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  <front>
    <journal-meta><journal-id journal-id-type="publisher">ESSD</journal-id><journal-title-group>
    <journal-title>Earth System Science Data</journal-title>
    <abbrev-journal-title abbrev-type="publisher">ESSD</abbrev-journal-title><abbrev-journal-title abbrev-type="nlm-ta">Earth Syst. Sci. Data</abbrev-journal-title>
  </journal-title-group><issn pub-type="epub">1866-3516</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/essd-10-2123-2018</article-id><title-group><article-title>OCTOPUS: an open cosmogenic isotope and luminescence database</article-title><alt-title>An open cosmogenic isotope and luminescence database</alt-title>
      </title-group><?xmltex \runningtitle{An open cosmogenic isotope and luminescence database}?><?xmltex \runningauthor{A. T. Codilean et al.}?>
      <contrib-group>
        <contrib contrib-type="author" corresp="yes" rid="aff1 aff2">
          <name><surname>Codilean</surname><given-names>Alexandru T.</given-names></name>
          <email>codilean@uow.edu.au</email>
        <ext-link>https://orcid.org/0000-0003-1895-5633</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1 aff3">
          <name><surname>Munack</surname><given-names>Henry</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-3750-9674</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1 aff2">
          <name><surname>Cohen</surname><given-names>Timothy J.</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Saktura</surname><given-names>Wanchese M.</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-7198-7776</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff4">
          <name><surname>Gray</surname><given-names>Andrew</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff5">
          <name><surname>Mudd</surname><given-names>Simon M.</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-1357-8501</ext-link></contrib>
        <aff id="aff1"><label>1</label><institution>GeoQuEST Research Centre, School of Earth and Environmental Sciences,<?xmltex \hack{\break}?> University of Wollongong, Wollongong NSW 2522, Australia</institution>
        </aff>
        <aff id="aff2"><label>2</label><institution>ARC Centre of Excellence for Australian Biodiversity and Heritage,<?xmltex \hack{\break}?> University of Wollongong, Wollongong NSW 2522, Australia</institution>
        </aff>
        <aff id="aff3"><label>3</label><institution>Research Institute for Post-Mining Landscapes (FIB), Finsterwalde 03238, Germany</institution>
        </aff>
        <aff id="aff4"><label>4</label><institution>Information Technology Services, University of Wollongong, Wollongong NSW 2522, Australia</institution>
        </aff>
        <aff id="aff5"><label>5</label><institution>School of GeoSciences, University of Edinburgh, Edinburgh EH8 9XP, UK</institution>
        </aff>
      </contrib-group>
      <author-notes><corresp id="corr1">Alexandru T. Codilean (codilean@uow.edu.au)</corresp></author-notes><pub-date><day>30</day><month>November</month><year>2018</year></pub-date>
      
      <volume>10</volume>
      <issue>4</issue>
      <fpage>2123</fpage><lpage>2139</lpage>
      <history>
        <date date-type="received"><day>5</day><month>March</month><year>2018</year></date>
           <date date-type="rev-request"><day>6</day><month>March</month><year>2018</year></date>
           <date date-type="rev-recd"><day>19</day><month>November</month><year>2018</year></date>
           <date date-type="accepted"><day>20</day><month>November</month><year>2018</year></date>
      </history>
      <permissions>
        
        
      <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://essd.copernicus.org/articles/10/2123/2018/essd-10-2123-2018.html">This article is available from https://essd.copernicus.org/articles/10/2123/2018/essd-10-2123-2018.html</self-uri><self-uri xlink:href="https://essd.copernicus.org/articles/10/2123/2018/essd-10-2123-2018.pdf">The full text article is available as a PDF file from https://essd.copernicus.org/articles/10/2123/2018/essd-10-2123-2018.pdf</self-uri>
      <abstract>
    <p id="d1e157">We present a database of cosmogenic radionuclide and luminescence measurements
in fluvial sediment. With support from the Australian National Data Service
(ANDS) we have built infrastructure for hosting and maintaining the data at
the University of Wollongong and making this available to the research
community via an Open Geospatial Consortium (OGC)-compliant web service. The
cosmogenic radionuclide (CRN) part of the database consists of <inline-formula><mml:math id="M1" display="inline"><mml:mrow class="chem"><mml:msup><mml:mi/><mml:mn mathvariant="normal">10</mml:mn></mml:msup><mml:mi mathvariant="normal">Be</mml:mi></mml:mrow></mml:math></inline-formula>
and <inline-formula><mml:math id="M2" display="inline"><mml:mrow class="chem"><mml:msup><mml:mi/><mml:mn mathvariant="normal">26</mml:mn></mml:msup><mml:mi mathvariant="normal">Al</mml:mi></mml:mrow></mml:math></inline-formula> measurements in modern fluvial sediment samples from
across the globe, along with ancillary geospatial vector and raster layers,
including sample site, basin outline, digital elevation model, gradient
raster, flow-direction and flow-accumulation rasters, atmospheric pressure
raster, and CRN production scaling and topographic shielding factor rasters.
Sample metadata are comprehensive and include all necessary information for
the recalculation of denudation rates using CAIRN, an open-source
program for calculating
basin-wide denudation rates from <inline-formula><mml:math id="M3" display="inline"><mml:mrow class="chem"><mml:msup><mml:mi/><mml:mn mathvariant="normal">10</mml:mn></mml:msup><mml:mi mathvariant="normal">Be</mml:mi></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M4" display="inline"><mml:mrow class="chem"><mml:msup><mml:mi/><mml:mn mathvariant="normal">26</mml:mn></mml:msup><mml:mi mathvariant="normal">Al</mml:mi></mml:mrow></mml:math></inline-formula> data.
Further all data have been recalculated and harmonised using the same
program. The luminescence part of the database consists of
thermoluminescence (TL) and optically stimulated luminescence (OSL)
measurements in fluvial sediment samples from stratigraphic sections and
sediment cores from across the Australian continent and includes ancillary
vector and raster geospatial data. The database can be interrogated and
downloaded via a custom-built web map service. More advanced interrogation
and exporting to various data formats, including the ESRI Shapefile and
Google Earth's KML, is also possible via the Web Feature Service (WFS)
capability running on the OCTOPUS server. Use of open standards also ensures
that data layers are visible to other OGC-compliant data-sharing services.
OCTOPUS and its associated data curation framework provide the opportunity
for researchers to reuse previously published but otherwise unusable CRN and
luminescence data. This delivers the potential to harness old but valuable
data that would otherwise be lost to the research community. OCTOPUS can be
accessed at <uri>https://earth.uow.edu.au</uri> (last access: 28 November 2018).
The individual data collections can also be accessed via the following DOIs:
<ext-link xlink:href="https://doi.org/10.4225/48/5a8367feac9b2" ext-link-type="DOI">10.4225/48/5a8367feac9b2</ext-link> (CRN International),
<ext-link xlink:href="https://doi.org/10.4225/48/5a836cdfac9b5" ext-link-type="DOI">10.4225/48/5a836cdfac9b5</ext-link> (CRN Australia), and
<ext-link xlink:href="https://doi.org/10.4225/48/5a836db1ac9b6" ext-link-type="DOI">10.4225/48/5a836db1ac9b6</ext-link> (OSL &amp; TL Australia).</p>
  </abstract>
    </article-meta>
  </front>
<body>
      

