable value
was subtracted from the anomaly time series, only if at least 12 months
of data were available before the fire event. It enables the observation of the
anomalies with respect to the pre-disturbance value. The time series of the
number of fires were plotted in absolute values.</p>
</sec>
</sec>
<sec id="Ch1.S3.SS3">
  <label>3.3</label><title>Extension to the ecosystem scale</title>
      <p id="d1e1261">Fires were then studied at the ecosystem scale to assess the general factors
and impacts of fire according to the specific features of each biome (Fig. 3). Five land cover classes were studied: grasslands and croplands (IGBP
labels 10, 12, and 14), savannas and shrublands (IGBP labels 6, 7, 8, and
9), needleleaf forests (IGBP labels 1 and 3), sparse broadleaf forests (IGBP
labels 2 and 4; AGB <inline-formula><mml:math id="M83" display="inline"><mml:mo>≤</mml:mo></mml:math></inline-formula> 150 Mg ha<inline-formula><mml:math id="M84" 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>), and dense broadleaf forests
(IGBP labels 2 and 4; AGB <inline-formula><mml:math id="M85" display="inline"><mml:mi mathvariant="italic">&gt;</mml:mi></mml:math></inline-formula> 150 Mg ha<inline-formula><mml:math id="M86" 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>). Only the latitude
band 60<inline-formula><mml:math id="M87" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> S–60<inline-formula><mml:math id="M88" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N was retained in order to be
consistent with the precipitation dataset extent. Only the range July 2012–December 2020 was conserved here for all datasets so as to match with
AMSR2 time period. For fire event selection, the time range was reduced
from September 2013–October 2019 to avoid fire events occurring at the very
beginning (or end respectively) of the period to be able to study possible pre- and
post-fire anomalies. Only areas showing a unique and intense fire event over
the 6-year period were considered to properly observe the factors and
impacts of this event over a long time period without any other disturbance.
This excluded dry areas with regular seasonal fires, such as the Sahel
region. Two conditions were empirically defined as mandatory to select a
fire event over a given pixel: (i) a minimum number of fires of 5 at the
height of the fire and (ii) a maximum number of fires of 2.5 outside the period
(<inline-formula><mml:math id="M89" display="inline"><mml:mrow><mml:mo>±</mml:mo><mml:mn mathvariant="normal">6</mml:mn></mml:mrow></mml:math></inline-formula> months) around the main fire event to ensure that the vegetation
recovery is linked with the main fire event and is not affected by another
significant one. Anomalies were computed with Eqs. (1) and (2), with a
climatology over all dates excepted the year of the fire event, in order to
remove these exceptional values. The anomaly time series were then shifted
to collocate in time all fire events and averaged by ecosystem. To ensure
the spatial representativeness of each ecosystem, the months with a number
of available points lower than half the maximum number of points of the
ecosystem were filtered out from the shifted time series.</p>
      <p id="d1e1331">Pre-fire climatic anomalies and post-fire vegetation anomalies were also
aggregated at different timeframes and plotted, in order to compare their
temporal behaviour in different ecosystems. The standard error of the mean
of the measurements <inline-formula><mml:math id="M90" display="inline"><mml:mi mathvariant="italic">σ</mml:mi></mml:math></inline-formula> was also computed with Eq. (3):
            <disp-formula id="Ch1.E3" content-type="numbered"><label>3</label><mml:math id="M91" display="block"><mml:mrow><mml:mi mathvariant="italic">σ</mml:mi><mml:mfenced open="(" close=")"><mml:mi>p</mml:mi></mml:mfenced><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mi mathvariant="normal">SD</mml:mi><mml:mfenced close=")" open="("><mml:mi>p</mml:mi></mml:mfenced></mml:mrow><mml:msqrt><mml:mi>n</mml:mi></mml:msqrt></mml:mfrac></mml:mstyle><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>
          where SD is the standard deviation of the population <inline-formula><mml:math id="M92" display="inline"><mml:mi>p</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math id="M93" display="inline"><mml:mi>n</mml:mi></mml:math></inline-formula> is the number
of samples.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F3" specific-use="star"><?xmltex \currentcnt{3}?><?xmltex \def\figurename{Figure}?><label>Figure 3</label><caption><p id="d1e1383">Location of the selected fires and histograms of the fire dates,
for grasslands and croplands (IGBP labels 10, 12, and 14), savannas and
shrublands (IGBP labels 6, 7, 8, and 9), needleleaf forests (IGBP labels 1
and 3), sparse broadleaf forests (IGBP labels 2 and 4; AGB <inline-formula><mml:math id="M94" display="inline"><mml:mo>≤</mml:mo></mml:math></inline-formula> 150 Mg ha<inline-formula><mml:math id="M95" display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>, and dense broadleaf forests (IGBP labels 2 and 4; AGB <inline-formula><mml:math id="M96" display="inline"><mml:mi mathvariant="italic">&gt;</mml:mi></mml:math></inline-formula> 150 Mg ha<inline-formula><mml:math id="M97" display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>. Areas affected by water, snow, or strong
topography were excluded (see Sect. 3.1).</p></caption>
          <?xmltex \igopts{width=426.791339pt}?><graphic xlink:href="https://bg.copernicus.org/articles/19/3317/2022/bg-19-3317-2022-f03.png"/>

