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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 Publications</publisher-name>
    <publisher-loc>Göttingen, Germany</publisher-loc>
  </publisher></journal-meta>
    <article-meta>
      <article-id pub-id-type="doi">10.5194/bg-14-5425-2017</article-id><title-group><article-title>Improving global paleogeography since the late Paleozoic<?xmltex \hack{\break}?> using paleobiology</article-title>
      </title-group><?xmltex \runningtitle{Improving global paleogeography since the late Paleozoic using paleobiology}?><?xmltex \runningauthor{W.~Cao et al.}?>
      <contrib-group>
        <contrib contrib-type="author" corresp="yes" rid="aff1">
          <name><surname>Cao</surname><given-names>Wenchao</given-names></name>
          <email>wenchao.cao@sydney.edu.au</email>
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Zahirovic</surname><given-names>Sabin</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-6751-4976</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1 aff4">
          <name><surname>Flament</surname><given-names>Nicolas</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-3237-0757</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Williams</surname><given-names>Simon</given-names></name>
          
        <ext-link>https://orcid.org/0000-0003-4670-8883</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2">
          <name><surname>Golonka</surname><given-names>Jan</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1 aff3">
          <name><surname>Müller</surname><given-names>R. Dietmar</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-3334-5764</ext-link></contrib>
        <aff id="aff1"><label>1</label><institution>EarthByte Group and Basin GENESIS Hub, School of Geosciences, The University of Sydney,<?xmltex \hack{\break}?> Sydney, NSW 2006, Australia</institution>
        </aff>
        <aff id="aff2"><label>2</label><institution>Faculty of Geology, Geophysics and Environmental Protection, AGH University of Science and Technology,<?xmltex \hack{\break}?> Mickiewicza 30, 30-059 Kraków, Poland</institution>
        </aff>
        <aff id="aff3"><label>3</label><institution>Sydney Informatics Hub, The University of Sydney, Sydney, NSW 2006, Australia</institution>
        </aff>
        <aff id="aff4"><label>a</label><institution>current address: School of Earth and Environmental Sciences, University of Wollongong,<?xmltex \hack{\break}?> Northfields Avenue, Wollongong, NSW 2522, Australia</institution>
        </aff>
      </contrib-group>
      <author-notes><corresp id="corr1">Wenchao Cao (wenchao.cao@sydney.edu.au)</corresp></author-notes><pub-date><day>4</day><month>December</month><year>2017</year></pub-date>
      
      <volume>14</volume>
      <issue>23</issue>
      <fpage>5425</fpage><lpage>5439</lpage>
      <history>
        <date date-type="received"><day>16</day><month>March</month><year>2017</year></date>
           <date date-type="rev-request"><day>18</day><month>April</month><year>2017</year></date>
           <date date-type="rev-recd"><day>10</day><month>October</month><year>2017</year></date>
           <date date-type="accepted"><day>21</day><month>October</month><year>2017</year></date>
      </history>
      <permissions>
        
        
      <license license-type="open-access"><license-p>This work is licensed under the Creative Commons Attribution 3.0 Unported License. To view a copy of this licence, visit <ext-link ext-link-type="uri" xlink:href="https://creativecommons.org/licenses/by/3.0/">https://creativecommons.org/licenses/by/3.0/</ext-link></license-p></license></permissions><self-uri xlink:href="https://bg.copernicus.org/articles/14/5425/2017/bg-14-5425-2017.html">This article is available from https://bg.copernicus.org/articles/14/5425/2017/bg-14-5425-2017.html</self-uri><self-uri xlink:href="https://bg.copernicus.org/articles/14/5425/2017/bg-14-5425-2017.pdf">The full text article is available as a PDF file from https://bg.copernicus.org/articles/14/5425/2017/bg-14-5425-2017.pdf</self-uri>
      <abstract>
    <p id="d1e152">Paleogeographic reconstructions are important to understand Earth's tectonic
evolution, past eustatic and regional sea level change, paleoclimate and
ocean circulation, deep Earth resources and to constrain and interpret the
dynamic topography predicted by mantle convection models. Global
paleogeographic maps have been compiled and published, but they are generally
presented as static maps with varying map projections, different time
intervals represented by the maps and different plate motion models that
underlie the paleogeographic reconstructions. This makes it difficult to
convert the maps into a digital form and link them to alternative digital
plate tectonic reconstructions. To address this limitation, we develop a
workflow to restore global paleogeographic maps to their present-day
coordinates and enable them to be linked to a different tectonic
reconstruction. We use marine fossil collections from the Paleobiology
Database to identify inconsistencies between their indicative
paleoenvironments and published paleogeographic maps, and revise the
locations of inferred paleo-coastlines that represent the estimated maximum
transgression surfaces by resolving these inconsistencies. As a result, the
consistency ratio between the paleogeography and the paleoenvironments
indicated by the marine fossil collections is increased from an average of
75 % to nearly full consistency (100 %). The paleogeography in the
main regions of North America, South America, Europe and Africa is
significantly revised, especially in the Late Carboniferous, Middle Permian,
Triassic, Jurassic, Late Cretaceous and most of the Cenozoic. The global
flooded continental areas since the Early Devonian calculated from the
revised paleogeography in this study are generally consistent with results
derived from other paleoenvironment and paleo-lithofacies data and with the
strontium isotope record in marine carbonates. We also estimate the
terrestrial areal change over time associated with transferring
reconstruction, filling gaps and modifying the paleogeographic geometries
based on the paleobiology test. This indicates that the variation of the
underlying plate reconstruction is the main factor that contributes to the
terrestrial areal change, and the effect of revising paleogeographic
geometries based on paleobiology is secondary.</p>
  </abstract>
    </article-meta>
  </front>
<body>
      

      <?xmltex \hack{\vspace{-2mm}}?>
<sec id="Ch1.S1" sec-type="intro">
  <title>Introduction</title>
      <p id="d1e164">Paleogeography, describing the ancient distribution of highlands, lowlands,
shallow seas and deep ocean basins, is widely used in a range of fields
including paleoclimatology, plate tectonic reconstructions,
paleobiogeography, resource exploration and geodynamics. Global deep-time
paleogeographic compilations have been published (e.g., Blakey, 2008; Golonka
et al., 2006; Ronov, et al., 1984, 1989; Scotese, 2001, 2004; Smith et al.,
1994). However, they are generally presented as static paleogeographic
snapshots with varying map projections and different time intervals
represented by the maps, and are tied to different plate motion models. This
makes it difficult to convert the maps into a digital format, link them to
alternative digital plate tectonic reconstructions and update them when
plate motion models are improved. It is therefore challenging to use
paleogeographic maps to help constrain or interpret numerical models of
mantle convection that predict long-wavelength topography (Gurnis et al.,
1998; Spasojevic and Gurnis, 2012) based on different tectonic
reconstructions, or as an input to models of past ocean and atmosphere
circulation/climate (Goddéris et al., 2014; Golonka et al., 1994) and
models of past erosion/sedimentation (Salles et al., 2017).</p>
      <p id="d1e167">In order to address these issues, we develop a workflow to restore the
ancient paleogeographic geometries back to their modern coordinates so that
the geometries can be attached to a different plate motion model. This is the
first step towards the construction of paleogeographic maps with flexible
spatial and temporal resolutions that are more easily testable and expandable
with the incorporation of new paleoenvironmental data sets (e.g., Wright et
al., 2013). In this study, we use a set of global paleogeographic maps
(Golonka et al., 2006) covering the entire Phanerozoic time period as the
base paleogeographic model. Coastlines on these paleogeographic maps
represent estimated maximum marine transgression surfaces (Kiessling et al.,
2003). We first restore the global paleogeographic geometries of Golonka et
al. (2006) to their present-day coordinates by reversing the sign of the
rotation angle, and then reconstruct them to geological times using a
different plate motion model of Matthews et al. (2016). We then use
paleoenvironmental information from marine fossil collections from the
Paleobiology Database to modify the inferred paleo-coastline locations and
paleogeographic geometries. Next, we use the revised paleogeography to
estimate the surface areas of global paleogeographic features including deep
oceans, shallow marine environments, landmasses, mountains and ice sheets. In
addition, we compare the global flooded continental areas since the Devonian
calculated from the revised paleogeography with other results derived from
other paleoenvironment and paleo-lithofacies maps (Ronov, 1994; Smith et al.,
1994; Walker et al., 2002; Blakey, 2003, 2008; Golonka, 2007b, 2009, 2012) or
from the strontium isotope record (van der Meer et al., 2017). We estimate
the terrestrial areal change over time associated with transferring
reconstruction, filling gaps and modifying the paleogeographic geometries
based on consistency test. Finally, we test the marine fossil collection data
set used in this study for fossil abundances over time using different
timescales of the International Commission on Stratigraphy (ICS2016; Cohen et
al., 2013, updated) and of Golonka (2000) and discuss the limitations of the workflow
we develop in this study.</p>
</sec>
<sec id="Ch1.S2">
  <title>Data and paleogeographic model</title>
      <p id="d1e176">The data used in this study are global paleogeographic maps and
paleoenvironmental data for the last 402 million years (Myr), which
originate from the set of paleogeographic maps produced by Golonka et al. (2006) and the Paleobiology Database (PBDB, <uri>https://paleobiodb.org</uri>), respectively.
The global paleogeographic compilation extending back to the Early Devonian
of Golonka et al. (2006) is divided into 24 time-interval maps using
the timescale of Golonka (2000) which is based on the original timescale
of Sloss (1988; Table 1). Each map is a compilation of paleo-lithofacies
and paleoenvironments for each geological time interval. These
paleogeographic reconstructions illustrate the changing configuration of ice
sheets, mountains, landmasses, shallow marine environments (inclusive of
shallow seas and continental slopes) and deep oceans over the last
<inline-formula><mml:math id="M1" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 400 Myr.</p>