<?pagebreak page2124?><sec id="Ch1.S1" sec-type="intro">
  <title>Introduction</title>
      <p id="d1e228">Cosmogenic radionuclide (CRN) exposure dating and luminescence dating are
suites of geochronological techniques that have become important for the
studying of Earth surface processes
<xref ref-type="bibr" rid="bib1.bibx64 bib1.bibx39" id="paren.1"><named-content content-type="pre">e.g.</named-content></xref>. Both permit quantifying the
timing of geological events by dating individual landforms. In addition, CRNs
can also be used to measure the rate at which landforms or landscapes are
being denuded by physical and chemical erosion processes. Thus, the two
suites of techniques have been extensively used among others to quantify
basin-wide denudation rates
<xref ref-type="bibr" rid="bib1.bibx75 bib1.bibx37" id="paren.2"/>, to reconstruct the extent
of Quaternary glaciations
<xref ref-type="bibr" rid="bib1.bibx71 bib1.bibx6 bib1.bibx46" id="paren.3"/>, to study how
rivers have adapted to past climate change via incision and aggradation
<xref ref-type="bibr" rid="bib1.bibx69 bib1.bibx51 bib1.bibx77" id="paren.4"/>, and to study
the timing of dune construction
<xref ref-type="bibr" rid="bib1.bibx30 bib1.bibx33 bib1.bibx13" id="paren.5"/>. Both
suites of techniques are costly (both in terms of time and money) and require
specialised training, laboratories, and equipment. As such, CRN and
luminescence studies are often very focused and involve a relatively small
number of samples (<inline-formula><mml:math id="M5" display="inline"><mml:mrow><mml:mi>n</mml:mi><mml:mo>&lt;</mml:mo><mml:mn mathvariant="normal">100</mml:mn></mml:mrow></mml:math></inline-formula>). The research questions being addressed by these
studies are very specific and study areas are often relatively small. Hence,
CRN and luminescence studies will produce small data sets that are unmanaged
and that may become <italic>forgotten</italic> once
the study has been completed and results are published. Further, despite
there being calls for minimum data reporting standards
<xref ref-type="bibr" rid="bib1.bibx27 bib1.bibx31" id="paren.6"><named-content content-type="pre">e.g.</named-content></xref>, the published work will
often not include appropriate levels of metadata to make the raw data
reusable with ease. The latter is especially important in the case of
cosmogenic nuclides as procedures used to interpret CRN data are regularly
revised and updated, requiring denudation rates and/or exposure ages to be
recalculated using updated measurement standards and calculation protocols.
Such recalculations are also necessary when comparing results produced by
different accelerator mass spectrometry (AMS) facilities that happen to
normalise results to different AMS standards. Therefore, without periodic
recalculation and maintenance of the data, CRN-based age and rate estimates,
for example, can become out of date after a few years. A system and framework
for managing CRN and luminescence data and metadata are critical to ensuring
the longevity and value of such data collections.</p>
      <p id="d1e269">Here we present a database of cosmogenic radionuclide and luminescence
measurements in fluvial sediment – OCTOPUS. With support from the Australian
National Data Service (ANDS) we have built infrastructure for hosting and
maintaining the data at the University of Wollongong and making this
available to the research community via an Open Geospatial Consortium
(OGC)-compliant web service (<uri>http://www.opengeospatial.org</uri>, last
access: 28 November 2018). The CRN part of the database consists of
<inline-formula><mml:math id="M6" display="inline"><mml:mrow class="chem"><mml:msup><mml:mi/><mml:mn mathvariant="normal">10</mml:mn></mml:msup><mml:mi mathvariant="normal">Be</mml:mi></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M7" display="inline"><mml:mrow class="chem"><mml:msup><mml:mi/><mml:mn mathvariant="normal">26</mml:mn></mml:msup><mml:mi mathvariant="normal">Al</mml:mi></mml:mrow></mml:math></inline-formula> measurements in fluvial sediment samples
from across the globe. Sample metadata are comprehensive and include all
necessary information for the recalculation of denudation rates using CAIRN,
an open-source program for calculating basin-wide denudation rates from
<inline-formula><mml:math id="M8" display="inline"><mml:mrow class="chem"><mml:msup><mml:mi/><mml:mn mathvariant="normal">10</mml:mn></mml:msup><mml:mi mathvariant="normal">Be</mml:mi></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M9" display="inline"><mml:mrow class="chem"><mml:msup><mml:mi/><mml:mn mathvariant="normal">26</mml:mn></mml:msup><mml:mi mathvariant="normal">Al</mml:mi></mml:mrow></mml:math></inline-formula> data <xref ref-type="bibr" rid="bib1.bibx56" id="paren.7"/>. To this end,
the database also includes a comprehensive suite of geospatial data layers,
both vector (e.g. sample site and basin outline) and raster (e.g. elevation,
gradient and flow-routing rasters, atmospheric pressure, and CRN production
scaling and topographic shielding factors). The luminescence part of the
database consists of thermoluminescence (TL) and optically stimulated
luminescence (OSL) measurements in fluvial sediment samples from
stratigraphic sections and sediment cores from across the Australian
continent. Comprehensive metadata and ancillary vector and raster geospatial
data are likewise included and available for download. OCTOPUS can be
accessed at <uri>https://earth.uow.edu.au</uri> (last access: 28 November 2018).</p>
</sec>
<sec id="Ch1.S2">
  <title>CRN and luminescence dating in a nutshell</title>
      <p id="d1e336">This section briefly describes the two suites of dating techniques and
provides information on CAIRN.</p>
<sec id="Ch1.S2.SS1">
  <?xmltex \opttitle{Inferring denudation rates from cosmogenic\hack{\break} {$\protect\chem{{}^{{10}}Be}$} (and {$\protect\chem{{}^{{26}}Al}$})}?><title>Inferring denudation rates from cosmogenic<?xmltex \hack{\break}?> <inline-formula><mml:math id="M10" display="inline"><mml:mrow class="chem"><mml:msup><mml:mi/><mml:mn mathvariant="normal">10</mml:mn></mml:msup><mml:mi mathvariant="normal">Be</mml:mi></mml:mrow></mml:math></inline-formula> (and <inline-formula><mml:math id="M11" display="inline"><mml:mrow class="chem"><mml:msup><mml:mi/><mml:mn mathvariant="normal">26</mml:mn></mml:msup><mml:mi mathvariant="normal">Al</mml:mi></mml:mrow></mml:math></inline-formula>)</title>
      <p id="d1e371">Cosmogenic nuclide exposure dating is based on the study of rare isotopes
produced by high-energy cosmic radiation breaking up the atoms that make up
the minerals and rocks at the Earth's surface. The term “in situ” is used to
distinguish these isotopes from those that are produced through the same
cosmic-ray-induced nuclear reactions in the atmosphere – termed
“meteoric” <xref ref-type="bibr" rid="bib1.bibx26 bib1.bibx39" id="paren.8"/>. Several of the in
situ cosmogenic nuclides, including the stable <inline-formula><mml:math id="M12" display="inline"><mml:mrow class="chem"><mml:msup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msup><mml:mi mathvariant="normal">He</mml:mi></mml:mrow></mml:math></inline-formula> and
<inline-formula><mml:math id="M13" display="inline"><mml:mrow class="chem"><mml:msup><mml:mi/><mml:mn mathvariant="normal">21</mml:mn></mml:msup><mml:mi mathvariant="normal">Ne</mml:mi></mml:mrow></mml:math></inline-formula>, and the radioactive <inline-formula><mml:math id="M14" display="inline"><mml:mrow class="chem"><mml:msup><mml:mi/><mml:mn mathvariant="normal">10</mml:mn></mml:msup><mml:mi mathvariant="normal">Be</mml:mi></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M15" display="inline"><mml:mrow class="chem"><mml:msup><mml:mi/><mml:mn mathvariant="normal">26</mml:mn></mml:msup><mml:mi mathvariant="normal">Al</mml:mi></mml:mrow></mml:math></inline-formula>, and
<inline-formula><mml:math id="M16" display="inline"><mml:mrow class="chem"><mml:msup><mml:mi/><mml:mn mathvariant="normal">36</mml:mn></mml:msup><mml:mi mathvariant="normal">Cl</mml:mi></mml:mrow></mml:math></inline-formula>, are now routinely measured and have been used in
geomorphological studies for the last three decades
<xref ref-type="bibr" rid="bib1.bibx8 bib1.bibx75 bib1.bibx26 bib1.bibx37" id="paren.9"/>.
Of these nuclides, however, <inline-formula><mml:math id="M17" display="inline"><mml:mrow class="chem"><mml:msup><mml:mi/><mml:mn mathvariant="normal">10</mml:mn></mml:msup><mml:mi mathvariant="normal">Be</mml:mi></mml:mrow></mml:math></inline-formula> produced in quartz is the
workhorse for in situ applications, and most in situ cosmogenic nuclide
studies have used <inline-formula><mml:math id="M18" display="inline"><mml:mrow class="chem"><mml:msup><mml:mi/><mml:mn mathvariant="normal">10</mml:mn></mml:msup><mml:mi mathvariant="normal">Be</mml:mi></mml:mrow></mml:math></inline-formula> either alone or in conjunction with other
cosmogenic nuclides such as <inline-formula><mml:math id="M19" display="inline"><mml:mrow class="chem"><mml:msup><mml:mi/><mml:mn mathvariant="normal">26</mml:mn></mml:msup><mml:mi mathvariant="normal">Al</mml:mi></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M20" display="inline"><mml:mrow class="chem"><mml:msup><mml:mi/><mml:mn mathvariant="normal">21</mml:mn></mml:msup><mml:mi mathvariant="normal">Ne</mml:mi></mml:mrow></mml:math></inline-formula>. Given the long
half-life of <inline-formula><mml:math id="M21" display="inline"><mml:mrow class="chem"><mml:msup><mml:mi/><mml:mn mathvariant="normal">10</mml:mn></mml:msup><mml:mi mathvariant="normal">Be</mml:mi></mml:mrow></mml:math></inline-formula>
<xref ref-type="bibr" rid="bib1.bibx17 bib1.bibx49" id="paren.10"><named-content content-type="pre"><inline-formula><mml:math id="M22" display="inline"><mml:mrow><mml:msub><mml:mi>T</mml:mi><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:mo>/</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msub><mml:mo>=</mml:mo><mml:mn mathvariant="normal">1.387</mml:mn></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M23" display="inline"><mml:mi mathvariant="normal">Myr</mml:mi></mml:math></inline-formula>,</named-content></xref>
and the increasingly low analytical backgrounds that can be realised, it is
now possible to analyse samples covering a wide range of temporal settings,
including historic times <xref ref-type="bibr" rid="bib1.bibx68" id="paren.11"><named-content content-type="pre">e.g.</named-content></xref>. The rate at
which cosmogenic nuclides are produced is extremely low – a few atoms per
gram of rock per year <xref ref-type="bibr" rid="bib1.bibx10" id="paren.12"/> and the rapid attenuation of
cosmic radiation with depth confines the production of cosmogenic nuclides to
the upper few metres of the crust, production rates decreasing roughly
exponentially with depth <xref ref-type="bibr" rid="bib1.bibx3 bib1.bibx4" id="paren.13"/>.
Production rates<?pagebreak page2125?> of cosmogenic nuclides are mainly a function of geomagnetic
latitude and altitude above sea level
<xref ref-type="bibr" rid="bib1.bibx7 bib1.bibx52" id="paren.14"/>. Site-specific cosmogenic nuclide
production rates are also subject to several other factors, the most
important of these being the geometry of the surrounding topography, which
shields part of the incoming cosmic radiation
<xref ref-type="bibr" rid="bib1.bibx28 bib1.bibx18 bib1.bibx25" id="paren.15"/>.</p>
      <p id="d1e551">The application of <inline-formula><mml:math id="M24" display="inline"><mml:mrow class="chem"><mml:msup><mml:mi/><mml:mn mathvariant="normal">10</mml:mn></mml:msup><mml:mi mathvariant="normal">Be</mml:mi></mml:mrow></mml:math></inline-formula> (or any other in situ-produced cosmogenic
nuclide) to the study of Earth surface processes is based on the principle
that its concentration is directly proportional to the exposure time to
cosmic radiation. Cosmogenic nuclides will accumulate in surficial deposits