        </fig>

</sec>
</sec>
<sec id="Ch1.S4">
  <label>4</label><title>Results</title>
<sec id="Ch1.S4.SS1">
  <label>4.1</label><title>Case study: analysis of three major fires</title>
      <p id="d1e1452">In evergreen forests of the South Coast of New South Wales in Australia
(Fig. 4a), fires reached a maximum in January 2020 (mean number of fires <inline-formula><mml:math id="M98" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 8). They are associated with high temperature and low precipitation (anom(<inline-formula><mml:math id="M99" display="inline"><mml:mi>T</mml:mi></mml:math></inline-formula>) <inline-formula><mml:math id="M100" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M101" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula>3<inline-formula><mml:math id="M102" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> C, anom(<inline-formula><mml:math id="M103" display="inline"><mml:mi>P</mml:mi></mml:math></inline-formula>) <inline-formula><mml:math id="M104" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M105" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>80 mm). The drought started 3 years
before fire (decrease in precipitation, SM, and TWS). All vegetation data
exhibit the same pattern, which is (i) a constant and mild decrease since
2012, (ii) a strong decrease just before and during the fire event
(<inline-formula><mml:math id="M106" display="inline"><mml:mo lspace="0mm">∼</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M107" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>0.15), and (iii) a rapid post-fire recovery
(<inline-formula><mml:math id="M108" display="inline"><mml:mo lspace="0mm">∼</mml:mo></mml:math></inline-formula> 1 year). C-VOD is the most affected vegetation variable.</p>
      <p id="d1e1535">In California, no major pre-fire drought is visible in summer 2018
(Fig. 4b). The Mendocino Complex was the strongest of the three case
studies, with 20 fires observed on average in August 2018. It provoked a
decrease in all vegetation variables, particularly in L-VOD (anom(L-VOD) <inline-formula><mml:math id="M109" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M110" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>0.08) and in EVI (anom(EVI) <inline-formula><mml:math id="M111" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M112" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>0.10). Whereas C- and X-VOD regained
their pre-fire values rapidly (<inline-formula><mml:math id="M113" display="inline"><mml:mo lspace="0mm">∼</mml:mo></mml:math></inline-formula> 1 year), EVI and L-VOD did
not.</p>
      <p id="d1e1573">In the dense rainforest near Santarém (Brazilian Amazon), the number of
detected fires in December 2015 is quite low (<inline-formula><mml:math id="M114" display="inline"><mml:mo lspace="0mm">∼</mml:mo></mml:math></inline-formula> 4.5) (Fig. 4c), but this value may be underestimated because of cloud coverage (Giglio
et al., 2020). Vegetation variables are stable before the fire event, even
if the L-VOD signal is quite noisy because only two SMOS pixels were considered
here. Strong positive temperature anomalies (<inline-formula><mml:math id="M115" display="inline"><mml:mo lspace="0mm">+</mml:mo></mml:math></inline-formula>3<inline-formula><mml:math id="M116" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> C), negative
precipitation anomalies (<inline-formula><mml:math id="M117" display="inline"><mml:mo lspace="0mm">-</mml:mo></mml:math></inline-formula>160 mm), and TWS anomalies (<inline-formula><mml:math id="M118" display="inline"><mml:mo lspace="0mm">-</mml:mo></mml:math></inline-formula>60 cm) are visible
during the fire and reach their extremum at the end of the fire period.
Surprisingly, SM stayed stable during the fire. L-VOD was substantially
impacted by the fire (anom(L-VOD) <inline-formula><mml:math id="M119" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M120" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>0.14), as well as EVI (anom(EVI) <inline-formula><mml:math id="M121" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M122" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>0.09). C- and X-VOD were barely affected (anom(C-VOD) <inline-formula><mml:math id="M123" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M124" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>0.04,
anom(X-VOD) <inline-formula><mml:math id="M125" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M126" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>0.01). EVI recovered in <inline-formula><mml:math id="M127" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 2–3 years, whereas
L-VOD never recovered its pre-fire level.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F4" specific-use="star"><?xmltex \currentcnt{4}?><?xmltex \def\figurename{Figure}?><label>Figure 4</label><caption><p id="d1e1681">Time series of the number of fires and anomaly time series of
EVI; X-, C-, and L-VOD;  <inline-formula><mml:math id="M128" display="inline"><mml:mi>P</mml:mi></mml:math></inline-formula>; SM; TWS; and <inline-formula><mml:math id="M129" display="inline"><mml:mi>T</mml:mi></mml:math></inline-formula> for <bold>(a)</bold> south-east Australia (13 SMOS
pixels); <bold>(b)</bold> the Mendocino Complex, California (4 SMOS pixels); and <bold>(c)</bold> Santarém (2 SMOS pixels).</p></caption>
          <?xmltex \igopts{width=455.244094pt}?><graphic xlink:href="https://bg.copernicus.org/articles/19/3317/2022/bg-19-3317-2022-f04.png"/>