<?xmltex \floatpos{p}?><table-wrap id="Ch1.T1" specific-use="star" orientation="landscape"><caption><p id="d1e192">Timescale since the Early Devonian (Golonka, 2000) used in the paleogeographic
maps of Golonka et al. (2006), the original timescale of
Sloss (1988) and of the International Commission on
Stratigraphy (ICS2016). Ages in italics are obtained by linear interpolation
between subdivisions.</p></caption><oasis:table frame="topbot"><?xmltex \begin{scaleboxenv}{.87}[.87]?><oasis:tgroup cols="11">
     <oasis:colspec colnum="1" colname="col1" align="left" colsep="1"/>
     <oasis:colspec colnum="2" colname="col2" align="left"/>
     <oasis:colspec colnum="3" colname="col3" align="right"/>
     <oasis:colspec colnum="4" colname="col4" align="right" colsep="1"/>
     <oasis:colspec colnum="5" colname="col5" align="left"/>
     <oasis:colspec colnum="6" colname="col6" align="left"/>
     <oasis:colspec colnum="7" colname="col7" align="right"/>
     <oasis:colspec colnum="8" colname="col8" align="right"/>
     <oasis:colspec colnum="9" colname="col9" align="right" colsep="1"/>
     <oasis:colspec colnum="10" colname="col10" align="right"/>
     <oasis:colspec colnum="11" colname="col11" align="right"/>
     <oasis:thead>
       <oasis:row>  
         <oasis:entry colname="col1"/>  
         <oasis:entry rowsep="1" namest="col2" nameend="col4" align="center" colsep="1">Sloss (1988) </oasis:entry>  
         <oasis:entry rowsep="1" namest="col5" nameend="col9" align="center" colsep="1">Golonka (2000) </oasis:entry>  
         <oasis:entry rowsep="1" namest="col10" nameend="col11" align="center">ICS2016 </oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">Era</oasis:entry>  
         <oasis:entry colname="col2">Subsequence</oasis:entry>  
         <oasis:entry colname="col3">Start</oasis:entry>  
         <oasis:entry colname="col4">End</oasis:entry>  
         <oasis:entry colname="col5">Time slice</oasis:entry>  
         <oasis:entry colname="col6">Epoch/age</oasis:entry>  
         <oasis:entry colname="col7">Start</oasis:entry>  
         <oasis:entry colname="col8">End</oasis:entry>  
         <oasis:entry colname="col9">Reconstruction</oasis:entry>  
         <oasis:entry colname="col10">Start</oasis:entry>  
         <oasis:entry colname="col11">End</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">  
         <oasis:entry colname="col1"/>  
         <oasis:entry colname="col2"/>  
         <oasis:entry colname="col3">(Ma)</oasis:entry>  
         <oasis:entry colname="col4">(Ma)</oasis:entry>  
         <oasis:entry colname="col5"/>  
         <oasis:entry colname="col6"/>  
         <oasis:entry colname="col7">(Ma)</oasis:entry>  
         <oasis:entry colname="col8">(Ma)</oasis:entry>  
         <oasis:entry colname="col9">time (Ma)</oasis:entry>  
         <oasis:entry colname="col10">(Ma)</oasis:entry>  
         <oasis:entry colname="col11">(Ma)</oasis:entry>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row>  
         <oasis:entry colname="col1">Cenozoic</oasis:entry>  
         <oasis:entry colname="col2">Tejas III</oasis:entry>  
         <oasis:entry colname="col3">29</oasis:entry>  
         <oasis:entry colname="col4">0</oasis:entry>  
         <oasis:entry colname="col5">late Tejas III</oasis:entry>  
         <oasis:entry colname="col6">Tortonian–Gelasian</oasis:entry>  
         <oasis:entry colname="col7">11</oasis:entry>  
         <oasis:entry colname="col8">2</oasis:entry>  
         <oasis:entry colname="col9">6</oasis:entry>  
         <oasis:entry colname="col10">11.63</oasis:entry>  
         <oasis:entry colname="col11">1.80</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1"/>  
         <oasis:entry colname="col2"/>  
         <oasis:entry colname="col3"/>  
         <oasis:entry colname="col4"/>  
         <oasis:entry colname="col5">late Tejas II</oasis:entry>  
         <oasis:entry colname="col6">Burdigalian–Serravallian</oasis:entry>  
         <oasis:entry colname="col7">20</oasis:entry>  
         <oasis:entry colname="col8">11</oasis:entry>  
         <oasis:entry colname="col9">14</oasis:entry>  
         <oasis:entry colname="col10">20.44</oasis:entry>  
         <oasis:entry colname="col11">11.63</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1"/>  
         <oasis:entry rowsep="1" colname="col2"/>  
         <oasis:entry rowsep="1" colname="col3"/>  
         <oasis:entry rowsep="1" colname="col4"/>  
         <oasis:entry rowsep="1" colname="col5">late Tejas I</oasis:entry>  
         <oasis:entry rowsep="1" colname="col6">Chattian–Aquitanian</oasis:entry>  
         <oasis:entry rowsep="1" colname="col7">29</oasis:entry>  
         <oasis:entry rowsep="1" colname="col8">20</oasis:entry>  
         <oasis:entry rowsep="1" colname="col9">22</oasis:entry>  
         <oasis:entry rowsep="1" colname="col10">28.1</oasis:entry>  
         <oasis:entry rowsep="1" colname="col11">20.44</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1"/>  
         <oasis:entry rowsep="1" colname="col2">Tejas II</oasis:entry>  
         <oasis:entry rowsep="1" colname="col3">39</oasis:entry>  
         <oasis:entry rowsep="1" colname="col4">29</oasis:entry>  
         <oasis:entry rowsep="1" colname="col5">early Tejas III</oasis:entry>  
         <oasis:entry rowsep="1" colname="col6">Priabonian–Rupelian</oasis:entry>  
         <oasis:entry rowsep="1" colname="col7">37</oasis:entry>  
         <oasis:entry rowsep="1" colname="col8">29</oasis:entry>  
         <oasis:entry rowsep="1" colname="col9">33</oasis:entry>  
         <oasis:entry rowsep="1" colname="col10">37.8</oasis:entry>  
         <oasis:entry rowsep="1" colname="col11">28.1</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1"/>  
         <oasis:entry colname="col2">Tejas I</oasis:entry>  
         <oasis:entry colname="col3">60</oasis:entry>  
         <oasis:entry colname="col4">39</oasis:entry>  
         <oasis:entry colname="col5">early Tejas II</oasis:entry>  
         <oasis:entry colname="col6">Lutetian–Bartonian</oasis:entry>  
         <oasis:entry colname="col7">49</oasis:entry>  
         <oasis:entry colname="col8">37</oasis:entry>  
         <oasis:entry colname="col9">45</oasis:entry>  
         <oasis:entry colname="col10">47.8</oasis:entry>  
         <oasis:entry colname="col11">37.8</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">  
         <oasis:entry colname="col1"/>  
         <oasis:entry colname="col2"/>  
         <oasis:entry colname="col3"/>  
         <oasis:entry colname="col4"/>  
         <oasis:entry colname="col5">early Tejas I</oasis:entry>  
         <oasis:entry colname="col6">Thanetian–Ypresian</oasis:entry>  
         <oasis:entry colname="col7">58</oasis:entry>  
         <oasis:entry colname="col8">49</oasis:entry>  
         <oasis:entry colname="col9">53</oasis:entry>  
         <oasis:entry colname="col10">59.2</oasis:entry>  
         <oasis:entry colname="col11">47.8</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">Mesozoic</oasis:entry>  
         <oasis:entry colname="col2">Zuni III</oasis:entry>  
         <oasis:entry colname="col3">96</oasis:entry>  
         <oasis:entry colname="col4">60</oasis:entry>  
         <oasis:entry colname="col5">late Zuni IV</oasis:entry>  
         <oasis:entry colname="col6">middle Campanian–Selandian (Late Cretaceous–earliest Paleogene)</oasis:entry>  
         <oasis:entry colname="col7">81</oasis:entry>  
         <oasis:entry colname="col8">58</oasis:entry>  
         <oasis:entry colname="col9">76</oasis:entry>  
         <oasis:entry colname="col10"><italic>79.8</italic></oasis:entry>  
         <oasis:entry colname="col11">59.2</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1"/>  
         <oasis:entry rowsep="1" colname="col2"/>  
         <oasis:entry rowsep="1" colname="col3"/>  
         <oasis:entry rowsep="1" colname="col4"/>  
         <oasis:entry rowsep="1" colname="col5">late Zuni III</oasis:entry>  
         <oasis:entry rowsep="1" colname="col6">late Cenomanian–early Campanian (Late Cretaceous)</oasis:entry>  
         <oasis:entry rowsep="1" colname="col7">94</oasis:entry>  
         <oasis:entry rowsep="1" colname="col8">81</oasis:entry>  
         <oasis:entry rowsep="1" colname="col9">90</oasis:entry>  
         <oasis:entry rowsep="1" colname="col10"><italic>96.1</italic></oasis:entry>  
         <oasis:entry rowsep="1" colname="col11"><italic>79.8</italic></oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1"/>  
         <oasis:entry colname="col2">Zuni II</oasis:entry>  
         <oasis:entry colname="col3">134</oasis:entry>  
         <oasis:entry colname="col4">96</oasis:entry>  
         <oasis:entry colname="col5">late Zuni II</oasis:entry>  
         <oasis:entry colname="col6">late Aptian–middle Cenomanian (Early Cretaceous–earliest Late Cretaceous)</oasis:entry>  
         <oasis:entry colname="col7">117</oasis:entry>  
         <oasis:entry colname="col8">94</oasis:entry>  
         <oasis:entry colname="col9">105</oasis:entry>  
         <oasis:entry colname="col10"><italic>119.0</italic></oasis:entry>  
         <oasis:entry colname="col11"><italic>96.1</italic></oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1"/>  
         <oasis:entry rowsep="1" colname="col2"/>  
         <oasis:entry rowsep="1" colname="col3"/>  
         <oasis:entry rowsep="1" colname="col4"/>  
         <oasis:entry rowsep="1" colname="col5">late Zuni I</oasis:entry>  
         <oasis:entry rowsep="1" colname="col6">late Valanginian–early Aptian (Early Cretaceous)</oasis:entry>  
         <oasis:entry rowsep="1" colname="col7">135</oasis:entry>  
         <oasis:entry rowsep="1" colname="col8">117</oasis:entry>  
         <oasis:entry rowsep="1" colname="col9">126</oasis:entry>  
         <oasis:entry rowsep="1" colname="col10"><italic>136.4</italic></oasis:entry>  
         <oasis:entry rowsep="1" colname="col11"><italic>119.0</italic></oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1"/>  