over time such that their concentration will be directly related to not only
the exposure age but also the rate at which the surface is eroding
<xref ref-type="bibr" rid="bib1.bibx50 bib1.bibx39 bib1.bibx76" id="paren.16"/>. As a
parcel of rock or sediment is brought toward the surface by erosion on a
hillslope, its <inline-formula><mml:math id="M25" display="inline"><mml:mrow class="chem"><mml:msup><mml:mi/><mml:mn mathvariant="normal">10</mml:mn></mml:msup><mml:mi mathvariant="normal">Be</mml:mi></mml:mrow></mml:math></inline-formula> concentration increases at a rate that depends
mainly on the rate of erosion, and the <inline-formula><mml:math id="M26" display="inline"><mml:mrow class="chem"><mml:msup><mml:mi/><mml:mn mathvariant="normal">10</mml:mn></mml:msup><mml:mi mathvariant="normal">Be</mml:mi></mml:mrow></mml:math></inline-formula> surface production rate
at that locality. When the parcel of rock or sediment reaches the surface, it
is transported via hillslope processes to the fluvial system, where it mixes
with sediment from other parts of the contributing catchment. Thus, rivers
act not only as agents of erosion but also as integrators, collecting
sediment from all parts of the catchment in an amount that is proportional to
their denudation rate such that, at the outlet of the catchment, the sediment
will contain an average concentration of <inline-formula><mml:math id="M27" display="inline"><mml:mrow class="chem"><mml:msup><mml:mi/><mml:mn mathvariant="normal">10</mml:mn></mml:msup><mml:mi mathvariant="normal">Be</mml:mi></mml:mrow></mml:math></inline-formula> (and <inline-formula><mml:math id="M28" display="inline"><mml:mrow class="chem"><mml:msup><mml:mi/><mml:mn mathvariant="normal">26</mml:mn></mml:msup><mml:mi mathvariant="normal">Al</mml:mi></mml:mrow></mml:math></inline-formula>)
that is a measure of the catchment's mean denudation rate
<xref ref-type="bibr" rid="bib1.bibx75 bib1.bibx37" id="paren.17"/>. The technique of
determining basin-wide denudation rates from CRN concentrations in stream
sediments was first introduced in the mid-1990s
<xref ref-type="bibr" rid="bib1.bibx14 bib1.bibx9 bib1.bibx38" id="paren.18"><named-content content-type="pre">e.g.</named-content></xref>, and
since that time denudation rates have been determined in over 4000 river
basins from a wide range of tectonic and climatic settings.</p>
</sec>
<sec id="Ch1.S2.SS2">
  <title>Luminescence dating of sediment</title>
      <p id="d1e632">Luminescence dating provides an estimate of the amount of time elapsed since
mineral grains (quartz or feldspar) were last exposed to intense heat or
sunlight. The suite of techniques includes thermoluminescence dating (TL), in
which the luminescence signal is produced by heating mineral grains in the
laboratory during measurement <xref ref-type="bibr" rid="bib1.bibx1 bib1.bibx44" id="paren.19"/>, and
optically stimulated luminescence dating (OSL), in which the luminescence
signal is produced by exposing the mineral grains to an intense light source
<xref ref-type="bibr" rid="bib1.bibx2" id="paren.20"/>. The suite of techniques can be used to date events as
young as a few decades
<xref ref-type="bibr" rid="bib1.bibx83 bib1.bibx66 bib1.bibx59 bib1.bibx24" id="paren.21"><named-content content-type="pre">e.g.</named-content></xref>
to those as old as nearly 1 <inline-formula><mml:math id="M29" display="inline"><mml:mi mathvariant="normal">Ma</mml:mi></mml:math></inline-formula> <xref ref-type="bibr" rid="bib1.bibx5" id="paren.22"/>. The basis of both
TL and OSL dating resides in measurements of the trapped charge (e.g.
electrons) within mineral lattice imperfections which accumulate over time.
When electrons are exposed to ionising radiation produced by the decay of
radioisotopes contained in the surrounding sediment matrix, and/or via
exposure to high-energy cosmic rays, electrons will move from a lower energy
level (valence band) to a higher energy level (conduction band). Moving
between the two bands, some of the energised electrons will become trapped by
defects in the crystal lattice. In a parcel of sediment that is buried and
thus shielded from sunlight and/or intense heat, the number of trapped
electrons will increase steadily with time in proportion to the intensity of
the ionising radiation flux (i.e. dose rate) and water saturation of the
sediment. When the irradiated mineral grains are exposed to sunlight (or
intense heat) the electrons will escape the traps, and the luminescence
clock is zeroed. Thus, TL and OSL provide ages that represent the last time
the electron traps were emptied or bleached – either by exposure of
the sediment to sunlight (e.g. during sediment transport) or by heating
(e.g. during a bush fire or in aboriginal hearths)
<xref ref-type="bibr" rid="bib1.bibx80 bib1.bibx64" id="paren.23"/>.</p>
      <p id="d1e660">When luminescence dating techniques are applied to sediments, an often used
assumption (when analysing multiple grains) is that the electron traps were
completely emptied prior to deposition and so the luminescence clock has been
effectively zeroed. In the case of OSL even short exposure to sunlight
(<inline-formula><mml:math id="M30" display="inline"><mml:mrow><mml:mo>&lt;</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:math></inline-formula> min) is sufficient to bleach the sediment grains and thus zero the
luminescence clock; however for TL, a longer exposure to sunlight is required
to remove the TL signal. Fine mineral grains (<inline-formula><mml:math id="M31" display="inline"><mml:mrow><mml:mo>&lt;</mml:mo><mml:mn mathvariant="normal">63</mml:mn></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M32" display="inline"><mml:mi mathvariant="normal">µ</mml:mi></mml:math></inline-formula>m) that are
transported by wind or as suspended fluvial sediment should be exposed to
sunlight while airborne or in the upper parts of the water column. On the
other hand, larger grains that travelled as bedload might only be partially
bleached. Independent of grain size, when dealing with fluvial sediment, the
bleaching characteristics of the sample need to be assessed in order to
determine the use of an applicable age model. Possible strategies for
determining bleaching characteristics include using geomorphic models that
reconstruct mineral grain pathways and thus predict optimal bleaching regimes
<xref ref-type="bibr" rid="bib1.bibx32" id="paren.24"><named-content content-type="pre">e.g.</named-content></xref>, analysing recently deposited sediment to
assess their residual OSL–TL signals
<xref ref-type="bibr" rid="bib1.bibx63 bib1.bibx70" id="paren.25"><named-content content-type="pre">e.g.</named-content></xref>, pairing with a
second independent dating technique such as radiocarbon dating
<xref ref-type="bibr" rid="bib1.bibx58" id="paren.26"><named-content content-type="pre">e.g.</named-content></xref>, and analysing different grain size fractions
or closely spaced samples with different depositional energies under the
assumption that these might have behaved differently during sediment
transport <xref ref-type="bibr" rid="bib1.bibx65" id="paren.27"><named-content content-type="pre">e.g.</named-content></xref>. Alternatively, various age
models can be applied to either single or multi-grain data sets <xref ref-type="bibr" rid="bib1.bibx34" id="paren.28"><named-content content-type="pre">e.g.
minimum age model;</named-content></xref>, which statistically differentiate
partially bleached grain populations so as to derive the equivalent dose and
subsequent age of the depositional event.</p>
</sec>
<?pagebreak page2126?><sec id="Ch1.S2.SS3">
  <title>The CAIRN method for calculating CRN-based basin-wide denudation rates</title>
      <p id="d1e722">CAIRN is an automated, open-source method for calculating basin-averaged
denudation rates so that inferred denudation rates are reproducible: the
method ingests topographic data, cosmogenic <inline-formula><mml:math id="M33" display="inline"><mml:mrow class="chem"><mml:msup><mml:mi/><mml:mn mathvariant="normal">10</mml:mn></mml:msup><mml:mi mathvariant="normal">Be</mml:mi></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M34" display="inline"><mml:mrow class="chem"><mml:msup><mml:mi/><mml:mn mathvariant="normal">26</mml:mn></mml:msup><mml:mi mathvariant="normal">Al</mml:mi></mml:mrow></mml:math></inline-formula>
concentrations and a parameter file and any two users with the same inputs
will calculate the same denudation rate <xref ref-type="bibr" rid="bib1.bibx56" id="paren.29"/>. CAIRN forward
models <inline-formula><mml:math id="M35" display="inline"><mml:mrow class="chem"><mml:msup><mml:mi/><mml:mn mathvariant="normal">10</mml:mn></mml:msup><mml:mi mathvariant="normal">Be</mml:mi></mml:mrow></mml:math></inline-formula> or <inline-formula><mml:math id="M36" display="inline"><mml:mrow class="chem"><mml:msup><mml:mi/><mml:mn mathvariant="normal">26</mml:mn></mml:msup><mml:mi mathvariant="normal">Al</mml:mi></mml:mrow></mml:math></inline-formula> concentrations at every pixel for a
given denudation rate, taking into account latitude and altitude scaling of
CRN production rates as well as snow, self, and topographic shielding. The
obtained concentrations are averaged to predict a basin-averaged
<inline-formula><mml:math id="M37" display="inline"><mml:mrow class="chem"><mml:msup><mml:mi/><mml:mn mathvariant="normal">10</mml:mn></mml:msup><mml:mi mathvariant="normal">Be</mml:mi></mml:mrow></mml:math></inline-formula> or <inline-formula><mml:math id="M38" display="inline"><mml:mrow class="chem"><mml:msup><mml:mi/><mml:mn mathvariant="normal">26</mml:mn></mml:msup><mml:mi mathvariant="normal">Al</mml:mi></mml:mrow></mml:math></inline-formula> concentration, and Newton's method is then
used to find the denudation rate for which the predicted concentration
matches the measured concentration and to derive associated uncertainties.
CAIRN is also capable of ingesting fixed denudation rates in masked portions
of the input raster, allowing users to calculate spatially varying denudation
rates in nested basins. In addition, CAIRN outputs spatially averaged CRN
production scaling and topographic shielding values that can be used with
other available CRN calculators that do not provide spatial averaging,
including the online calculators formerly known as the CRONUS-Earth online
calculators <xref ref-type="bibr" rid="bib1.bibx7" id="paren.30"/> and the Microsoft Excel-based COSMOCALC
<xref ref-type="bibr" rid="bib1.bibx73" id="paren.31"/>. Because there is no graphical interface and because
releases of the software are tagged, CAIRN users can simply publish digital
elevation model (DEM) metadata, CRN data files, and CAIRN input files, and
denudation rates should be reproducible. The open-source framework means that
the code can be modified to include updated methods for production rates and
scaling factors. Future users can thus recalculate denudation rates using
updated versions of the code. CAIRN includes scripts for producing separate
basin rasters for each cosmogenic sample from a regional topographic raster
so that the denudation rate calculations can be run on multiple processors,
meaning that large regional data sets can be processed simultaneously on
compute clusters.</p>
</sec>
</sec>
<sec id="Ch1.S3">
  <title>Accessing data from OCTOPUS</title>
      <p id="d1e814">This section provides a description of the software infrastructure behind
OCTOPUS. It also describes the ways in which data can be accessed,
interrogated, and downloaded. The software infrastructure behind OCTOPUS
consists of a combination of off-the-shelf open-source packages, bespoke code
for handling the upload and download of data, and a web interface.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F1"><caption><p id="d1e819">The setup of
the OCTOPUS data-storage and -sharing platform. See text for more details.</p></caption>
        <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://essd.copernicus.org/articles/10/2123/2018/essd-10-2123-2018-f01.png"/>