        </fig>

</sec>
<sec id="Ch1.S4.SS2">
  <label>4.2</label><title>Extension to the ecosystem scale</title>
      <p id="d1e1721">In this section, major fires from September 2013 to October 2019 were
analysed at the ecosystem scale by shifting the anomaly time series of all
variables on the fire date <inline-formula><mml:math id="M130" display="inline"><mml:mrow><mml:msub><mml:mi>t</mml:mi><mml:mi mathvariant="normal">fire</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>. The considered fires are well spread
spatially and temporally over the 6-year period (Fig. 3). In grasslands
and savannas (Fig. 5a and b), pre-fire anomalies of hydrologic variables
are slightly positive, and temperature anomalies are negative during 2 years
before fire. Concurrently, vegetation variables start to increase and reach
a maximum a few months before the fire event (particularly C- and X-VOD).
Anomalies of vegetation variables also show a light surplus over needleleaf
forests just before the fire event (Fig. 5c). Over forests (Fig. 5c, d, e), a 1-year pre-fire drought is visible through the temperature increase
and the decrease in precipitation, SM, and TWS. For all ecosystems, these
drought conditions intensify just before and during fire and end a few
months after fire. During fire, all vegetation variables abruptly decrease
in all ecosystems, EVI being the most impacted one and also faster to
recover. L-VOD is particularly long to recover over forests, especially
dense broadleaf ones (more than 4 years, Fig. 5e). In needleleaf forests
(Fig. 5c), VODs continue to decrease for 1 year. In low-vegetation
ecosystems (Fig. 5a and b), C- and X-VOD never regain their immediate
pre-fire values, which were particularly high.</p>
      <p id="d1e1735">Anomalies of climate variables were also averaged in space and in time,
within timeframes of 6 months, from 24 to 1 month pre-fire, in order to
observe their general trends (Fig. 6). The error bars were computed with Eq. (3). Precipitation anomalies (Fig. 6a) are negative from 6 months pre-fire
for all classes and reach <inline-formula><mml:math id="M131" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>15 mm per month on average before the fire
event. The precipitation deficit is more intense in dense broadleaf forests,
starting 2 years pre-fire and reaching <inline-formula><mml:math id="M132" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>55 mm per month before the fire
event. SM anomalies (Fig. 6b) are similar for the three forest classes. The
SM deficit starts 18 months pre-fire and reaches <inline-formula><mml:math id="M133" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>0.04 m<inline-formula><mml:math id="M134" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msup></mml:math></inline-formula> m<inline-formula><mml:math id="M135" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>
before the fire event. Savannas and grasslands are affected later (6 months
pre-fire) and to a lesser extent (<inline-formula><mml:math id="M136" display="inline"><mml:mo lspace="0mm">∼</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M137" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>0.01 m<inline-formula><mml:math id="M138" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msup></mml:math></inline-formula> m<inline-formula><mml:math id="M139" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>),
as previously observed in Fig. 5. TWS anomalies (Fig. 6c) are negative from
24 months pre-fire for needleleaf forests and from 6 months pre-fire for
dense broadleaf forests. This ecosystem is again the most impacted one, with
a minimum TWS anomaly of <inline-formula><mml:math id="M140" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>7 cm before fire. Temperature anomalies (Fig. 6d)
show significant negative anomalies in grasslands, savannas, and needleleaf
forests from 2 to 1 year pre-fire. From 6 months pre-fire, temperature
anomalies show a surplus in nearly all ecosystems and reach
<inline-formula><mml:math id="M141" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula>1.1<inline-formula><mml:math id="M142" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> C in needleleaf forests and <inline-formula><mml:math id="M143" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula>0.7<inline-formula><mml:math id="M144" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> C in dense
broadleaf forests before the fire event. In summary, pre-fire drought is
mainly observed in forests, with particularly low hydrological values in
dense forests (rainforests) and particularly high temperatures in
needleleaf forests (boreal ecosystems). Savannas and grasslands barely
suffer from pre-fire drought; temperatures are even mild 1 year pre-fire.</p>
      <p id="d1e1856">Vegetation variable anomalies were averaged within timeframes of 6 months,
from 1 to 36 months post-fire, in order to observe the global impacts and
recovery time (Fig. 7). We considered that a variable has totally recovered
when its anomaly is between <inline-formula><mml:math id="M145" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>0.005 and <inline-formula><mml:math id="M146" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula>0.005. Immediately after fire, EVI
is the most impacted variable, with average anomalies of <inline-formula><mml:math id="M147" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>0.026 over
grasslands, <inline-formula><mml:math id="M148" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>0.022 over savannas, <inline-formula><mml:math id="M149" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>0.033 over needleleaf forests, <inline-formula><mml:math id="M150" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>0.051
over sparse broadleaf forests, and <inline-formula><mml:math id="M151" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>0.048 over dense broadleaf forests (Fig. 7a). EVI recovers rapidly, in about 25 to 30 months. X-VOD is less affected
over forests (<inline-formula><mml:math id="M152" display="inline"><mml:mo lspace="0mm">-</mml:mo></mml:math></inline-formula>0.015) than over low vegetation (<inline-formula><mml:math id="M153" display="inline"><mml:mo lspace="0mm">-</mml:mo></mml:math></inline-formula>0.025) (Fig. 7b). X-VOD
gets back to normal within 3 years, savannas and shrublands taking the
longest to recover. C-VOD recovers slower than X-VOD, in particular over
forests (Fig. 7c). L-VOD is mainly affected over dense broadleaf forests
(Fig. 7d). Negative anomalies decrease up to <inline-formula><mml:math id="M154" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>0.05 6 months post-fire,
then slowly increase. L-VOD is less affected than C-VOD elsewhere. It also
shows a delayed impact over needleleaf forests, as for C- and X-VOD.</p>