         <oasis:entry colname="col2">Zuni I</oasis:entry>  
         <oasis:entry colname="col3">186</oasis:entry>  
         <oasis:entry colname="col4">134</oasis:entry>  
         <oasis:entry colname="col5">early Zuni III</oasis:entry>  
         <oasis:entry colname="col6">late Tithonian–early Valanginian (latest Late Jurassic–earliest Early Cretaceous)</oasis:entry>  
         <oasis:entry colname="col7">146</oasis:entry>  
         <oasis:entry colname="col8">135</oasis:entry>  
         <oasis:entry colname="col9">140</oasis:entry>  
         <oasis:entry colname="col10"><italic>147.4</italic></oasis:entry>  
         <oasis:entry colname="col11"><italic>136.4</italic></oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1"/>  
         <oasis:entry colname="col2"/>  
         <oasis:entry colname="col3"/>  
         <oasis:entry colname="col4"/>  
         <oasis:entry colname="col5">early Zuni II</oasis:entry>  
         <oasis:entry colname="col6">late Bathonian–middle Tithonian (earliest Middle Jurassic–Late Jurassic)</oasis:entry>  
         <oasis:entry colname="col7">166</oasis:entry>  
         <oasis:entry colname="col8">146</oasis:entry>  
         <oasis:entry colname="col9">152</oasis:entry>  
         <oasis:entry colname="col10"><italic>166.8</italic></oasis:entry>  
         <oasis:entry colname="col11"><italic>147.4</italic></oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1"/>  
         <oasis:entry rowsep="1" colname="col2"/>  
         <oasis:entry rowsep="1" colname="col3"/>  
         <oasis:entry rowsep="1" colname="col4"/>  
         <oasis:entry rowsep="1" colname="col5">early Zuni I</oasis:entry>  
         <oasis:entry rowsep="1" colname="col6">middle Aalenian–middle Bathonian (Middle Jurassic)</oasis:entry>  
         <oasis:entry rowsep="1" colname="col7">179</oasis:entry>  
         <oasis:entry rowsep="1" colname="col8">166</oasis:entry>  
         <oasis:entry rowsep="1" colname="col9">169</oasis:entry>  
         <oasis:entry rowsep="1" colname="col10"><italic>172.8</italic></oasis:entry>  
         <oasis:entry rowsep="1" colname="col11"><italic>166.8</italic></oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1"/>  
         <oasis:entry colname="col2">Absaroka III</oasis:entry>  
         <oasis:entry colname="col3">245</oasis:entry>  
         <oasis:entry colname="col4">186</oasis:entry>  
         <oasis:entry colname="col5">late Absaroka III</oasis:entry>  
         <oasis:entry colname="col6">late Hettangian–early Aalenian (Early Jurassic–earliest Middle Jurassic)</oasis:entry>  
         <oasis:entry colname="col7">203</oasis:entry>  
         <oasis:entry colname="col8">179</oasis:entry>  
         <oasis:entry colname="col9">195</oasis:entry>  
         <oasis:entry colname="col10"><italic>200.0</italic></oasis:entry>  
         <oasis:entry colname="col11"><italic>172.8</italic></oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1"/>  
         <oasis:entry colname="col2"/>  
         <oasis:entry colname="col3"/>  
         <oasis:entry colname="col4"/>  
         <oasis:entry colname="col5">late Absaroka II</oasis:entry>  
         <oasis:entry colname="col6">late Carnian–middle Hettangian (Late Triassic–earliest Jurassic)</oasis:entry>  
         <oasis:entry colname="col7">224</oasis:entry>  
         <oasis:entry colname="col8">203</oasis:entry>  
         <oasis:entry colname="col9">218</oasis:entry>  
         <oasis:entry colname="col10"><italic>232</italic></oasis:entry>  
         <oasis:entry colname="col11"><italic>200.0</italic></oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">  
         <oasis:entry colname="col1"/>  
         <oasis:entry colname="col2"/>  
         <oasis:entry colname="col3"/>  
         <oasis:entry colname="col4"/>  
         <oasis:entry colname="col5">late Absaroka I</oasis:entry>  
         <oasis:entry colname="col6">Induan–early Carnian (Early–earliest Late Triassic)</oasis:entry>  
         <oasis:entry colname="col7">248</oasis:entry>  
         <oasis:entry colname="col8">224</oasis:entry>  
         <oasis:entry colname="col9">232</oasis:entry>  
         <oasis:entry colname="col10">252.17</oasis:entry>  
         <oasis:entry colname="col11"><italic>232</italic></oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">Paleozoic</oasis:entry>  
         <oasis:entry colname="col2">Absaroka II</oasis:entry>  
         <oasis:entry colname="col3">268</oasis:entry>  
         <oasis:entry colname="col4">245</oasis:entry>  
         <oasis:entry colname="col5">early Absaroka IV</oasis:entry>  
         <oasis:entry colname="col6">Roadian–Changhsingian (Late Permian)</oasis:entry>  
         <oasis:entry colname="col7">269</oasis:entry>  
         <oasis:entry colname="col8">248</oasis:entry>  
         <oasis:entry colname="col9">255</oasis:entry>  
         <oasis:entry colname="col10">272.3</oasis:entry>  
         <oasis:entry colname="col11">252.17</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1"/>  
         <oasis:entry rowsep="1" colname="col2"/>  
         <oasis:entry rowsep="1" colname="col3"/>  
         <oasis:entry rowsep="1" colname="col4"/>  
         <oasis:entry rowsep="1" colname="col5">early Absaroka III</oasis:entry>  
         <oasis:entry rowsep="1" colname="col6">Sakmarian–Kungurian (Early Permian)</oasis:entry>  
         <oasis:entry rowsep="1" colname="col7">285</oasis:entry>  
         <oasis:entry rowsep="1" colname="col8">269</oasis:entry>  
         <oasis:entry rowsep="1" colname="col9">277</oasis:entry>  
         <oasis:entry rowsep="1" colname="col10">295.0</oasis:entry>  
         <oasis:entry rowsep="1" colname="col11">272.3</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1"/>  
         <oasis:entry colname="col2">Absaroka I</oasis:entry>  
         <oasis:entry colname="col3">330</oasis:entry>  
         <oasis:entry colname="col4">268</oasis:entry>  
         <oasis:entry colname="col5">early Absaroka II</oasis:entry>  
         <oasis:entry colname="col6">Gzhelian–Asselian (latest Carboniferous–earliest Permian)</oasis:entry>  
         <oasis:entry colname="col7">296</oasis:entry>  
         <oasis:entry colname="col8">285</oasis:entry>  
         <oasis:entry colname="col9">287</oasis:entry>  
         <oasis:entry colname="col10">303.7</oasis:entry>  
         <oasis:entry colname="col11">295.0</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1"/>  
         <oasis:entry rowsep="1" colname="col2"/>  
         <oasis:entry rowsep="1" colname="col3"/>  
         <oasis:entry rowsep="1" colname="col4"/>  
         <oasis:entry rowsep="1" colname="col5">early Absaroka I</oasis:entry>  
         <oasis:entry rowsep="1" colname="col6">Bashkirian–Kasimovian (Late Carboniferous)</oasis:entry>  
         <oasis:entry rowsep="1" colname="col7">323</oasis:entry>  
         <oasis:entry rowsep="1" colname="col8">296</oasis:entry>  
         <oasis:entry rowsep="1" colname="col9">302</oasis:entry>  
         <oasis:entry rowsep="1" colname="col10">323.2</oasis:entry>  
         <oasis:entry rowsep="1" colname="col11">303.7</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1"/>  
         <oasis:entry colname="col2">Kaskaskia II</oasis:entry>  
         <oasis:entry colname="col3">362</oasis:entry>  
         <oasis:entry colname="col4">330</oasis:entry>  
         <oasis:entry colname="col5">Kaskaskia IV</oasis:entry>  
         <oasis:entry colname="col6">middle Visean–Serpukhovian (Lower Carboniferous)</oasis:entry>  
         <oasis:entry colname="col7">338</oasis:entry>  
         <oasis:entry colname="col8">323</oasis:entry>  
         <oasis:entry colname="col9">328</oasis:entry>  
         <oasis:entry colname="col10"><italic>341.4</italic></oasis:entry>  
         <oasis:entry colname="col11">323.2</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1"/>  
         <oasis:entry rowsep="1" colname="col2"/>  
         <oasis:entry rowsep="1" colname="col3"/>  
         <oasis:entry rowsep="1" colname="col4"/>  
         <oasis:entry rowsep="1" colname="col5">Kaskaskia III</oasis:entry>  
         <oasis:entry rowsep="1" colname="col6">late Famennian–early Visean (latest Devonian–Early Carboniferous)</oasis:entry>  
         <oasis:entry rowsep="1" colname="col7">359</oasis:entry>  
         <oasis:entry rowsep="1" colname="col8">338</oasis:entry>  
         <oasis:entry rowsep="1" colname="col9">348</oasis:entry>  
         <oasis:entry rowsep="1" colname="col10"><italic>365.6</italic></oasis:entry>  
         <oasis:entry rowsep="1" colname="col11"><italic>341.4</italic></oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1"/>  
         <oasis:entry colname="col2">Kaskaskia I</oasis:entry>  
         <oasis:entry colname="col3">401</oasis:entry>  
         <oasis:entry colname="col4">362</oasis:entry>  
         <oasis:entry colname="col5">Kaskaskia II</oasis:entry>  
         <oasis:entry colname="col6">Givetian–early Famennian (Middle–Late Devonian)</oasis:entry>  
         <oasis:entry colname="col7">380</oasis:entry>  
         <oasis:entry colname="col8">359</oasis:entry>  
         <oasis:entry colname="col9">368</oasis:entry>  
         <oasis:entry colname="col10">387.7</oasis:entry>  
         <oasis:entry colname="col11"><italic>365.6</italic></oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1"/>  
         <oasis:entry colname="col2"/>  
         <oasis:entry colname="col3"/>  
         <oasis:entry colname="col4"/>  
         <oasis:entry colname="col5">Kaskaskia I</oasis:entry>  
         <oasis:entry colname="col6">late Pragian–Eifelian (Early–Middle Devonian)</oasis:entry>  
         <oasis:entry colname="col7">402</oasis:entry>  
         <oasis:entry colname="col8">380</oasis:entry>  
         <oasis:entry colname="col9">396</oasis:entry>  
         <oasis:entry colname="col10"><italic>408.7</italic></oasis:entry>  
         <oasis:entry colname="col11">387.7</oasis:entry>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup><?xmltex \end{scaleboxenv}?></oasis:table></table-wrap>