      </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F2" specific-use="star"><caption><p id="d1e830">The OCTOPUS web interface with main elements: (1) message box that
provides the user with step-by-step help on how to navigate the web page,
(2) collapsible panel with a list of all available data layers,
(3) navigation buttons, (4) data download button, (5) Google Terrain base map
and point and polygon data layers. See text for more details.</p></caption>
        <?xmltex \igopts{width=497.923228pt}?><graphic xlink:href="https://essd.copernicus.org/articles/10/2123/2018/essd-10-2123-2018-f02.png"/>

      </fig>

<sec id="Ch1.S3.SS1">
  <title>System architecture</title>
      <p id="d1e845">The software architecture behind OCTOPUS is illustrated in
Fig. <xref ref-type="fig" rid="Ch1.F1"/>. The data are stored in two separate
locations. First, tabular data and the point and polygon geometries
associated with each sample site or study (see Sect. 4) are stored in a
PostGIS database. PostGIS (<uri>https://postgis.net</uri>, last access:
28 November 2018) is a spatial database extender for the PostgreSQL
object-relational database management system
(<uri>https://www.postgresql.org</uri>, last access: 28 November 2018), adding
support for geographic objects and allowing location-based queries to be run
in SQL. Second, all data (tabular, vector, and raster) and auxiliary
information (e.g. CAIRN input and output files) (see Sect. 4) are also stored
in separate zip archives, with one zip file for each study. This hybrid
setup was chosen over having all tabular, vector, and raster data together
in the PostGIS database because (i) it offered more flexibility regarding the
list of files and file formats that could be included for download, and
(ii) it made the coding of data upload and download simpler. The PostGIS
database is connected to a GeoServer instance
(Fig. <xref ref-type="fig" rid="Ch1.F1"/>). GeoServer is an open-source server that
allows the sharing, processing, and editing of geospatial data
(<uri>http://geoserver.org</uri>, last access: 28 November 2018), and implements a
range of OCG data-sharing standards, including the widely used Web Feature
Service (WFS) and the Web Map Service (WMS) standards. GeoServer also
produces a variety of commonly used geospatial data formats via WFS,
including KML and the ESRI Shapefile,
and so can export data for using with popular desktop GIS applications such
as Google Earth, ArcGIS, and QGIS (Fig. <xref ref-type="fig" rid="Ch1.F1"/>). It is
also possible to connect to the GeoServer instance directly in QGIS<?pagebreak page2127?> and
interrogate the data via the WFS protocol (see below). The OpenLayers
(<uri>https://openlayers.org</uri>, last access: 28 November 2018) JavaScript
library is used to display the geospatial data served by the GeoServer
instance in a web browser (Fig. <xref ref-type="fig" rid="Ch1.F1"/>). OpenLayers also
allows for the data to be queried and a selection to be made for download.</p>
</sec>
<sec id="Ch1.S3.SS2">
  <title>Accessing data using the web interface</title>
      <p id="d1e875">The web interface has a simple design and its sole purpose is to enable
users to visualise the various data collections and to select data for
download. The web interface includes the following elements
(Fig. <xref ref-type="fig" rid="Ch1.F2"/>): a message box that provides the user with
step-by-step help on how to navigate the web page (Fig. <xref ref-type="fig" rid="Ch1.F2"/>,
#1); a collapsible panel with a list of all available data layers – these
are grouped by data collection (see Sect. 4) and can be toggled on or off
(Fig. <xref ref-type="fig" rid="Ch1.F2"/>, #2); navigation buttons allowing zooming and
scrolling (Fig. <xref ref-type="fig" rid="Ch1.F2"/>, #3); and the data download button
(Fig. <xref ref-type="fig" rid="Ch1.F2"/>, #4). The latter opens a dialogue panel and switches
the cursor from panning mode to selection mode, allowing for data layers to
be selected and added to a download list. The OpenLayers map frame uses
Google Terrain as the base layer and the point and polygon data are displayed
using different colours for each collection (Fig. <xref ref-type="fig" rid="Ch1.F2"/>, #5).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F3" specific-use="star"><caption><p id="d1e893">Screenshots of the OCTOPUS web page illustrating a typical user
session. See text for more details.</p></caption>
          <?xmltex \igopts{width=455.244094pt}?><graphic xlink:href="https://essd.copernicus.org/articles/10/2123/2018/essd-10-2123-2018-f03.png"/>

        </fig>

      <p id="d1e902"><?xmltex \hack{\newpage}?>Figure <xref ref-type="fig" rid="Ch1.F3"/> illustrates a typical user interaction with the web
interface. First, the user displays the data collection(s) of interest and
navigates to the desired geographical area. This can be achieved by using the
navigation buttons or simply by clicking (to zoom) and dragging (to pan) on
the map area. To query the data, the user clicks on a point or polygon
feature. This action displays an information panel that includes a subset of
the records available as part of the attribute table for each point or
polygon feature. In the case of overlapping features, the information panel
displays records for all features (Fig. <xref ref-type="fig" rid="Ch1.F3"/>, #1). Displayed
information includes sample ID, publication details, and recalculated
<inline-formula><mml:math id="M39" display="inline"><mml:mrow class="chem"><mml:msup><mml:mi/><mml:mn mathvariant="normal">10</mml:mn></mml:msup><mml:mi mathvariant="normal">Be</mml:mi></mml:mrow></mml:math></inline-formula>-based denudation rate with uncertainty for CRN data, or
published age with uncertainty for OSL–TL data. The dialogue
panel closes automatically once the user clicks anywhere outside of the panel
in the map display window. The displayed data are only a subset of the
available attribute data and are meant to provide the user with basic
information about each point or polygon record. To download data, the user
clicks on the download button. This action turns the cursor into a selection
tool (the user drags a box around desired points and polygons to select) and
displays a dialogue panel requesting user information such as name, email
address, and the intended use of the data (Fig. <xref ref-type="fig" rid="Ch1.F3"/>, #2–3).
The user has the option to fine-tune the list of selected studies by toggling
on or off each study from the list generated after the selection box <?pagebreak page2128?>is
drawn. It is possible to select multiple studies from multiple collections at
the same time. A valid email address is required as links to the data are
sent to the user via email immediately after the download button is
pressed. There is no verification of who the data requestor is or where that
person is from; however, none of the fields can be left empty and all entered
information is stored in a log file permanently and is used for reporting
purposes. Thus, although not mandatory, providing some meaningful information
when downloading the data via the web interface will support future efforts
to secure funding for OCTOPUS.</p>
</sec>
<?pagebreak page2129?><sec id="Ch1.S3.SS3">
  <title>Accessing data using the Web Feature Service (WFS) capability</title>
      <p id="d1e930">The web interface allows users to download all of the data: tabular, vector,
and raster. The data are organised in studies – each publication is a
“study” – with files belonging to
each study stored in separated zip archives (see below). The size of these
zip archives ranges from as small as 1 MB to just over 2.5 GB, and so the
web interface is meant for downloading a small number of studies per session
rather than the entire collection – the size of which at the time of writing
was just over 165 GB. Users who want access to a subset or to the entire
collection but who do not need access to the raster data, however, can
download the tabular and vector data using the WFS capability running on the
GeoServer instance, instead. WFS allows geospatial data to be interrogated
and requested for download using a URL via a web browser or displayed
directly in desktop applications such as QGIS (see below). It is beyond the
scope of this paper to provide a manual on WFS. Rather, here we provide a
series of examples that users can modify to perform basic queries and
download data. For a more comprehensive introduction to WFS and GeoServer,
the reader is referred to <xref ref-type="bibr" rid="bib1.bibx45" id="text.32"/> or to the
GeoServer documentation web page at <uri>http://docs.geoserver.org</uri> (last
access: 28 November 2018).</p>
      <p id="d1e939">The following example WFS request will download all drainage basins belonging
to the CRN International collection in the ESRI Shapefile format:
<preformat><![CDATA[http://earth.uow.edu.au:80/geoserver/
       wfs?request=GetFeature&typename
       =be10-denude:crn_int_basins&
       outputformat=SHAPE-ZIP]]></preformat>
<?xmltex \hack{\noindent}?>In the above example, <monospace>be10-denude:crn_int_ basins</monospace>
is the name of the data layer to be downloaded and <preformat preformat-type="code"><![CDATA[SHAPE-ZIP]]></preformat> refers to
the format used to export the data (here, ESRI Shapefile). To obtain a full list of available data layers and
export data formats, one should use the following request:
<preformat><![CDATA[http://earth.uow.edu.au:80/geoserver/
       wfs?request=GetCapabilities]]></preformat>
<?xmltex \hack{\noindent}?>and look under <preformat preformat-type="code"><![CDATA[FeatureTypeList]]></preformat> and
<preformat preformat-type="code"><![CDATA[ows:OperationsMetadata]]></preformat> in the results displayed for layer names and
data formats, respectively. It is possible to request only a subset of the
data by using the CQL/ECQL query language. For example, the following WFS
request will download all drainage basins (with CRN data in the attribute
table) from the CRN Australia collection in the ESRI
Shapefile format that were published
between 2005 and 2010:
<preformat><![CDATA[http://earth.uow.edu.au:80/geoserver/
       wfs?request=GetFeature&typename
       =be10-denude:crn_aus_basins&
       outputformat=SHAPE-ZIP&
       CQL_FILTER=pubyear+BETWEEN+
       2005+AND+2010]]></preformat>
<?xmltex \hack{\noindent}?>where <preformat preformat-type="code"><![CDATA[pubyear]]></preformat> is the name of the field containing the
publication year (see Table S1, included as part of the Supplement).
Similarly, <preformat preformat-type="code"><![CDATA[CQL_FILTER=ebe_mmkyr<10]]></preformat> will download all records with a
<inline-formula><mml:math id="M40" display="inline"><mml:mrow class="chem"><mml:msup><mml:mi/><mml:mn mathvariant="normal">10</mml:mn></mml:msup><mml:mi mathvariant="normal">Be</mml:mi></mml:mrow></mml:math></inline-formula> denudation rate <inline-formula><mml:math id="M41" display="inline"><mml:mrow><mml:mo>&lt;</mml:mo><mml:mn mathvariant="normal">10</mml:mn></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M42" display="inline"><mml:mrow><mml:mi mathvariant="normal">mm</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msup><mml:mi mathvariant="normal">kyr</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula>, and
<preformat preformat-type="code"><![CDATA[CQL_FILTER=studyid='S066']]></preformat> will download all records that belong to
study S066. Lastly, it is also possible to subset the data by geographic
location:
<preformat><![CDATA[http://earth.uow.edu.au:80/geoserver/
       wfs?request=GetFeature&typename
       =be10-denude:crn_int_basins&
       outputformat=SHAPE-ZIP&
       BBOX=-0,20,40,60,EPSG:4326]]></preformat>
<?xmltex \hack{\noindent}?>where <preformat preformat-type="code"><![CDATA[0,20,40,60]]></preformat> are the coordinates of the bounding
box used to clip the data (following the format: x1,x2,y1,y2) and
<preformat preformat-type="code"><![CDATA[EPSG:4326]]></preformat> indicates that the coordinates are WGS84 latitude and
longitude in degrees (for a complete list of EPSG references see
<uri>http://spatialreference.org</uri>, last access: 28 November 2018).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F4" specific-use="star"><caption><p id="d1e1036">Screenshot of the QGIS application interface displaying data from
OCTOPUS accessed through a WFS connection. A WFS connection will provide
direct access to the data, meaning that (1) its symbology can be modified,
(2) it can be queried, and analysis functions can be run on it.</p></caption>
          <?xmltex \igopts{width=497.923228pt}?><graphic xlink:href="https://essd.copernicus.org/articles/10/2123/2018/essd-10-2123-2018-f04.png"/>