      <?xmltex \floatpos{p}?><fig id="Ch1.F5" specific-use="star"><?xmltex \currentcnt{5}?><?xmltex \def\figurename{Figure}?><label>Figure 5</label><caption><p id="d1e1933"> </p></caption>
          <?xmltex \igopts{width=369.885827pt}?><graphic xlink:href="https://bg.copernicus.org/articles/19/3317/2022/bg-19-3317-2022-f05-part01.png"/>

        </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F6" specific-use="star"><?xmltex \currentcnt{5}?><?xmltex \def\figurename{Figure}?><label>Figure 5</label><caption><p id="d1e1944">Time series of the number of fires and anomaly time series of
EVI; X-, C-, and L-VOD; <inline-formula><mml:math id="M155" display="inline"><mml:mi>P</mml:mi></mml:math></inline-formula>; SM; TWS; and <inline-formula><mml:math id="M156" display="inline"><mml:mi>T</mml:mi></mml:math></inline-formula>, shifted on the fire date, for the following biomes: <bold>(a)</bold> grasslands and croplands, <bold>(b)</bold> savannas and shrublands, <bold>(c)</bold> needleleaf forest, <bold>(d)</bold> sparse broadleaf forest, and <bold>(e)</bold> dense
broadleaf forest. Missing values appear when the number of available
points is lower than half the maximum number of points of the biome (empty
circles in the lower panel). This is mostly due to snow filtering. Data are
kept otherwise (black filled dots).</p></caption>
          <?xmltex \igopts{width=398.338583pt}?><graphic xlink:href="https://bg.copernicus.org/articles/19/3317/2022/bg-19-3317-2022-f05-part02.png"/>

        </fig>

</sec>
</sec>
<sec id="Ch1.S5">
  <label>5</label><title>Discussion</title>
<sec id="Ch1.S5.SS1">
  <label>5.1</label><title>Case study: analysis of three major fires</title>
      <p id="d1e2000">In south-east Australia, a strong pre-fire drought is
visible not only in the climate variables but also in the mild decrease in vegetation
variables (Fig. 4a), linked with VWC deficit. Ehsani et al. (2020) stated
that the air temperature from December 2019 to February 2020 was about
1<inline-formula><mml:math id="M157" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> C higher than usual, which increased evapotranspiration, while
the lack of precipitation prevented the soil from satisfying the moisture
demand and led to a significant vegetation drying (fuel) that facilitated
the propagation of fires. After the fire event, L-VOD regained its pre-fire
values within a year, meaning that the woody biomass was not entirely
destroyed. Indeed, these eucalyptus forests are known to be somewhat fire
resistant (Wilkinson and Jennings, 1993; Caccamo et al., 2015). They can
regenerate branches and leaves by resprouting from heat-resistant buds
(Burrows, 2002). The rapid recovery of vegetation data can also be explained
by the recovery of VWC, linked with the post-fire increase in precipitation
and SM (Konings et al., 2021). Indeed, in 2020, SM values exceeded those of
the previous decade (anom(SM) <inline-formula><mml:math id="M158" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M159" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula>0.15 m<inline-formula><mml:math id="M160" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msup></mml:math></inline-formula> m<inline-formula><mml:math id="M161" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>), corresponding
to the end of the severe drought affecting south-east Australia associated
with the 2020–2021 La Niña event (BoM, 2021). The increase in SM and
precipitation may also have expedited the extinction of fires (Ehsani et
al., 2020).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F7" specific-use="star"><?xmltex \currentcnt{6}?><?xmltex \def\figurename{Figure}?><label>Figure 6</label><caption><p id="d1e2049">Anomalies of <bold>(a)</bold> precipitation, <bold>(b)</bold> SM, <bold>(c)</bold> TWS, and <bold>(d)</bold> temperature, for each ecosystem, at several pre-fire timescales. The error
bars were computed with Eq. (3).</p></caption>
          <?xmltex \igopts{width=455.244094pt}?><graphic xlink:href="https://bg.copernicus.org/articles/19/3317/2022/bg-19-3317-2022-f06.png"/>