      <?xmltex \floatpos{t}?><fig id="Ch1.F1" specific-use="star"><caption><p id="d1e1171">Global distributions and number of
fossil collections since the Devonian. The greyscale background shows global
present-day topography ETOPO1 (Amante and Eakins, 2009) with lighter shades
corresponding to increasing elevation. Fossil collections from the PBDB are
colored following the standard used by the International Commission on
Stratigraphy.</p></caption>
        <?xmltex \igopts{width=398.338583pt}?><graphic xlink:href="https://bg.copernicus.org/articles/14/5425/2017/bg-14-5425-2017-f01.png"/>

      </fig>

      <p id="d1e1181">The paleogeographic maps of Golonka et al. (2006) are constructed using a
plate tectonic model available in the supplement of Golonka (2007a), where
relative plate motions are described. In this rotation model, paleomagnetic
data are used to constrain the paleolatitudinal positions of continents and
rotation of plates, and hotspots, where applicable, are used as reference
points to calculate paleolongtitudes (Golonka, 2007a). This rotation model
is necessary to restore these paleogeographic geometries (Golonka et al.,
2006) to their present-day coordinates so that they can be attached to a
different plate motion model. The relative plate motions of Golonka (2006,
2007a) are based on the reconstruction of Scotese (1997, 2004).</p>
      <p id="d1e1184">Here, we use a global plate kinematic model to reconstruct paleogeographies
back in time from present-day locations. The global tectonic reconstruction
of Matthews et al. (2016), with continuously closing plate boundaries from
410–0 Ma, is primarily constructed from a Mesozoic and Cenozoic plate model
(230–0 Ma; Müller et al., 2016) and a Paleozoic model (410–250 Ma; Domeier and Torsvik, 2014). This model is a relative plate motion model that
is ultimately tied to Earth's spin axis through a paleomagnetic reference
frame for times before 70 Ma, and a moving hotspot reference frame for
younger times (Matthews et al., 2016).</p>
      <p id="d1e1187">The PBDB is a compilation of global fossil data covering deep geological
time. All fossil collections in the database contain detailed metadata,
including on the time range (typically biostratigraphic age), present-day
geographic coordinates, host lithology and paleoenvironment. Figure 1
represents distributions of the global fossil collections at present-day
coordinates and shows their numbers since the Devonian. The recorded
fossil collections are unevenly distributed both spatially and temporally,
largely due to the differences in fossil preservation, the spatial sampling
biases of fossil localities and the uneven entry of fossil data to the PBDB
(Alroy, 2010). For this study, a total of 57 854 fossil collections with
temporal and paleoenvironmental assignments from 402 to 2 Ma were
downloaded from the database on 7 September 2016.</p>
</sec>
<sec id="Ch1.S3">
  <title>Methods</title>
      <p id="d1e1196">The methodology can be divided into three main steps: (1) the original
paleogeographic geometries are restored to present-day coordinates by
applying the inverse of the rotations used to make the reconstruction, (2) these restored geometries are then rotated to new locations using the plate
tectonic model of Matthews et al. (2016) and (3) the paleo-coastline locations
and paleogeographic geometries are adjusted using paleoenvironmental data
from the PBDB. Figure 2 illustrates the generalized workflow that can be
applied to a different paleogeography model. In order to represent the
paleogeographic maps as digital geographic geometries, they are first
georeferenced using the original projection and coordinate system (global
Mollweide in Golonka et al., 2006), and then re-projected into the WGS84
geographic coordinate system. The resulting maps are then attached to the
original rotation model using the open-source and cross-platform plate
reconstruction software <italic>GPlates</italic> (<uri>http://gplates.org</uri>). Every plate is then assigned a
unique plate ID that defines the rotation of the tectonic elements so that
the paleogeographic geometries can be rotated back to their present-day
coordinates (see example in Fig. 3a, b). We use present-day coastlines and
terrane boundaries with the plate IDs of Golonka (2007a) as a reference to
refine the rotations and ensure that the paleogeographic geometries are
restored accurately to their present-day locations.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F2"><caption><p id="d1e1207">Workflow used to transfer a set of paleogeographic geometries from
one reconstruction to another, followed by revision using
paleoenvironmental information indicated by marine fossil collections from
the Paleobiology Database (PBDB).</p></caption>
        <?xmltex \igopts{width=239.00315pt}?><graphic xlink:href="https://bg.copernicus.org/articles/14/5425/2017/bg-14-5425-2017-f02.png"/>

      </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F3" specific-use="star"><caption><p id="d1e1218"><bold>(a)</bold> Original global paleogeographic map from Golonka et al. (2006)
at 126 Ma. <bold>(b)</bold> Global paleogeographic geometries at 126 Ma in present-day
coordinates. <bold>(c)</bold> Global paleogeography at 126 Ma reconstructed using the
plate motion model of Matthews et al. (2016). Gaps are highlighted in pink.
<bold>(d)</bold> Global paleogeography at 126 Ma reconstructed using the reconstruction
of Matthews et al. (2016) with gaps fixed by filling with adjacent
paleoenvironment attributes. Grey lines indicate reconstructed present-day
coastlines and terrane boundaries. Mollweide projection with 0<inline-formula><mml:math id="M2" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E central meridian.</p></caption>
        <?xmltex \igopts{width=369.885827pt}?><graphic xlink:href="https://bg.copernicus.org/articles/14/5425/2017/bg-14-5425-2017-f03.png"/>