        </fig>

      <p id="d1e1045">For users that wish to display and interrogate the data without actually
downloading any files, it is possible to access OCTOPUS from QGIS directly by
using the “add WFS layer” function and connecting to
<preformat><![CDATA[http://earth.uow.edu.au:80/geoserver/wfs]]></preformat>
<?xmltex \hack{\noindent}?>QGIS is a free and open-source cross-platform desktop GIS
application that supports viewing, editing, and analysis of geospatial data
(<uri>https://www.qgis.org</uri>, last access: 28 November 2018). An example QGIS
session with a WFS connection to OCTOPUS is shown in Fig. <xref ref-type="fig" rid="Ch1.F4"/>. A
WFS connection will provide direct access to the data, and so any data
accessed remotely is treated in the same way as data stored locally. Thus, it
is possible to modify the symbology of the layers, query the data, and run
analysis functions on them. However, all the above come at the cost of much
more data being transmitted, and so users wanting to perform analyses on the
OCTOPUS collections are recommended to instead download a local copy of the
data first using one of the methods described above.</p>
</sec>
</sec>
<sec id="Ch1.S4">
  <title>The OCTOPUS data collections and data structure</title>
      <p id="d1e1065">The compiled CRN and OSL–TL data are organised in three collections, namely
(i) CRN International, including <inline-formula><mml:math id="M43" display="inline"><mml:mrow class="chem"><mml:msup><mml:mi/><mml:mn mathvariant="normal">10</mml:mn></mml:msup><mml:mi mathvariant="normal">Be</mml:mi></mml:mrow></mml:math></inline-formula> (and <inline-formula><mml:math id="M44" display="inline"><mml:mrow class="chem"><mml:msup><mml:mi/><mml:mn mathvariant="normal">26</mml:mn></mml:msup><mml:mi mathvariant="normal">Al</mml:mi></mml:mrow></mml:math></inline-formula>)
measurements in fluvial sediment samples from across the globe but excluding
Australia; (ii) CRN Australia, including <inline-formula><mml:math id="M45" display="inline"><mml:mrow class="chem"><mml:msup><mml:mi/><mml:mn mathvariant="normal">10</mml:mn></mml:msup><mml:mi mathvariant="normal">Be</mml:mi></mml:mrow></mml:math></inline-formula> (and
<inline-formula><mml:math id="M46" display="inline"><mml:mrow class="chem"><mml:msup><mml:mi/><mml:mn mathvariant="normal">26</mml:mn></mml:msup><mml:mi mathvariant="normal">Al</mml:mi></mml:mrow></mml:math></inline-formula>) measurements in fluvial sediment samples from Australia; and
(iii) OSL &amp; TL Australia, including OSL and TL measurements in
fluvial sediment samples from stratigraphic sections and sediment cores from
across the Australian continent. The aim of OCTOPUS is to<?pagebreak page2130?> compile and
incorporate all data – both published and unpublished – that is publicly
available and we do not think that it is our role to decide on the quality of
the data that is already published. However, in some instances, where a
publication did not provide sufficient information for the data files to be
produced (e.g, insufficient information to be able to confidently locate and
delineate drainage basins) and this information could not be obtained from
elsewhere, those data were excluded from OCTOPUS. Further, despite our best
efforts it is likely that we have missed some studies during our search.
Given the above, there are studies that were excluded from the current
release of OCTOPUS. This was not an editorial decision except in cases where
we had no choice due to a lack of information (see above).</p>

      <?xmltex \floatpos{p}?><fig id="Ch1.F5" specific-use="star"><caption><p id="d1e1118">Data organisation diagrams for the CRN and OSL–TL collections. See
text for details.</p></caption>
        <?xmltex \igopts{width=441.017717pt}?><graphic xlink:href="https://essd.copernicus.org/articles/10/2123/2018/essd-10-2123-2018-f05.png"/>