        </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F8" specific-use="star"><?xmltex \currentcnt{7}?><?xmltex \def\figurename{Figure}?><label>Figure 7</label><caption><p id="d1e2072">Anomalies of <bold>(a)</bold> EVI, <bold>(b)</bold> X-VOD, <bold>(c)</bold> C-VOD, and <bold>(d)</bold> L-VOD, for
each ecosystem, at several post-fire timescales. The error bars were
computed with Eq. (3).</p></caption>
          <?xmltex \igopts{width=455.244094pt}?><graphic xlink:href="https://bg.copernicus.org/articles/19/3317/2022/bg-19-3317-2022-f07.png"/>

        </fig>

      <p id="d1e2094">For California, the study by Brown et al. (2020) provides a comprehensive
analysis of the climate and fuel conditions leading to the 2018 Mendocino
Complex and reports several events that are also noticeable in our
analysis. Among these, positive rainfall and SM anomalies in winter
2016/17 are depicted in Fig. 4b, which led to the second consecutive
spring with above-average accumulation of fine fuel (grasses). Positive
temperature anomalies in winter 2017/18 are also visible, when a lack of
storm enabled the survival of grasses. In April 2018, precipitation and warm
temperatures led to above-normal spring brush and grass growth. No major
drought is visible in summer 2018, but low rainfall and warm temperatures
led to a rapid drying of fuels and induced a poor overnight humidity
recovery. All these similarities with the findings by Brown et al. (2020)  support
our observations. The dramatic fire impacted EVI and L-VOD in the long term.
Eucalyptus, pine trees, and chaparral were burned. Even if this type of
vegetation is fire-adapted, the strength of the fire seemed to have
destroyed most of it (34 % vegetation loss, Hansen et al., 2013).
Increased forest fire activity in recent decades in California has likely
been enabled by the legacy of fire suppression, human settlement, and
anthropogenic climate change (Abatzoglou and Williams, 2016). Stephens et
al. (2018) stated that the massive current tree mortality in California will
undoubtedly provoke severe “mass fires” in the coming decades, driven by
the amount of dry and combustible wood.</p>
      <p id="d1e2097">In the Santarém region (Amazon), the winter 2015 wildfire was attributed to
high temperature and low precipitation linked with El Niño event
(Berenguer et al., 2018), which clearly emerges from Fig. 4c. These extreme
drought conditions worsened during and at the end of the fire and may
explain its strength. Several factors can explain this observation. First,
MODIS may not detect all fires in January 2016 in this area because of (i) the
cloud coverage (Roy et al., 2008) and (ii) the dense vegetation cover hiding
understorey fires (Withey et al., 2018). This would be in line with the 2016
Hansen et al. (2013)  tree cover loss detection (Fig. 2). Secondly, drought may
sometimes keep increasing after fire extinguishment because the removal of
the vegetation cover and the deterioration of the soil contributes to
maintaining a hot and dry climate (Auld and Bradstock, 1996; Veraverbeke et
al., 2010). This phenomenon is also visible in the savanna and in the sparse
broadleaf biome (Fig. 5b and d). Contrary to TWS and precipitation, SM
stayed stable during the fire, maybe because of the reduced accuracy of SM
measurements under very dense forest. The 3-year recovery time of EVI
after the severe fire indicates a moderate regrowth of leaves and grasses.
In contrast, L-VOD never regained its pre-fire values, meaning that trunks
were impacted in the long term.</p>
</sec>
<sec id="Ch1.S5.SS2">
  <label>5.2</label><title>Extension to the ecosystem scale</title>
      <p id="d1e2108">Grasslands, croplands, shrublands, and savannas do not show signs of pre-fire
drought (Figs. 5a, b and 6). Indeed, in these dry ecosystems, the standard
summer conditions are often prone to wildfire ignitions (Chaparro et al.,
2016). A substantial increase in vegetation variables, C- and X-VOD in
particular, occurs 1 to 2 years before fire, which implies an increase in
vegetation density, e.g. available fuel. This is consistent with the fact
that the C and X bands are more sensitive to dry low shrubland vegetation
(Jackson et al., 1982; de Jeu et al., 2008). Immediately before fire, both
VOD and SM values drop down, suggesting a decrease in VWC, especially over
grasslands (Fig. 5a). The increase in vegetation material combined with the
decrease in VWC may contribute to triggering large wildfires (Forkel et al.,
2017; Kuhn-Régnier et al., 2021). Indeed, the fire risk in savannas is
highest for dry vegetation with enough fuel to enable drastic burning
(Mbow et al., 2004). This vegetation growth might be enabled by negative
pre-fire temperature anomalies and a light positive anomaly in pre-fire
hydrological variables (Fig. 6). Vegetation variables are less impacted by
fires (Fig. 7), which are rapid and burn through the grass layer, resulting
in less destruction than in forests (Menaut et al., 1990; Gignoux et al.,
1997). L-VOD in particular is slightly impacted because the burned vegetation
is mainly leaf biomass. EVI quickly recovers after fire, probably because
fire burns most of the AGB of grass species but spares their large
underground root systems, resulting in a rapid establishment of new shoots
(Hochberg et al., 1994). The exceptionally high pre-fire vegetation
variable values are never regained.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F9" specific-use="star"><?xmltex \currentcnt{8}?><?xmltex \def\figurename{Figure}?><label>Figure 8</label><caption><p id="d1e2113">Anomalies of vegetation variables (<inline-formula><mml:math id="M162" display="inline"><mml:mi>V</mml:mi></mml:math></inline-formula>) averaged <bold>(a)</bold> from 1 to 3 months post-fire and <bold>(b)</bold> from 24 to 35 months post-fire, with respect to
the number of fires by pixel (MODIS), for dense broadleaf forests only. The
anomalies were normalized with the 99th quantile of each variable
<inline-formula><mml:math id="M163" display="inline"><mml:mrow><mml:msub><mml:mi>V</mml:mi><mml:mi mathvariant="normal">max</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> (EVI<inline-formula><mml:math id="M164" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mi mathvariant="normal">max</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0.60</mml:mn></mml:mrow></mml:math></inline-formula>, X-VOD<inline-formula><mml:math id="M165" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mi mathvariant="normal">max</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn mathvariant="normal">1.03</mml:mn></mml:mrow></mml:math></inline-formula>, C-VOD<inline-formula><mml:math id="M166" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mi mathvariant="normal">max</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn mathvariant="normal">1.20</mml:mn></mml:mrow></mml:math></inline-formula>, and L-VOD<inline-formula><mml:math id="M167" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mi mathvariant="normal">max</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn mathvariant="normal">1.20</mml:mn></mml:mrow></mml:math></inline-formula>).</p></caption>
          <?xmltex \igopts{width=483.69685pt}?><graphic xlink:href="https://bg.copernicus.org/articles/19/3317/2022/bg-19-3317-2022-f08.png"/>