      </fig>

<?xmltex \floatpos{t}?><table-wrap id="Ch1.T2" specific-use="star"><caption><p id="d1e1251">Lookup table to classify fossil data indicating different
paleoenvironments into marine or terrestrial settings and their
corresponding paleogeographic types presented in Golonka et al. (2006).
Terrestrial fossil paleoenvironments correspond to paleogeographic features
of landmasses, mountains or ice sheets and marine fossil paleoenvironments
to shallow marine environments or deep oceans.</p></caption><oasis:table frame="topbot"><?xmltex \begin{scaleboxenv}{.80}[.80]?><oasis:tgroup cols="6">
     <oasis:colspec colnum="1" colname="col1" align="center" colsep="1"/>
     <oasis:colspec colnum="2" colname="col2" align="left"/>
     <oasis:colspec colnum="3" colname="col3" align="left" colsep="1"/>
     <oasis:colspec colnum="4" colname="col4" align="center" colsep="1"/>
     <oasis:colspec colnum="5" colname="col5" align="left"/>
     <oasis:colspec colnum="6" colname="col6" align="left"/>
     <oasis:thead>
       <oasis:row rowsep="1">

         <oasis:entry namest="col1" nameend="col3" colsep="1">Marine </oasis:entry>

         <oasis:entry namest="col4" nameend="col6" colsep="0">Terrestrial/transitional zone </oasis:entry>

       </oasis:row>
       <oasis:row rowsep="1">

         <oasis:entry colname="col1">Paleogeography</oasis:entry>

         <oasis:entry namest="col2" nameend="col3" align="center" colsep="1">Fossil paleoenvironments </oasis:entry>

         <oasis:entry colname="col4">Paleogeography</oasis:entry>

         <oasis:entry namest="col5" nameend="col6" align="center" colsep="1">Fossil paleoenvironments </oasis:entry>

       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row>
       <?xmltex \rotentry?>
         <oasis:entry colname="col1" morerows="18">shallow marine environments/deep oceans</oasis:entry>

         <oasis:entry colname="col2">marine indet.</oasis:entry>

         <oasis:entry colname="col3">slope</oasis:entry>
       <?xmltex \rotentry?>
         <oasis:entry rowsep="1" colname="col4" morerows="17">Landmasses/mountains</oasis:entry>

         <oasis:entry colname="col5">terrestrial indet.</oasis:entry>

         <oasis:entry colname="col6">pond</oasis:entry>

       </oasis:row>
       <oasis:row>

         <oasis:entry colname="col2">carbonate indet.</oasis:entry>

         <oasis:entry colname="col3">basinal (carbonate)</oasis:entry>

         <oasis:entry colname="col5">fluvial indet.</oasis:entry>

         <oasis:entry colname="col6">crater lake</oasis:entry>

       </oasis:row>
       <oasis:row>

         <oasis:entry colname="col2">peritidal</oasis:entry>

         <oasis:entry colname="col3">basinal (siliceous)</oasis:entry>

         <oasis:entry colname="col5">alluvial fan</oasis:entry>

         <oasis:entry colname="col6">lacustrine delta plain</oasis:entry>

       </oasis:row>
       <oasis:row>

         <oasis:entry colname="col2">shallow subtidal indet.</oasis:entry>

         <oasis:entry colname="col3">marginal marine indet.</oasis:entry>

         <oasis:entry colname="col5">channel lag</oasis:entry>

         <oasis:entry colname="col6">lacustrine interdistributary bay</oasis:entry>

       </oasis:row>
       <oasis:row>

         <oasis:entry colname="col2">open shallow subtidal</oasis:entry>

         <oasis:entry colname="col3">coastal indet.</oasis:entry>

         <oasis:entry colname="col5">coarse channel fill</oasis:entry>

         <oasis:entry colname="col6">lacustrine delta front</oasis:entry>

       </oasis:row>
       <oasis:row>

         <oasis:entry colname="col2">lagoonal/restricted shallow subtidal</oasis:entry>

         <oasis:entry colname="col3">estuary/bay</oasis:entry>

         <oasis:entry colname="col5">fine channel fill</oasis:entry>

         <oasis:entry colname="col6">lacustrine prodelta</oasis:entry>

       </oasis:row>
       <oasis:row>

         <oasis:entry colname="col2">sand shoal</oasis:entry>

         <oasis:entry colname="col3">lagoonal</oasis:entry>

         <oasis:entry colname="col5">channel</oasis:entry>

         <oasis:entry colname="col6">lacustrine deltaic indet.</oasis:entry>

       </oasis:row>
       <oasis:row>

         <oasis:entry colname="col2">reef, buildup or bioherm</oasis:entry>

         <oasis:entry colname="col3">paralic indet.</oasis:entry>

         <oasis:entry colname="col5">wet floodplain</oasis:entry>

         <oasis:entry colname="col6">lacustrine indet.</oasis:entry>

       </oasis:row>
       <oasis:row>

         <oasis:entry colname="col2">peri-reef or sub-reef</oasis:entry>

         <oasis:entry colname="col3">interdistributary bay</oasis:entry>

         <oasis:entry colname="col5">dry floodplain</oasis:entry>

         <oasis:entry colname="col6">dune</oasis:entry>

       </oasis:row>
       <oasis:row>

         <oasis:entry colname="col2">intra-shelf/intraplatform reef</oasis:entry>

         <oasis:entry colname="col3">delta front</oasis:entry>

         <oasis:entry colname="col5">floodplain</oasis:entry>

         <oasis:entry colname="col6">inter-dune</oasis:entry>

       </oasis:row>
       <oasis:row>

         <oasis:entry colname="col2">platform/shelf-margin reef</oasis:entry>

         <oasis:entry colname="col3">prodelta</oasis:entry>

         <oasis:entry colname="col5">crevasse splay</oasis:entry>

         <oasis:entry colname="col6">loess</oasis:entry>

       </oasis:row>
       <oasis:row>

         <oasis:entry colname="col2">slope/ramp reef</oasis:entry>

         <oasis:entry colname="col3">deltaic indet.</oasis:entry>

         <oasis:entry colname="col5">levee</oasis:entry>

         <oasis:entry colname="col6">eolian indet.</oasis:entry>

       </oasis:row>
       <oasis:row>

         <oasis:entry colname="col2">basin reef</oasis:entry>

         <oasis:entry colname="col3">foreshore</oasis:entry>

         <oasis:entry colname="col5">mire/swamp</oasis:entry>

         <oasis:entry colname="col6">cave</oasis:entry>

       </oasis:row>
       <oasis:row>

         <oasis:entry colname="col2">deep subtidal ramp</oasis:entry>

         <oasis:entry colname="col3">shore face</oasis:entry>

         <oasis:entry colname="col5">fluvial–lacustrine indet.</oasis:entry>

         <oasis:entry colname="col6">fissure fill</oasis:entry>

       </oasis:row>
       <oasis:row>

         <oasis:entry colname="col2">deep subtidal shelf</oasis:entry>

         <oasis:entry colname="col3">transition zone/lower shore face</oasis:entry>

         <oasis:entry colname="col5">delta plain</oasis:entry>

         <oasis:entry colname="col6">sinkhole</oasis:entry>

       </oasis:row>
       <oasis:row>

         <oasis:entry colname="col2">deep subtidal indet.</oasis:entry>

         <oasis:entry colname="col3">offshore</oasis:entry>

         <oasis:entry colname="col5">fluvial–deltaic indet.</oasis:entry>

         <oasis:entry colname="col6">karst indet.</oasis:entry>

       </oasis:row>
       <oasis:row>

         <oasis:entry colname="col2">offshore ramp</oasis:entry>

         <oasis:entry colname="col3">submarine fan</oasis:entry>

         <oasis:entry colname="col5">lacustrine – large</oasis:entry>

         <oasis:entry colname="col6">tar</oasis:entry>

       </oasis:row>
       <oasis:row>

         <oasis:entry colname="col2">offshore shelf</oasis:entry>

         <oasis:entry colname="col3">basinal (siliciclastic)</oasis:entry>

         <oasis:entry rowsep="1" colname="col5">lacustrine – small</oasis:entry>

         <oasis:entry rowsep="1" colname="col6">spring</oasis:entry>

       </oasis:row>
       <oasis:row>

         <oasis:entry colname="col2">offshore indet.</oasis:entry>

         <oasis:entry colname="col3">deep-water indet.</oasis:entry>

         <oasis:entry colname="col4">ice sheets</oasis:entry>

         <oasis:entry namest="col5" nameend="col6" colsep="1">glacial </oasis:entry>

       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup><?xmltex \end{scaleboxenv}?></oasis:table></table-wrap>