      </fig>

<sec id="Ch1.S4.SS1">
  <title>CRN International and CRN Australia</title>
      <?pagebreak page2132?><p id="d1e1132">The CRN International and CRN Australia collections consist of
<inline-formula><mml:math id="M47" display="inline"><mml:mrow class="chem"><mml:msup><mml:mi/><mml:mn mathvariant="normal">10</mml:mn></mml:msup><mml:mi mathvariant="normal">Be</mml:mi></mml:mrow></mml:math></inline-formula> (and where available, also <inline-formula><mml:math id="M48" display="inline"><mml:mrow class="chem"><mml:msup><mml:mi/><mml:mn mathvariant="normal">26</mml:mn></mml:msup><mml:mi mathvariant="normal">Al</mml:mi></mml:mrow></mml:math></inline-formula>) basin-wide
denudation rates published in the peer-reviewed literature up to 2018. As
already mentioned, the data are organised in studies, with files belonging to
each study stored in separated zip archives (Fig. <xref ref-type="fig" rid="Ch1.F5"/>).
The mean sample number per study is <inline-formula><mml:math id="M49" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">20</mml:mn></mml:mrow></mml:math></inline-formula> and the ratio of published
<inline-formula><mml:math id="M50" display="inline"><mml:mrow class="chem"><mml:msup><mml:mi/><mml:mn mathvariant="normal">26</mml:mn></mml:msup><mml:mi mathvariant="normal">Al</mml:mi></mml:mrow></mml:math></inline-formula> to published <inline-formula><mml:math id="M51" display="inline"><mml:mrow class="chem"><mml:msup><mml:mi/><mml:mn mathvariant="normal">10</mml:mn></mml:msup><mml:mi mathvariant="normal">Be</mml:mi></mml:mrow></mml:math></inline-formula> measurements is approximately 1 to
10. For each <inline-formula><mml:math id="M52" display="inline"><mml:mrow class="chem"><mml:msup><mml:mi/><mml:mn mathvariant="normal">10</mml:mn></mml:msup><mml:mi mathvariant="normal">Be</mml:mi></mml:mrow></mml:math></inline-formula> data point, there is a point geometry file
representing the location of the sample site, and a polygon geometry file
representing the outline of the drainage basin from which the sampled
material is originating. An attribute table including published and
recalculated <inline-formula><mml:math id="M53" display="inline"><mml:mrow class="chem"><mml:msup><mml:mi/><mml:mn mathvariant="normal">10</mml:mn></mml:msup><mml:mi mathvariant="normal">Be</mml:mi></mml:mrow></mml:math></inline-formula> (and <inline-formula><mml:math id="M54" display="inline"><mml:mrow class="chem"><mml:msup><mml:mi/><mml:mn mathvariant="normal">26</mml:mn></mml:msup><mml:mi mathvariant="normal">Al</mml:mi></mml:mrow></mml:math></inline-formula>) data and a comprehensive set
of metadata is linked to the polygon geometry file. A complete description of
all attribute data entries is provided in Table S1, included as part of the
Supplement. For each study, each zip archive also includes seven raster
layers: (i) a hydrologically corrected DEM with elevation values in metres
(file name suffix: <preformat preformat-type="code"><![CDATA[_demhydro]]></preformat>), (ii) a flow-direction raster calculated
using the D8 flow-routing method <xref ref-type="bibr" rid="bib1.bibx48" id="paren.33"/>
(<preformat preformat-type="code"><![CDATA[_d8flowdir]]></preformat>), (iii) a flow-accumulation raster calculated with the
same D8 method (<preformat preformat-type="code"><![CDATA[_flowacc]]></preformat>), (iv) a slope gradient raster calculated
using the method described in <xref ref-type="bibr" rid="bib1.bibx43" id="text.34"/> with units in
<inline-formula><mml:math id="M55" display="inline"><mml:mrow><mml:mi mathvariant="normal">m</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msup><mml:mi mathvariant="normal">km</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula> (<preformat preformat-type="code"><![CDATA[_gradmkm]]></preformat>), (v) an atmospheric pressure raster,
showing local atmospheric pressure in <inline-formula><mml:math id="M56" display="inline"><mml:mi mathvariant="normal">hPa</mml:mi></mml:math></inline-formula> calculated based on the
NCEP2 climate reanalysis data <xref ref-type="bibr" rid="bib1.bibx22" id="paren.35"/> (<preformat preformat-type="code"><![CDATA[_atmospres]]></preformat>),
(vi) a cosmogenic nuclide production scaling raster calculated using the
method described in <xref ref-type="bibr" rid="bib1.bibx72" id="text.36"/> (<preformat preformat-type="code"><![CDATA[_prodscale]]></preformat>), and (vii) a
cosmogenic nuclide production topographic shielding raster calculated using
the method described in <xref ref-type="bibr" rid="bib1.bibx18" id="text.37"/> (<preformat preformat-type="code"><![CDATA[_toposhield]]></preformat>). All
raster layers were derived using the Shuttle Radar Topography Mission (SRTM)
90 <inline-formula><mml:math id="M57" display="inline"><mml:mi mathvariant="normal">m</mml:mi></mml:math></inline-formula> Digital Elevation Database <xref ref-type="bibr" rid="bib1.bibx29" id="paren.38"/> and extend
20 <inline-formula><mml:math id="M58" display="inline"><mml:mi mathvariant="normal">km</mml:mi></mml:math></inline-formula> beyond the boundaries of the drainage basins in each study. For
two studies, namely <xref ref-type="bibr" rid="bib1.bibx41" id="text.39"/> and <xref ref-type="bibr" rid="bib1.bibx62" id="text.40"/>, due
to very large basin areas, all raster layers with the exception of slope
gradient were calculated from SRTM data resampled to 500 <inline-formula><mml:math id="M59" display="inline"><mml:mi mathvariant="normal">m</mml:mi></mml:math></inline-formula>
resolution. Each zip archive also includes a series of text files
representing CAIRN configuration and input data files, and CAIRN output
files, including files to be used with the online calculators formerly known
as the CRONUS-Earth online calculators <xref ref-type="bibr" rid="bib1.bibx7" id="paren.41"/>.</p>
      <p id="d1e1329">Published <inline-formula><mml:math id="M60" display="inline"><mml:mrow class="chem"><mml:msup><mml:mi/><mml:mn mathvariant="normal">10</mml:mn></mml:msup><mml:mi mathvariant="normal">Be</mml:mi></mml:mrow></mml:math></inline-formula> concentrations (<inline-formula><mml:math id="M61" display="inline"><mml:mrow><mml:mi mathvariant="normal">atoms</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msup><mml:mi mathvariant="normal">g</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula>) were
renormalised to the Nishiizumi 2007 <inline-formula><mml:math id="M62" display="inline"><mml:mrow class="chem"><mml:msup><mml:mi/><mml:mn mathvariant="normal">10</mml:mn></mml:msup><mml:mi mathvariant="normal">Be</mml:mi></mml:mrow></mml:math></inline-formula> AMS standard
<xref ref-type="bibr" rid="bib1.bibx57" id="paren.42"/>, and basin-wide denudation rates recalculated with
CAIRN. Basin-averaged nuclide production from neutrons and muons was
calculated with the approximation of <xref ref-type="bibr" rid="bib1.bibx12" id="text.43"/> and using a
sea-level and high-latitude total <inline-formula><mml:math id="M63" display="inline"><mml:mrow class="chem"><mml:msup><mml:mi/><mml:mn mathvariant="normal">10</mml:mn></mml:msup><mml:mi mathvariant="normal">Be</mml:mi></mml:mrow></mml:math></inline-formula> production rate of
4.3 <inline-formula><mml:math id="M64" display="inline"><mml:mrow><mml:mi mathvariant="normal">atoms</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msup><mml:mi mathvariant="normal">g</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msup><mml:mi mathvariant="normal">yr</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula> <xref ref-type="bibr" rid="bib1.bibx56" id="paren.44"/>. Production rates
for catchment-wide denudation rates were calculated at every pixel using the
SRTM 90 <inline-formula><mml:math id="M65" display="inline"><mml:mi mathvariant="normal">m</mml:mi></mml:math></inline-formula> DEM, with the time-independent Lal/Stone scaling scheme
<xref ref-type="bibr" rid="bib1.bibx72" id="paren.45"/>. Atmospheric pressure was calculated via interpolation
from the NCEP2 reanalysis data <xref ref-type="bibr" rid="bib1.bibx22" id="paren.46"/>. Topographic shielding
was calculated from the same DEM using the method of <xref ref-type="bibr" rid="bib1.bibx18" id="text.47"/>
with <inline-formula><mml:math id="M66" display="inline"><mml:mrow><mml:mi mathvariant="italic">θ</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">8</mml:mn></mml:mrow></mml:math></inline-formula><inline-formula><mml:math id="M67" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> and <inline-formula><mml:math id="M68" display="inline"><mml:mrow><mml:mi mathvariant="italic">ϕ</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">5</mml:mn></mml:mrow></mml:math></inline-formula><inline-formula><mml:math id="M69" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>. Following the submission
of this paper, a new study by <xref ref-type="bibr" rid="bib1.bibx25" id="text.48"/> showed that topographic
shielding corrections are inappropriate for calculating basin-wide denudation
rates, in most settings, and are only required for steep catchments with
non-uniform distribution of quartz and/or denudation rates. For this reason,
future iterations of the CRN International and CRN
Australia collections will also include <inline-formula><mml:math id="M70" display="inline"><mml:mrow class="chem"><mml:msup><mml:mi/><mml:mn mathvariant="normal">10</mml:mn></mml:msup><mml:mi mathvariant="normal">Be</mml:mi></mml:mrow></mml:math></inline-formula> (and where available
<inline-formula><mml:math id="M71" display="inline"><mml:mrow class="chem"><mml:msup><mml:mi/><mml:mn mathvariant="normal">26</mml:mn></mml:msup><mml:mi mathvariant="normal">Al</mml:mi></mml:mrow></mml:math></inline-formula>) denudation rates calculated without correcting for
topographic shielding. All calculations assumed a <inline-formula><mml:math id="M72" display="inline"><mml:mrow class="chem"><mml:msup><mml:mi/><mml:mn mathvariant="normal">10</mml:mn></mml:msup><mml:mi mathvariant="normal">Be</mml:mi></mml:mrow></mml:math></inline-formula> half-life of
<inline-formula><mml:math id="M73" display="inline"><mml:mrow><mml:mn mathvariant="normal">1.387</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">0.012</mml:mn></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M74" display="inline"><mml:mi mathvariant="normal">Myr</mml:mi></mml:math></inline-formula> <xref ref-type="bibr" rid="bib1.bibx17 bib1.bibx49" id="paren.49"/>.</p>
      <p id="d1e1540">For simplicity and consistency across the global compilation, no corrections
were made for lithological differences in quartz abundance, glacier cover,
and snow shielding. Performing such corrections in a consistent manner on a
global scale is impossible. However, all CAIRN input and configuration files
are provided and these corrections can be readily applied by end users to
individual studies. Further, CRN International and CRN
Australia include both the originally published denudation rates and the
ones recalculated using CAIRN, and so detailed comparisons can be made by
users. Figure <xref ref-type="fig" rid="Ch1.F6"/> shows a first-order
comparison between published and recalculated <inline-formula><mml:math id="M75" display="inline"><mml:mrow class="chem"><mml:msup><mml:mi/><mml:mn mathvariant="normal">10</mml:mn></mml:msup><mml:mi mathvariant="normal">Be</mml:mi></mml:mrow></mml:math></inline-formula> denudation
rates. With the exception of a small number of data points (<inline-formula><mml:math id="M76" display="inline"><mml:mrow><mml:mi>n</mml:mi><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">10</mml:mn></mml:mrow></mml:math></inline-formula>),
there is good agreement between published and recalculated <inline-formula><mml:math id="M77" display="inline"><mml:mrow class="chem"><mml:msup><mml:mi/><mml:mn mathvariant="normal">10</mml:mn></mml:msup><mml:mi mathvariant="normal">Be</mml:mi></mml:mrow></mml:math></inline-formula>
denudation rates, with no obvious trends related to elevation or basin size.
Where large discrepancies exist, these are due either to differences in
drainage basins as published versus drainage basins identified on the SRTM
DEM during data recalculation or due to corrections that were applied to the
data in the original publication that were not appropriately described in the
latter. Discrepancies also exist in the case of studies where substantial
portions of a drainage basin consisted on non-quartz-bearing lithologies
<xref ref-type="bibr" rid="bib1.bibx67 bib1.bibx23" id="paren.50"><named-content content-type="pre">e.g.</named-content></xref> and where corrections for quartz
abundance were applied to the data in the original publications but were not
replicated here. The number of such basins is small, however, and will not
impact any regional or larger-scale analyses done with the CRN data. For
small-scale studies users should compare published with recalculated
denudation rates and determine whether a new recalculation that involves
corrections for quartz abundance, glacier cover, and/or snow shielding is
warranted.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F6"><caption><p id="d1e1588">Published versus recalculated <inline-formula><mml:math id="M78" display="inline"><mml:mrow class="chem"><mml:msup><mml:mi/><mml:mn mathvariant="normal">10</mml:mn></mml:msup><mml:mi mathvariant="normal">Be</mml:mi></mml:mrow></mml:math></inline-formula>-based denudation rates.
Data points are coloured according to average basin elevation and circle
sizes are proportional to basin area. Note the good agreement between the
two data sets and the lack of obvious trends related to basin elevation and
basin area.</p></caption>
          <?xmltex \igopts{width=227.622047pt}?><graphic xlink:href="https://essd.copernicus.org/articles/10/2123/2018/essd-10-2123-2018-f06.png"/>