        </fig>

      <p id="d1e2203">In needleleaf forest anomaly time series (Fig. 5c), the numerous missing
values correspond to the filtering of snow in winter. These wildfires are
located in the Northern Hemisphere temperate and boreal forests and mostly
occur in late spring and summer (Fig. 3). De Groot et al. (2013) explained
that most fires in Canada occur during summer, due to lightning strikes,
whereas most fires in Russia occur during spring and are human-caused. We
found a strong pre-fire drought in this ecosystem (low SM and high
temperature 1 year pre-fire, Fig. 6), which is well documented for
previous fire episodes (Weber and Stocks, 1998). Our results are in line
with those of Forkel et al. (2012), who found that previous-summer SM was a
good predictor for burned area in Siberian larch forests. Indeed, negative
summer anomalies led to low frozen water the following winter and to less
water being released during the following spring–summer season, which in turn
eased the outbreak of large wildfires. VODs also showed a light surplus
before fire, possibly linked with litter thickening (e.g. dead needles,
cured grass, leaf litter), which also facilitates fire propagation (de Groot
et al., 2013). We found a delayed impact of fire on vegetation variables,
as well as a longer recovery time than in other ecosystems, of about 3–4 years
(Figs. 5c and 7). This duration is slightly less than what was found in other
studies (5 years in Canada, Goetz et al., 2006; 5 to 8 years in North
America, Jin et al., 2012), but our findings still confirm previous results
from Yang et al. (2017), who showed with NDVI analyses over North America
that the fire effect on needleleaf trees was stronger and longer than on
other vegetation types. Fires in North America are predominantly
stand-replacing and high-intensity crown fires (Stocks et al., 2004; Jin et
al., 2012), whereas fires in Eurasia are generally lower-intensity surface
fires and less destructive for the vegetation (de Groot et al., 2013). These
different fire regimes are influenced by tree species (Rogers et al., 2015).
Time series were plotted separately over each continent (Fig. S1). L-VOD and
EVI recover more slowly in North America than in Eurasia (<inline-formula><mml:math id="M168" display="inline"><mml:mo lspace="0mm">∼</mml:mo></mml:math></inline-formula> 4 vs. <inline-formula><mml:math id="M169" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 2 years for L-VOD, <inline-formula><mml:math id="M170" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 3 vs.
<inline-formula><mml:math id="M171" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 2 years for EVI), confirming these different boreal fire
regimes. Moreover, we found that L-VOD is moderately impacted during fire,
which can be attributed to the dominant destruction of needles and branches
by boreal fires (Alexander and Cruz, 2011).</p>
      <p id="d1e2235">Sparse broadleaf forests (AGB <inline-formula><mml:math id="M172" display="inline"><mml:mo>≤</mml:mo></mml:math></inline-formula> 150 Mg ha<inline-formula><mml:math id="M173" 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>) subject to wildfires
are mostly located in subtropical and temperate areas of the Americas, West
Africa, Australia, and South-East Asia (Fig. 3). A drying trend is visible
1 year pre-fire (Figs. 5d and 6). The link between drought and wildfires
was previously observed by de Marzo et al. (2021) in the Argentine Gran
Chaco, by Cheng et al. (2013) in the Mexican Yucatán forest, and by Vadrevu
et al. (2019) in South-East Asian forests, with a prominent influence of
precipitation variations over temperature variations. L-VOD and EVI are
particularly impacted by fire, but they recover quickly (1 year for EVI, 2.5 years for L-VOD). Yang et al. (2017) also found a rapid recovery time over
North American broadleaf trees due to their fire-adaptive resprouting
regeneration mode. The same observations were made in the fire-prone Argentine
Chaco forest by Torres et al. (2014).</p>
      <p id="d1e2257">Dense broadleaf forests are mostly located in the tropics (Fig. 3). We can
notice a few fires in the densest rainforests (Congo basin, central Amazon)
because (i) they are usually too humid to burn (Cochrane, 2003; Forkel et
al., 2017), (ii) MODIS active fire detections are underestimated under thick
cloud coverage or for understorey fires (Giglio et al., 2020), and (iii) seasonally flooded areas were excluded in order to use only robust VOD
estimations (Bousquet et al., 2021). A consistent drought is visible 8 months before fire events (Fig. 5e), with high negative SM, TWS, and
precipitation anomalies (Fig. 6). Chen et al. (2013) also found TWS deficits
before severe fire seasons across the southern Amazon. Indeed, rainfall
shortage generates high water deficits (i.e. high negative TWS and SM
anomalies), which cause tree mortality and leaf shedding (visible in pre-fire
EVI decrease) and thus increase fuel availability (Aragão et al., 2018).
Nevertheless, no pre-fire VOD decrease is observed here, showing that tree
species of dense forests can maintain their VWC. Drought-related fires were