      <p id="d1e1601">When the paleogeographic geometries in present-day coordinates are attached
to a new reconstruction model, as Matthews et al. (2016) used in this study,
the resulting paleogeographies result in gaps (Fig. 3c, pink) and overlaps
between neighboring polygons, when compared to the original reconstruction
(Fig. 3a). These gaps and overlaps essentially arise from the differences in
the reconstructions described in Matthews et al. (2016) and Golonka et al. (2006). The reconstruction of Golonka et al. (2006) has a tighter fit of the
major continents within Pangea prior to the supercontinent breakup. In
addition, this reconstruction contains a different plate motion history and
block boundary definitions in regions of complex continental deformation,
for example along active continental margins (e.g., Himalayas, western North
America; Fig. 3c).</p>
      <p id="d1e1604">The gaps and overlaps cause changes in the total terrestrial or oceanic
paleogeographic areas at different time intervals, becoming larger or
smaller, when compared with the original paleogeographic maps (Golonka et
al., 2006). The gaps can be fixed by interactively extending the outlines of
the polygons in a GIS platform to make the plates connect as in the original
paleogeographic maps (Fig. 3a, c, d). Changes in the extent of total
terrestrial or oceanic area of the paleogeographies with filled gaps are
compared with the original paleogeographies in Fig. 3d (Golonka et al., 2006).</p>
      <p id="d1e1607">Once the gaps are filled, the reconstructed paleogeographic features are
compared with the paleoenvironments indicated by the marine fossil
collections from the PBDB. These comparisons aim to identify the differences
between the mapped paleogeography and the marine fossil collection
environments in order to revise the paleo-coastline locations and
paleogeographic geometries. Fossil collections belonging to each time
interval (Table 1; Golonka, 2000) are first extracted from the data set
downloaded from the PBDB. Only the fossil collections with temporal ranges
lying entirely within the corresponding time intervals are selected, as
opposed to including the fossil collections that have larger temporal
ranges. Fossil collections with temporal ranges crossing any time-interval
boundary are not taken into consideration. As a result, a minimum number of
fossil collections are selected for each time interval. The selected fossil
collections are classified into either the terrestrial or marine setting
category, according to a lookup table (Table 2).</p>
      <p id="d1e1610">Marine fossil collections are then attached to the plate motion model of
Matthews et al. (2016) so they can be reconstructed at each time interval.
Subsequently, a point-in-polygon test is used to determine whether or not the
indicated marine fossil collection is within the appropriate marine
paleogeographic polygon. The results of these tests are discussed in the
following section.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F4"><caption><p id="d1e1616"><bold>(a)</bold> Test between the global paleogeography at 76 Ma reconstructed
using the plate motion model of Matthews et al. (2016) with gaps fixed and
the paleoenvironments indicated by the marine fossil collections from the
PBDB. <bold>(b)</bold> Area modified (blue) to resolve the test inconsistencies. <bold>(c)</bold> Test
between the revised paleogeography at 76 Ma and the same marine fossil
collections. Mollweide projection with 0<inline-formula><mml:math id="M3" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E central meridian.</p></caption>
        <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://bg.copernicus.org/articles/14/5425/2017/bg-14-5425-2017-f04.png"/>

      </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F5" specific-use="star"><caption><p id="d1e1644">Test between unrevised and revised paleogeography at 76 Ma, respectively, and paleoenvironments indicated by the marine fossil
collections from the PBDB, and revision of the paleo-coastlines and
paleogeographic geometries based on the test results, for southern North
America <bold>(a, b, c)</bold>, southern South America <bold>(d, e, f)</bold>, northern Africa <bold>(g, h, i)</bold> and India <bold>(j, k, l)</bold>. Regional Mollweide projection.</p></caption>
        <?xmltex \igopts{width=369.885827pt}?><graphic xlink:href="https://bg.copernicus.org/articles/14/5425/2017/bg-14-5425-2017-f05.png"/>

      </fig>

      <p id="d1e1665">In the next step, we modify the paleo-coastline locations and
paleogeographic geometries based on the test (Figs. 4, 5 and Supplement).
Modifications are made according to the following rules. (1) Marine fossil
collections from the PBDB are presumed to be well dated, constrained
geographically, not reworked and representative of their broader
paleoenvironments. Their indicative environments are assumed to be correct.
(2) Only marine fossil collections within 500 km of the nearest
paleo-coastlines are taken into account as most marine fossil collections
used in this study are located within 500 km from the paleo-coastlines (see
Fig. S1 in the Supplement). (3) The paleo-coastlines and
paleogeographic geometries are modified until they are consistent with the
marine fossil collection environments and at the same time remain about 30
km distance from the fossil points used (Fig. 5c, f, l). (4) The adjacent
paleo-coastlines are accordingly adjusted and smoothed (Figs. 4, 5). (5) The
modified area (Fig. 5b, e, k, blue) resulting from shifting the coastline is
filled using the shallow marine environment. These rules are designed to
maximize the use of the paleoenvironmental information obtained from the
marine fossil collections to improve the coastline locations and
paleogeography while attempting to minimize spurious modifications.</p>
      <p id="d1e1668">However, in some rare cases, outlier marine fossil data may be a deceptive
recorder of paleogeography. For instance, Wichura et al. (2015) discussed
the discovery of a <inline-formula><mml:math id="M4" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 17 Myr old beaked whale fossil 740 km
inland from the present-day coastline of the Indian Ocean in east
Africa. The authors found evidence to suggest that this whale could have
traveled inland from the Indian Ocean along an eastward-directed fluvial
(terrestrial) drainage system and was stranded there, rather than
representing a marine setting that would be implied under our assumptions.
Therefore, theoretically, when using the fossil collections to improve
paleogeography, additional concerns about living habits of fossils and
associated geological settings should be taken into account. In this study,
we have removed this misleading fossil whale from the data set. Such
instances of deceptive fossil data are a potential limitation within our
workflow, which we seek to minimize by excluding inconsistent fossils more
than 500 km away from previously interpreted paleo-coastlines described
above.
<?xmltex \hack{\newpage}?></p>
</sec>
<sec id="Ch1.S4">
  <title>Results</title>
<sec id="Ch1.S4.SS1">
  <title>Paleoenvironmental tests</title>
      <p id="d1e1691">Global reconstructed paleogeographic maps from 402 to 2 Ma are tested
against paleoenvironments indicated by the marine fossil collections that
are reconstructed in the same rotation model (Matthews et al., 2016). The
consistency ratio is defined by the marine fossil collections within shallow
marine or deep ocean paleogeographic polygons as a percentage of all marine
fossil collections at the time interval, and in contrast, the inconsistency
ratio is defined by the marine fossil collections not within shallow marine or deep
ocean paleogeography as a percentage of all marine fossil collections. Heine
et al. (2015) used a similar metric to evaluate global paleo-coastline models
since the Cretaceous.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F6"><caption><p id="d1e1696"><bold>(a)</bold> Consistency ratios between global paleogeography with gap
filled, but before PBDB test for the period 402–2 Ma, reconstructed using
the plate motion model of Matthews et al. (2016) and the paleoenvironments
indicated by the marine fossil collections from the PBDB. <bold>(b)</bold> Numbers of
consistent (light grey) and inconsistent (dark grey) marine fossil
collections used in the tests for each time interval from 402 to 2 Ma.</p></caption>
          <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://bg.copernicus.org/articles/14/5425/2017/bg-14-5425-2017-f06.png"/>

        </fig>

      <p id="d1e1710">The inconsistent marine fossil collections are used to modify coastlines and
paleogeographic geometries according to the rules outlined in the Methods
section. The consistency ratios of marine fossil collections during 402–2 Ma are all over 55 %, with an average of 75 % (Fig. 6a, shaded area)
although with large fluctuations over time (Fig. 6). This indicates that the
paleogeography of Golonka et al. (2006) has relatively high consistency with
the fossil records. However, 52 fossil collections over all time intervals
cannot be resolved as they are over 500 km distant from the nearest
coastline (for example, red points in Fig. 5c, l). Therefore, in some cases,
the paleogeography cannot be fully reconciled with the paleobiology (see
Supplement). The results since the Cretaceous are similar to that of Heine
et al. (2015).</p>
      <p id="d1e1713">The sums of marine fossil collections change significantly over time (Fig. 6b); for example, there are more than 4000 in total within 269–248 Ma but only 20
during 37–29 Ma. These variations are due to the spatiotemporal sampling
bias and incompleteness of the fossil record (Benton et al., 2000; Benson
and Upchurch, 2013; Smith et al., 2012; Valentine et al., 2006; Wright et
al., 2013), biota extinction and recovery (Hallam and Wignall, 1997; Hart,
1996), the uneven entry of fossil data to the PBDB (Alroy, 2010) and our
temporal selection criterion. In addition, the differences in the duration
of geological time subdivisions lead to some time intervals having shorter
time spans that contain fewer fossil records, which we discuss in a later
section. As for the time intervals during which fossil data are scarce, the
fossil collections are of limited use in improving paleogeography. However,
additional records in the future will increase the usefulness of the PBDB in
such instances.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F7" specific-use="star"><caption><p id="d1e1719">Global paleogeography from 402 to 2 Ma reconstructed using the
plate motion model of Matthews et al. (2016) and revised using
paleoenvironmental data from the PBDB. Black dotted lines indicate
subduction zones, and other black lines denote mid-ocean ridges and
transforms. Grey outlines delineate reconstructed present-day coastlines and
terranes. Mollweide projection with 0<inline-formula><mml:math id="M5" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E central meridian.</p></caption>
          <?xmltex \igopts{width=421.100787pt}?><graphic xlink:href="https://bg.copernicus.org/articles/14/5425/2017/bg-14-5425-2017-f07-part01.png"/>