        </fig>

      <p id="d1e1610">Approximately 5 % of compiled <inline-formula><mml:math id="M79" display="inline"><mml:mrow class="chem"><mml:msup><mml:mi/><mml:mn mathvariant="normal">10</mml:mn></mml:msup><mml:mi mathvariant="normal">Be</mml:mi></mml:mrow></mml:math></inline-formula> measurements – all of which
were published in two highly regarded journals – could not be incorporated
into OCTOPUS due to information that is insufficient to reproduce drainage basin
extents.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F7" specific-use="star"><caption><p id="d1e1627">The global CRN data set: <bold>(a)</bold> geographical extent and
latitudinal sample distribution, <bold>(b)</bold> average basin slope versus
recalculated <inline-formula><mml:math id="M80" display="inline"><mml:mrow class="chem"><mml:msup><mml:mi/><mml:mn mathvariant="normal">10</mml:mn></mml:msup><mml:mi mathvariant="normal">Be</mml:mi></mml:mrow></mml:math></inline-formula> denudation rate, and <bold>(c)</bold> average basin
elevation versus recalculated <inline-formula><mml:math id="M81" display="inline"><mml:mrow class="chem"><mml:msup><mml:mi/><mml:mn mathvariant="normal">10</mml:mn></mml:msup><mml:mi mathvariant="normal">Be</mml:mi></mml:mrow></mml:math></inline-formula> denudation rate. Data points
in <bold>(b)</bold> and <bold>(c)</bold> are coloured according to average basin
elevation and circle sizes are proportional with basin area. Contour lines
show kernel density estimates for the point clouds (arbitrary units).</p></caption>
          <?xmltex \igopts{width=369.885827pt}?><graphic xlink:href="https://essd.copernicus.org/articles/10/2123/2018/essd-10-2123-2018-f07.png"/>

        </fig>

      <p id="d1e1676">In terms of geographical extent, the global CRN compilation exhibits
considerable bias (Fig. <xref ref-type="fig" rid="Ch1.F7"/>a). The majority of the
<inline-formula><mml:math id="M82" display="inline"><mml:mrow class="chem"><mml:msup><mml:mi/><mml:mn mathvariant="normal">10</mml:mn></mml:msup><mml:mi mathvariant="normal">Be</mml:mi></mml:mrow></mml:math></inline-formula> (and <inline-formula><mml:math id="M83" display="inline"><mml:mrow class="chem"><mml:msup><mml:mi/><mml:mn mathvariant="normal">26</mml:mn></mml:msup><mml:mi mathvariant="normal">Al</mml:mi></mml:mrow></mml:math></inline-formula>) measurements are from Northern Hemisphere
drainage basins, clustering around distinct, mostly tectonically active,
topographic regions, such as the Pacific coast of the United States, the
Appalachians, the European<?pagebreak page2133?> Alps, and the Tibet-Himalaya region. Due to some recent
studies, there is also good coverage of the South American Cordillera.
However, there is a considerable lack of data from low-gradient and
tectonically passive regions, such as large parts of Australia, most of
Africa, and most of Asia less the Tibet-Himalaya region. Further, there are
no data from latitudes above <inline-formula><mml:math id="M84" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">55</mml:mn></mml:mrow></mml:math></inline-formula><inline-formula><mml:math id="M85" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>. The observed geographical
bias is a reflection of the intense interest of the geomorphological
community in estimating rates of erosion and weathering in tectonically
active mountain regions with one of several aims to understand the role of
surface processes in the global climate system (e.g.
<xref ref-type="bibr" rid="bib1.bibx55" id="altparen.51"/>; <?xmltex \hack{\mbox\bgroup}?><xref ref-type="bibr" rid="bib1.bibx61" id="altparen.52"/><?xmltex \hack{\egroup}?>;
<xref ref-type="bibr" rid="bib1.bibx78 bib1.bibx42" id="altparen.53"/>). Further, the
lack of data from high latitudes is partly due to the desire to stay away
from formerly glaciated environments. Although the geographical bias does not
make the CRN collection less valuable, it may confound studies aiming to
infer global-scale trends from these data
<xref ref-type="bibr" rid="bib1.bibx60 bib1.bibx79 bib1.bibx40" id="paren.54"><named-content content-type="pre">cf.</named-content></xref>.
Despite the geographical bias, however, the global CRN data sample basins
with a wide range of slope gradients, elevations, and basin areas
(Fig. <xref ref-type="fig" rid="Ch1.F7"/>b–c).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F8" specific-use="star"><caption><p id="d1e1744">The spatial and temporal extents of the OSL &amp; TL Australia data set.
Blue triangles denote TL measurements and yellow circles denote OSL
measurements. Grey lines depict major topographic drainage divisions and
river regions based on the Australian Hydrological Geospatial Fabric
(Geofabric).</p></caption>
          <?xmltex \igopts{width=355.659449pt}?><graphic xlink:href="https://essd.copernicus.org/articles/10/2123/2018/essd-10-2123-2018-f08.png"/>