suggested to prevail over deforestation fires in the Amazon and are
predicted to increase in the near future (Aragão et al., 2018). The
opening of forest canopies also boosts incident radiation levels which leads
to temperature rise (Ray et al., 2005). The combination of fuel increase in
a drier and hotter environment converts forests into fire-prone ecosystems
(Aragão et al., 2018). We also found that dense broadleaf forests were
the ecosystem most impacted by fire (Fig. 7) because the absolute pre-fire
values of vegetation variables are particularly high and because it is not
a fire-adapted ecosystem (Cochrane, 2003). L-VOD in particular decreases
strongly and recovers very slowly (Fig. 7d), as previously observed over the
Santarém fire (Fig. 4c). The strong post-fire decrease in L-VOD is due not only to
biomass destruction but also to water stress in the remaining vegetation
(Konings et al., 2021). This finding confirms the significant and damaging
impact of fires in the dense broadleaf ecosystem previously observed by
Silva et al. (2018) and de Faria et al. (2021). L-VOD was previously proven
to be more sensitive to high AGB values than C- and X-VOD
(Rodriguez-Fernandez et al., 2018). Here, we suggest that L-VOD depicts
the fire impact on high-AGB areas better than the other vegetation
variables.</p>
      <p id="d1e2260">For all biomes, EVI is the most rapid index to recover, because leaves
rapidly resprout. EVI and X-VOD seem better adapted for grassland fire
monitoring; C-VOD is better for savanna fire monitoring; and L-VOD is better for forest fire monitoring.</p>
</sec>
<sec id="Ch1.S5.SS3">
  <label>5.3</label><title>The potential of L-VOD for vegetation recovery monitoring over dense
forests</title>
      <p id="d1e2271">Normalized anomalies of vegetation variables were also plotted with respect
to the number of fires in the dense broadleaf ecosystem, immediately after
fire (1–3 months post-fire, Fig. 8a) and over a longer period (1–2 years
post-fire, Fig. 8b). A quasi-linear relationship is visible between all
vegetation estimates and the number of fires. As previously observed in
Sect. 4.2, EVI and L-VOD are the most impacted variables immediately after
fire (Fig. 8a), while L-VOD is still significantly affected 1 to 2 years
after fire (up to <inline-formula><mml:math id="M174" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>0.06, Fig. 8b). L-VOD then shows a clear response to fire
events over high-AGB areas, not only immediately but also in the long term and
proportionally to the number of fires within a SMOS pixel. Thanks to its
sensitivity to coarse woody elements and to its deep penetration through the
vegetation layer, L-VOD is better correlated with high AGB than other
vegetation variables (Rodriguez-Fernandez et al., 2018) and could be used
for post-fire recovery monitoring over dense forests. One must keep in mind
that not only the biomass density (AGB) but also its hydrological status
(VWC) are depicted in the VOD.</p>
</sec>
</sec>
<sec id="Ch1.S6" sec-type="conclusions">
  <label>6</label><title>Conclusions</title>
      <p id="d1e2290">In this paper, we analysed the pre-fire behaviour of four satellite-based
fire likelihood factors, including SMOS SM. In forests, which generally
maintain a steady humidity, we found that fires are linked with intense and
prolonged drought. Pre-fire temperature anomalies are particularly high in
boreal needleleaf forests. In savannas and grasslands, in agreement with
previous studies (Mbow et al., 2004), we found evidence of an increase in
available fuel prior to fire events, enabled by humid and cold conditions a
few years before. We also found that vegetation variables recover rapidly in
these ecosystems, as wildfires are often rapid and mildly destructive for
trees. In contrast, over forests, fires can damage the vegetation in the
long term. Zhang et al. (2021) demonstrated the potential of C-band
vegetation optical depth to detect the vegetation change patterns caused by
fire in the southern Amazon. Our study confirms these findings and extends
it to the ecosystem scale and to two extra wavelengths. Dense broadleaf
forest fires particularly impact the L-band emission, which represents
coarse woody elements (trunks and stems), whereas sparse vegetation fires
affect the C and X bands more, which are more sensitive to small branches and
leaves. For all biomes, the visible-infrared index (EVI) drops down after
fire but recovers quickly, as it represents only herbage and canopy foliage.
The long-term impact on L-VOD in dense broadleaf forests shows that fires in
this ecosystem are severely destructive for trunks, while smaller woody
elements and leaves resprout faster. Thus, L-VOD seems to be the best-adapted
vegetation variable for the monitoring of dense vegetation recovery after
large fires.</p>
      <p id="d1e2293">The increasing number of wildfires threatens the stability of several
ecosystems. It is then particularly important to monitor the vegetation
health, and the L band proved to be complementary to existing measurements,
especially over dense forests.</p>
</sec>