        </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F8" specific-use="star"><caption><p id="d1e1739">(continued)</p></caption>
          <?xmltex \hack{\addtocounter{figure}{-1}}?>
          <?xmltex \igopts{width=421.100787pt}?><graphic xlink:href="https://bg.copernicus.org/articles/14/5425/2017/bg-14-5425-2017-f07-part02.png"/>

        </fig>

</sec>
<sec id="Ch1.S4.SS2">
  <title>Revised global reconstructed paleogeography</title>
      <p id="d1e1756">Based on the PBDB test results at all the time intervals, we can revise the
inferred paleo-coastlines and paleogeographic geometries using the approach
described in the Methods section. As a result, the revised paleo-coastlines
and paleogeographies are significantly improved, mainly in the regions of
North America, South America, Europe and Africa during the Late Carboniferous,
Middle Permian, Triassic, Jurassic, Late Cretaceous and most of Cenozoic
(Figs. 4, 5, 6 and Supplement). The resulting improved global
paleogeographic maps since the Devonian are presented in Fig. 7. They
provide improved paleo-coastlines that are important to constrain past
changes in sea level and long-wavelength dynamic topography.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F9"><caption><p id="d1e1761">Global paleogeographic feature areas as percentages of Earth's total
surface area estimated from the revised paleogeographic maps from 402 Ma to
2 Ma.</p></caption>
          <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://bg.copernicus.org/articles/14/5425/2017/bg-14-5425-2017-f08.png"/>

        </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F10"><caption><p id="d1e1772">Global flooded continental area since the Early Devonian from
the original paleogeographic maps of Golonka et al. (2006; grey solid line)
and from the revised paleogeography in this study (pink line). Results for
Blakey (2003, 2008), Golonka (2007b, 2009, 2012), Ronov (1994), Smith et al. (2004) and Walker et al. (2002) are as in van der Meer et al. (2017). The van
der Meer et al. (2017) curve (green line) is derived from the strontium
isotope record of marine carbonates.</p></caption>
          <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://bg.copernicus.org/articles/14/5425/2017/bg-14-5425-2017-f09.png"/>

        </fig>

      <p id="d1e1782">We subsequently calculate the area covered by each paleogeographic feature
as a percentage of Earth's total surface area at each time interval from 402 to 2 Ma (Fig. 8), using the HEALPix pixelization method that results in
equal sampling of data on a sphere (Górski et al., 2005) and therefore
equal sampling of surface areas. This method effectively excludes the effect
of overlaps between paleogeographic geometries.</p>
      <p id="d1e1785">As a result, the areas of landmass, mountain and ice sheet generally
indicate increasing trends, while shallow marine and deep ocean areas show
decreasing trends through geological time (Fig. 8). Overall, the computed
areas increase in the following order: ice sheet (average 1.0 % of Earth surface),
mountain belts (3.4 %), shallow marine (14.3 %), landmass (21.3 %) and
deep ocean (60.1 %). Only during the time interval of 323–296 Ma are landmass
and shallow marine areas nearly equal at about 14.0 %, and only during
359–285 Ma do ice sheet areas exceed mountain areas, but ice sheets only exist
during 380–285, 81–58 and 37–2 Ma. With Pangea formation during the
latest Carboniferous or the Early Permian and breakup initiation in the
Early Jurassic (Blakey, 2003; Domeier et al., 2012; Lenardic, 2016; Stampfli
et al., 2013; Vai, 2003; Veevers, 2004; Yeh and Shellnutt, 2016), these
paleogeographic feature areas significantly change over time (Fig. 8).
During 323–296 Ma (Late Carboniferous–earliest Permian), the landmass
extent reaches its smallest area (13.6 %) and subsequently undergoes a
rapid increase until peaking at 26.6 % between 224 and 203 Ma (Late
Triassic). In contrast, ice sheets reach their largest area (7.2 %)
between 323 and 296 Ma. In the Early Jurassic of Pangea breakup, landmass area
rapidly decreases from 26.6 % between 224 and 203 Ma to 23.5 % between
203 and 179 Ma, but shallow marine area increases by 3.7 %.</p>
</sec>
</sec>
<sec id="Ch1.S5">
  <title>Discussions</title>
<sec id="Ch1.S5.SS1">
  <title>Global flooded continental areas</title>
      <p id="d1e1800">We estimate the global flooded continental areas since the Early Devonian
from the revised paleogeography in this study (Fig. 9, pink solid line) and
from the original paleogeographic maps of Golonka et al. (2006; Fig. 9,
grey solid line). Both sets of results are similar, with a decrease during
Pangea amalgamation from the Late Devonian until the Late
Carboniferous, increase from the Early Jurassic with the breakup of
Pangea until the Late Cretaceous and then a decrease again until the
Pleistocene. We compare the two curves (pink solid line, grey
solid line; Fig. 9) to the results of other studies (Fig. 9; Ronov, 1994; Smith et
al., 1994; Walker et al., 2002; Blakey, 2003, 2008; Golonka, 2007b, 2009,
2012) derived from independent paleoenvironment and paleo-lithofacies data.
The results are generally consistent, except for the periods 338–269 Ma and
248–203 Ma, during which the flooded continental areas for this study and
Golonka et al. (2006) are smaller, reflecting smaller extent of
transgression in these times. Van der Meer et al. (2017, green line in Fig. 9) derived sea level and continental flooding from the strontium isotope
record of marine carbonates. These results are generally consistent with the
estimates from paleoenvironment and paleo-lithofacies data, except during
the Permian and the Late Jurassic–early Cretaceous, during which van
der Meer et al. (2017) predict larger extent of flooding than others (Fig. 9). This could indicate that the evolution of <inline-formula><mml:math id="M6" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">87</mml:mn></mml:msup></mml:math></inline-formula>Sr <inline-formula><mml:math id="M7" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M8" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">86</mml:mn></mml:msup></mml:math></inline-formula>Sr reflects
variations in the composition of emergent continental crust (Bataille et
al., 2017; Flament et al., 2013) as well as global weathering rates (e.g.,
Flament et al., 2013; Vérard et al., 2015; van der Meer et al., 2017).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F11"><caption><p id="d1e1830">Terrestrial areal change due to filling gaps and modifying the
paleo-coastlines and paleogeographic geometries over time. Green: based on
the original paleogeographic maps of Golonka et al. (2006); red: based on
paleogeography reconstructed using a different plate motion model of
Matthews et al. (2016) and gaps filled; blue: based on paleogeography with
gaps fixed and revised using the paleoenvironments indicated by marine
fossil collections from the PBDB.</p></caption>
          <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://bg.copernicus.org/articles/14/5425/2017/bg-14-5425-2017-f10.png"/>

        </fig>

</sec>
<sec id="Ch1.S5.SS2">
  <title>Terrestrial areal change associated with transferring reconstruction,
filling gaps and revising paleogeography</title>
      <p id="d1e1845">We estimate the terrestrial areas, including ice sheets, mountains and
landmasses, as percentages of Earth's surface area, from the original
paleogeography of Golonka et al. (2006; Fig. 10, green), from the
paleogeography reconstructed using a different plate motion model of
Matthews et al. (2016) and gaps filled (Fig. 10, red) and from the
paleogeography with gaps fixed and revised using the paleoenvironmental
information indicated by marine fossil collections from the PBDB (Fig. 10,
blue). These three curves are similar and generally indicate a reverse
changing trend to the flooded continental areal curves over time (Fig. 9),
as expected. We also calculate the areas of the terrestrial paleogeographic
geometries after transferring the reconstruction but before filling gaps and
the results are nearly identical to the original terrestrial paleogeographic
areas of Golonka et al. (2006). This is because the reconstruction of
Golonka et al. (2006) has a tighter fit of the major continents within
Pangea prior to the supercontinent breakup than the reconstruction of
Matthews et al. (2016), so that transferring the paleogeographic geometries
mainly produces gaps rather than overlaps. Comparing between the three
curves (Fig. 10), filling gaps results in a larger terrestrial areal change
than revising paleogeographic geometries based on PBDB test. Therefore,
variation of the underlying plate reconstruction is the main factor that
contributes to the terrestrial areal change (Fig. 10, red and green), and
the effect of revising paleogeographic geometries based on paleobiology is
secondary (Fig. 10, blue).
<?xmltex \hack{\newpage}?></p>
</sec>
<sec id="Ch1.S5.SS3">
  <title>Marine fossil collection abundances in two different timescales</title>
      <p id="d1e1855">We test the marine fossil collection data set used in this study for fossil
abundances over time with two different timescales: ICS2016 and Golonka (2000; Table 1). The results indicate the abundances of the data set in the
two timescales are significantly different in most time intervals (Fig. 11). Generally, shorter time spans contain fewer data; for
instance, there are about 400 marine fossil collections between 224 and 203 Ma using the Golonka (2000) timescale (Fig. 11, red), while there are over
1300 collections during 232–200 Ma using the ICS2016 timescale (Fig. 11, blue). In addition, the difference of the start age and end age of the time
interval could remarkably affect the fossil abundance, so that there are
over 2000 marine fossil collections between 387.7 and 365.6 Ma in ICS2016 but
fewer than 300 collections between 380 and 359 Ma using the Golonka (2000) timescale. As a result, the timescale applied to the paleobiology could
significantly affect the fossil collection abundance being assigned to
paleogeographic time intervals.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F12"><caption><p id="d1e1860">Fossil abundance test on the marine fossil collection data set used
in this study with two different timescales: Golonka (2000) and ICS2016
(Table 1).</p></caption>
          <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://bg.copernicus.org/articles/14/5425/2017/bg-14-5425-2017-f11.png"/>

        </fig>

</sec>
<sec id="Ch1.S5.SS4">
  <title>Limitations of the workflow</title>
      <p id="d1e1875">The workflow we develop in this study illustrates transferring
paleogeographic geometries from one plate motion model to another and then
using paleoenvironmental information indicated by marine fossil collections
from the PBDB to improve the paleo-coastline locations and paleogeographic
geometries. However, the methodology still has some limitations.
Transferring paleogeographic geometries to a different reconstruction
inevitably results in gaps and/or overlaps, which can only be addressed
using presently laborious methods. In addition, revising the coastlines and
paleogeographic geometries based on the PBDB test is also currently achieved
manually, and could be automated in the future.
<?xmltex \hack{\newpage}?></p>
      <p id="d1e1879">Paleogeographic maps such as those considered here typically represent
discrete time periods of many millions of years, whereas global plate motion
models, even though also based on tectonic stages, provide a somewhat more
continuous description of evolving plate configurations. A remaining
question is how to provide a continuous representation of paleogeographic
change that combines continuous plate motion models with paleogeographic
maps that do not explicitly capture changes at the same temporal resolution.
In addition, it is currently difficult to apply a timescale to the raw
paleobiology data from the PBDB that are currently not tied to any timescale. The paleoenvironmental data used here have variable temporal
resolutions, but the paleo-coastlines representing maximum transgressions
are presented in a location at specific times. However, due to the
inaccessibility of the original data that were used to build the
paleogeographic maps, we are not in a position to estimate the temporal
resolution of the original coastlines and paleogeographic maps.</p>
      <p id="d1e1882">The PBDB is a widely used resource (e.g., Wright et al., 2013; Finnegan et
al., 2015; Heim et al., 2015; Mannion et al., 2015; Nicolson et al., 2015;
Fischer et al., 2016; Tennant et al., 2016; Close et al., 2017; Zaffos et
al., 2017), yet, the spatial coverage of data is still highly heterogeneous,
with relatively few data points across large areas of the globe for some
time periods. Hence, it is important to combine it with other geological data,
such as stratigraphic data from StratDB Database (<uri>http://sil.usask.ca</uri>) and
Macrostrat Database (<uri>https://macrostrat.org/</uri>) and other sources of
paleoenvironment and paleo-lithofacies data, to further constrain the
paleogeographic reconstructions.</p>
</sec>
</sec>
<sec id="Ch1.S6" sec-type="conclusions">
  <title>Conclusions</title>
      <p id="d1e1898">Our study highlights the flexibility of digital paleogeographic models
linked to plate tectonic reconstructions in order to better understand the
interplay of continental growth and eustasy, with wider implications for
understanding Earth's paleotopography, ocean circulation and the role of
mantle convection in shaping long-wavelength topography. We present a
workflow that enables the construction of paleogeographic maps with variable
spatial and temporal resolutions, while also becoming more testable and
expandable with the incorporation of new paleoenvironmental data sets.</p>
      <p id="d1e1901">We develop an approach to revise the paleo-coastline locations and
paleogeographic geometries using paleoenvironmental information indicated
by the marine fossil collections from the PBDB. Using this approach, the
consistency ratio between the paleogeography and the paleobiology records
since the Devonian is increased from an average 75 % to nearly full
consistency. The paleogeography in the main regions of North America, South
America, Europe and Africa is significantly improved, especially in the Late
Carboniferous, Middle Permian, Triassic, Jurassic, Late Cretaceous and most
portions of the Cenozoic. The flooded continental areas since the Late
Devonian inferred from the revised global paleogeography in this study are
generally consistent with the results derived from other paleoenvironment
and paleo-lithofacies data or from the strontium isotope record in marine
carbonates.</p>
      <p id="d1e1904">Comparing the terrestrial areal change over time associated with
transferring the reconstruction and filling gaps, and revising
paleogeographic geometries using the paleoenvironmental data from the PBDB,
indicates that reconstruction difference is a main factor in
paleogeographic areal change when comparing with the original maps, and revising
paleogeographic geometries based on PBDB test is secondary.</p>
</sec>
<sec id="Ch1.Sx1" specific-use="unnumbered">
  <title>Information about the supplement</title>
      <p id="d1e1913">We provide two sets of digital global paleogeographic maps during 402–2 Ma:
(1) the paleogeography reconstructed using the plate motion model of Matthews et
al. (2016) and revised using paleoenvironmental information indicated by
the marine fossil collections from the PBDB and (2) the original paleogeography
of Golonka et al. (2006). We also provide the original rotation file of Golonka et al. (2006), a set of paleogeographic maps illustrating the PBDB test and
revision of paleo-coastlines and paleogeographic geometries, a set of
GeoTiff files of all revised paleogeographic maps, paleobiology data in
shapefile used in this study separated into two sets of consistent marine
fossil collections and inconsistent marine fossil collections, an animation
for the revised global paleogeographic maps, and a README file outlined the
workflow of this study.</p>
</sec>

      
      </body>
    <back><app-group>
        <supplementary-material position="anchor"><p id="d1e1915"><bold>The Supplement related to this article is available online at <inline-supplementary-material xlink:href="https://doi.org/10.5194/bg-14-5425-2017-supplement" xlink:title="zip">https://doi.org/10.5194/bg-14-5425-2017-supplement</inline-supplementary-material>.</bold></p></supplementary-material>
        </app-group><notes notes-type="dataavailability">

      <p id="d1e1923">No data sets were used in this article.</p>
  </notes><notes notes-type="competinginterests">

      <p id="d1e1929">The authors declare that they have no conflict of
interest.</p>
  </notes><ack><title>Acknowledgements</title><p id="d1e1935">This work was supported by Australian Research Council grants
IH130200012 (RDM, SZ), DE160101020 (NF) and SIEF RP 04-174 (SW). W. Cao was also
supported by a University of Sydney International Scholarship (USydIS). We
thank Julia Sheehan and Logan Yeo for digitizing these paleogeographic maps,
and John Cannon and Michael Chin for help with GPlates and pyGPlates. We
sincerely thank Shanan Peters and three anonymous
reviewers for their constructive reviews and suggestions. We thank Natascha
Töpfer for editorial support and Tina Treude for editing the manuscript. We are also thankful for the entire PBDB team and all PBDB data contributors. This is
Paleobiology Database Publication 296.<?xmltex \hack{\newpage}?><?xmltex \hack{\noindent}?>Edited by: Tina Treude<?xmltex \hack{\newline}?>
Reviewed by: Shanan Peters and three anonymous referees</p></ack><ref-list>
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    <!--<article-title-html>Improving global paleogeography since the late Paleozoic using paleobiology</article-title-html>
<abstract-html><p class="p">Paleogeographic reconstructions are important to understand Earth's tectonic
evolution, past eustatic and regional sea level change, paleoclimate and
ocean circulation, deep Earth resources and to constrain and interpret the
dynamic topography predicted by mantle convection models. Global
paleogeographic maps have been compiled and published, but they are generally
presented as static maps with varying map projections, different time
intervals represented by the maps and different plate motion models that
underlie the paleogeographic reconstructions. This makes it difficult to
convert the maps into a digital form and link them to alternative digital
plate tectonic reconstructions. To address this limitation, we develop a
workflow to restore global paleogeographic maps to their present-day
coordinates and enable them to be linked to a different tectonic
reconstruction. We use marine fossil collections from the Paleobiology
Database to identify inconsistencies between their indicative
paleoenvironments and published paleogeographic maps, and revise the
locations of inferred paleo-coastlines that represent the estimated maximum
transgression surfaces by resolving these inconsistencies. As a result, the
consistency ratio between the paleogeography and the paleoenvironments
indicated by the marine fossil collections is increased from an average of
75 % to nearly full consistency (100 %). The paleogeography in the
main regions of North America, South America, Europe and Africa is
significantly revised, especially in the Late Carboniferous, Middle Permian,
Triassic, Jurassic, Late Cretaceous and most of the Cenozoic. The global
flooded continental areas since the Early Devonian calculated from the
revised paleogeography in this study are generally consistent with results
derived from other paleoenvironment and paleo-lithofacies data and with the
strontium isotope record in marine carbonates. We also estimate the
terrestrial areal change over time associated with transferring
reconstruction, filling gaps and modifying the paleogeographic geometries
based on the paleobiology test. This indicates that the variation of the
underlying plate reconstruction is the main factor that contributes to the
terrestrial areal change, and the effect of revising paleogeographic
geometries based on paleobiology is secondary.</p></abstract-html>
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