      
      </body>
    <back><notes notes-type="codeavailability"><title>Code availability</title>

      <p id="d1e2300">All MATLAB analysis codes are available upon request.</p>
  </notes><notes notes-type="dataavailability"><title>Data availability</title>

      <p id="d1e2306">SMOS L2 was obtained from ESA's DPGS
(Data Processing Ground Segment). AMSR2 data were provided by Vrije Universiteit Amsterdam (Richard de Jeu) and NASA GSFC (Goddard Space Flight Center) (Manfred Owe) (2014).
AMSR2/GCOM-W1 surface soil moisture (LPRM) L3 1 d 25 km <inline-formula><mml:math id="M175" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 25 km ascending V001 data were edited by the Goddard Earth Sciences Data and Information Services Center (GES DISC) (Bill Teng) of Greenbelt, Maryland, USA (<ext-link xlink:href="https://doi.org/10.5067/M5DTR2QUYLS2" ext-link-type="DOI">10.5067/M5DTR2QUYLS2</ext-link>, de Jeu  and Owe, 2014).
TWS data were obtained from the GFZ (German Research Centre for Geosciences) GravIS (Gravity Information Service) web portal.
Fire, temperature, and EVI data came from the NASA Earth Observations (NEO) portal and Land Processes Distributed Active Archive Center (LP DAAC).
IMS Daily Northern Hemisphere Snow and Ice Analysis at 4 km resolution, version 1, came from the United States National Ice Center (USNIC) of Boulder, Colorado, USA, delivered by the National Snow and Ice Data Center (NSIDC) (<ext-link xlink:href="https://doi.org/10.7265/N52R3PMC" ext-link-type="DOI">10.7265/N52R3PMC</ext-link>, NSIDC, 2008).</p>
  </notes><app-group>
        <supplementary-material position="anchor"><p id="d1e2322">The supplement related to this article is available online at: <inline-supplementary-material xlink:href="https://doi.org/10.5194/bg-19-3317-2022-supplement" xlink:title="pdf">https://doi.org/10.5194/bg-19-3317-2022-supplement</inline-supplementary-material>.</p></supplementary-material>
        </app-group><notes notes-type="authorcontribution"><title>Author contributions</title>

      <p id="d1e2331">EB, AM, NRF, and YK planned the research discussed in this
paper. EB performed most of the computations. SM provided the AGB
dataset and expertise on AGB and on forest loss estimation. All authors
participated in the writing and provided comments and suggestions.</p>
  </notes><notes notes-type="competinginterests"><title>Competing interests</title>

      <p id="d1e2337">The contact author has declared that none of the authors has any competing interests.</p>
  </notes><notes notes-type="disclaimer"><title>Disclaimer</title>

      <p id="d1e2343">Publisher’s note: Copernicus Publications remains neutral with regard to jurisdictional claims in published maps and institutional affiliations.</p>
  </notes><ack><title>Acknowledgements</title><p id="d1e2349">The authors would like to thank the
European Space Agency (ESA).
The authors wish to thank David Chaparro and Matthias Forkel for their relevant comments and reviews which considerably improved the paper.</p></ack><notes notes-type="financialsupport"><title>Financial support</title>

      <p id="d1e2355">This research has been supported by the Centre National d'Etudes Spatiales (CATDS CEC SM contract grant) and by the CNES (Centre National d'Etudes Spatiales) TOSCA (Terre, Océans, Surfaces Continentales, Atmosphère) programme.</p>
  </notes><notes notes-type="reviewstatement"><title>Review statement</title>

      <p id="d1e2361">This paper was edited by Alexandra Konings and reviewed by Matthias Forkel and David Chaparro.</p>
  </notes><ref-list>
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