        </fig>

</sec>
<sec id="Ch1.S4.SS2">
  <?xmltex \opttitle{OSL \& TL Australia}?><title>OSL &amp; TL Australia</title>
      <?pagebreak page2134?><p id="d1e1760">The OSL &amp; TL Australia collection consists of thermoluminescence (TL) and
optically stimulated luminescence (OSL) measurements in fluvial sediment
samples from stratigraphic sections and sediment cores from across the
Australian continent. The collection includes data published in the
peer-reviewed literature up to 2017 and also previously unpublished data
compiled from technical reports and various Honours, MSc, and PhD theses. The
majority of the TL data are from sources published from 1986 up to 2005,
whereas the majority of the OSL data are from sources less than 10 years old
(Fig. <xref ref-type="fig" rid="Ch1.F8"/>). In terms of geographical extent both TL
and OSL data are concentrated in the south-eastern and eastern parts of the
Australian continent, with <inline-formula><mml:math id="M86" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">500</mml:mn></mml:mrow></mml:math></inline-formula> measurements from Australia's largest
river basins – Lake Eyre (LEB) and Murray-Darling (MDB) basins – and with
an equal amount from rivers draining the eastern seaboard
(Fig. <xref ref-type="fig" rid="Ch1.F8"/>). The western half of Australia is
severely understudied, with one single OSL study for the entire region,
namely <xref ref-type="bibr" rid="bib1.bibx74" id="text.55"/>. Focused interest on river systems is proximal
to high-population density areas, where floods are a potential threat (e.g.
Brisbane River, after major floods in 2011;
<?xmltex \hack{\mbox\bgroup}?><xref ref-type="bibr" rid="bib1.bibx24" id="altparen.56"/><?xmltex \hack{\egroup}?>), or where rivers are of great agricultural
importance, such as the MDB. This well-justified bias, however, leaves a gap in the understanding of regions dominated by rivers that are now dry or ephemeral and yet that could
hold information on past climatic regimes now buried under the desert
sand. The focus on
south-eastern coastal river systems draining the Great Dividing Range could
be a source of bias in continent-wide interpretations, where the rivers
draining the western intracontinental ranges and plains remain
underrepresented.</p>
      <?pagebreak page2135?><p id="d1e1785">Similarly to the CRN collections, the data are organised in studies – each
publication is a study – with files belonging to each study stored in
separated zip archives (Fig. <xref ref-type="fig" rid="Ch1.F5"/>). For each OSL or TL
data point, there is a point geometry file representing the location of the
sample site. An attribute table including published OSL or TL ages and a
comprehensive set of metadata is linked to the point geometry file (a
complete description of all attribute data entries is provided in Table S2,
included as part of the Supplement). The zip archive also includes two
separate polygon geometry files: one representing the outline of the drainage
basin of the most downstream sample and one representing the area extending
20 <inline-formula><mml:math id="M87" display="inline"><mml:mi mathvariant="normal">km</mml:mi></mml:math></inline-formula> beyond the boundaries of this drainage basin. For studies with
basin areas up to 100 000 <inline-formula><mml:math id="M88" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">km</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>, each zip archive also includes
four raster layers: (i) a hydrologically corrected DEM with elevation values
in <inline-formula><mml:math id="M89" display="inline"><mml:mi mathvariant="normal">m</mml:mi></mml:math></inline-formula> (file name suffix: <preformat preformat-type="code"><![CDATA[_demhydro]]></preformat>), (ii) a flow-direction
raster calculated using the D8 flow-routing method
<xref ref-type="bibr" rid="bib1.bibx48" id="paren.57"/> (<preformat preformat-type="code"><![CDATA[_d8flowdir]]></preformat>), (iii) a flow-accumulation
raster calculated with the same D8 method (<preformat preformat-type="code"><![CDATA[_flowacc]]></preformat>), and (iv) a
slope gradient raster calculated using the method described in
<xref ref-type="bibr" rid="bib1.bibx43" id="text.58"/> with units in <inline-formula><mml:math id="M90" display="inline"><mml:mrow><mml:mi mathvariant="normal">m</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msup><mml:mi mathvariant="normal">km</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula> (<preformat preformat-type="code"><![CDATA[_gradmkm]]></preformat>). All
raster layers were derived using the hydrologically enforced SRTM
30 <inline-formula><mml:math id="M91" display="inline"><mml:mi mathvariant="normal">m</mml:mi></mml:math></inline-formula> digital elevation model (DEM-H) obtained from Geoscience
Australia <xref ref-type="bibr" rid="bib1.bibx36" id="paren.59"/> and were clipped to the extent of the 20 <inline-formula><mml:math id="M92" display="inline"><mml:mi mathvariant="normal">km</mml:mi></mml:math></inline-formula>
buffer polygon layer. For studies with basin areas exceeding
100 000 <inline-formula><mml:math id="M93" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">km</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>
<xref ref-type="bibr" rid="bib1.bibx15 bib1.bibx11 bib1.bibx47" id="paren.60"><named-content content-type="pre">e.g.</named-content></xref> raster
layers (i) to (iii) were derived using Geoscience Australia's GEODATA
250 <inline-formula><mml:math id="M94" display="inline"><mml:mi mathvariant="normal">m</mml:mi></mml:math></inline-formula> digital elevation model and flow-direction grid
<?xmltex \hack{\mbox\bgroup}?><xref ref-type="bibr" rid="bib1.bibx35" id="paren.61"/><?xmltex \hack{\egroup}?>, as the SRTM DEM produced files that were too large
to transfer online.</p>
</sec>
<sec id="Ch1.S4.SS3">
  <title>Other collections</title>
      <p id="d1e1905">In addition to the CRN and OSL–TL collections described above, the current
version of OCTOPUS also includes additional CRN data organised under two
collections: CRN XXL and CRN In-Prep. These two collections
are not officially supported by the OCTOPUS project, and are included here
only for completeness. The first collection consists of five studies with
samples from the Yangtse <xref ref-type="bibr" rid="bib1.bibx16" id="paren.62"/>, Amazon
<xref ref-type="bibr" rid="bib1.bibx81 bib1.bibx82" id="paren.63"/>, Ganga
<xref ref-type="bibr" rid="bib1.bibx53" id="paren.64"/>, and Brahmaputra basins <xref ref-type="bibr" rid="bib1.bibx54" id="paren.65"/>.
These studies focused on very large basins that could only be handled by
CAIRN when run using a 500 <inline-formula><mml:math id="M95" display="inline"><mml:mi mathvariant="normal">m</mml:mi></mml:math></inline-formula> resolution DEM that, however, produced
drainage basins that were substantially different to what was published,
especially in the case of rivers in the Amazon basin. Further,
<xref ref-type="bibr" rid="bib1.bibx16" id="text.66"/> do not report denudation rates – suggesting that
calculating these might have little meaning for their samples – and both
<xref ref-type="bibr" rid="bib1.bibx81 bib1.bibx82" id="text.67"/> and
<xref ref-type="bibr" rid="bib1.bibx53 bib1.bibx54" id="text.68"/> perform corrections to the data,
some of which (e.g. removing floodplain areas from production rate
calculations) we did not wish to replicate. To this end, CRN XXL
does not include recalculated values nor does it include any raster layers.
CRN In-Prep is an inventory of samples processed at the University
of Wollongong where <inline-formula><mml:math id="M96" display="inline"><mml:mrow class="chem"><mml:msup><mml:mi/><mml:mn mathvariant="normal">10</mml:mn></mml:msup><mml:mi mathvariant="normal">Be</mml:mi></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M97" display="inline"><mml:mrow class="chem"><mml:msup><mml:mi/><mml:mn mathvariant="normal">26</mml:mn></mml:msup><mml:mi mathvariant="normal">Al</mml:mi></mml:mrow></mml:math></inline-formula> have been measured and
the data are not yet published. The collection includes sample metadata and
point and polygon geometry files.</p>
</sec>
</sec>
<sec id="Ch1.S5">
  <title>User contributions to OCTOPUS</title>
      <p id="d1e1969">User contributions to OCTOPUS are welcome. Those wishing to submit data
should download a study and use that as the template for data structure,
formats, and naming convention (see also Fig. <xref ref-type="fig" rid="Ch1.F5"/>). As a
minimum, a contribution should include point and polygon geometry files, and
an attribute table with all records listed in Tables S1 and S2 with the exception
of those records that are output by CAIRN. Data files should be
submitted to the contact address listed in the email received from OCTOPUS
when downloading data. The data collections making up OCTOPUS have been
assigned digital object identifiers (DOIs), and as a consequence, adding new
data needs to follow a versioning scheme, with each new version requiring new
DOIs. Thus, data contributed by users will be incorporated in the next
release of a given collection, rather than being added to the current one.</p><?xmltex \hack{\newpage}?>
</sec>

      
      </body>
    <back><notes notes-type="dataavailability">

      <p id="d1e1979">OCTOPUS can be accessed at <uri>https://earth.uow.edu.au</uri>
(last access: 28 November 2018). The data collections that make up the 2018
release of OCTOPUS (version 1 – Dooku's Dilemma) have been assigned the
following DOIs: <ext-link xlink:href="https://doi.org/10.4225/48/5a8367feac9b2" ext-link-type="DOI">10.4225/48/5a8367feac9b2</ext-link> (CRN International;
<xref ref-type="bibr" rid="bib1.bibx19" id="altparen.69"/>), <ext-link xlink:href="https://doi.org/10.4225/48/5a836cdfac9b5" ext-link-type="DOI">10.4225/48/5a836cdfac9b5</ext-link> (CRN Australia;
<xref ref-type="bibr" rid="bib1.bibx20" id="altparen.70"/>), and <ext-link xlink:href="https://doi.org/10.4225/48/5a836db1ac9b6" ext-link-type="DOI">10.4225/48/5a836db1ac9b6</ext-link> (OSL &amp; TL
Australia; <xref ref-type="bibr" rid="bib1.bibx21" id="altparen.71"/>). A copy of OCTOPUS has also been deployed to
<uri>https://earthtest.uow.edu.au</uri> (last access: 28 November 2018). This copy
is not supported and is used for testing modifications to the website and
data collections before deployment to the official site. Users should refer
to the DOIs provided to ensure that they are accessing the current and
supported version of the data.</p>
  </notes>
<sec id="Ch1.S6" sec-type="conclusions">
  <title>Conclusions</title>
      <p id="d1e2013">We have produced a database of cosmogenic radionuclide and luminescence
measurements in fluvial sediment and we have built infrastructure for hosting
and maintaining the data at the University of Wollongong and making them
available to the research community via an Open Geospatial Consortium (OGC)-compliant web service. The database consists of <inline-formula><mml:math id="M98" display="inline"><mml:mrow class="chem"><mml:msup><mml:mi/><mml:mn mathvariant="normal">10</mml:mn></mml:msup><mml:mi mathvariant="normal">Be</mml:mi></mml:mrow></mml:math></inline-formula>,
<inline-formula><mml:math id="M99" display="inline"><mml:mrow class="chem"><mml:msup><mml:mi/><mml:mn mathvariant="normal">26</mml:mn></mml:msup><mml:mi mathvariant="normal">Al</mml:mi></mml:mrow></mml:math></inline-formula>, TL, and OSL measurements in fluvial sediment samples along
with ancillary geospatial vector and raster layers. Sample metadata are
comprehensive and include all necessary information for the recalculation of
<inline-formula><mml:math id="M100" display="inline"><mml:mrow class="chem"><mml:msup><mml:mi/><mml:mn mathvariant="normal">10</mml:mn></mml:msup><mml:mi mathvariant="normal">Be</mml:mi></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M101" display="inline"><mml:mrow class="chem"><mml:msup><mml:mi/><mml:mn mathvariant="normal">26</mml:mn></mml:msup><mml:mi mathvariant="normal">Al</mml:mi></mml:mrow></mml:math></inline-formula> denudation rates using the CAIRN program.
The repository and visualisation system enable easy search and discovery of
available data. Use of open standards also ensures that data layers are
visible to other OGC-compliant data-sharing services. Thus, this project will
turn data that were previously invisible to those not within the CRN and
luminescence research community into a findable resource. This aspect is of
particular importance to industry or local government who are yet to discover
the value of geochronological data, for example, in evaluating how
human-induced land use practices have accelerated soil erosion and which
measures are necessary for restoring these rates to their natural benchmark
levels. Our intention is for OCTOPUS to become the default go-to place for
CRN and luminescence data. The availability of the repository and its
associated data curation framework will provide the opportunity for
researchers to store, curate, recalculate and reuse previously published but
otherwise unusable CRN and luminescence data. This delivers the potential to
harness old but valuable data that would otherwise be lost to the research
community. OCTOPUS will enable new research and generate new knowledge by
converting a multitude of disconnected data sets into one connected and
streamlined database. Current data sets allow local-scale analyses. The
streamlined database will allow for regional-scale and<?pagebreak page2136?> even continental- or
global-scale analyses. The transparent data reanalysis framework will also
reduce research time and avoid the duplication of effort, which will be highly
attractive to other researchers. Ultimately, OCTOPUS will ensure that CRN and
luminescence data are reusable beyond the scope of the project for which they
were initially collected.</p><supplementary-material position="anchor"><p id="d1e2063">The supplement related to this article is available online at: <inline-supplementary-material xlink:href="https://doi.org/10.5194/essd-10-2123-2018-supplement" xlink:title="pdf">https://doi.org/10.5194/essd-10-2123-2018-supplement</inline-supplementary-material>.</p></supplementary-material>
</sec><notes notes-type="authorcontribution">

      <p id="d1e2073">ATC, HM, TJC, and  WMS compiled the CRN and luminescence data;
ATC and HM performed the GIS analyses and the data recalculations using CAIRN with input
from SMM; AG designed and built the OCTOPUS platform and web interface with input
from ATC. All authors contributed to the writing of the manuscript.</p>
  </notes><notes notes-type="competinginterests">

      <p id="d1e2079">The authors declare that they have no conflict of
interest.</p>
  </notes><ack><title>Acknowledgements</title><p id="d1e2085">We acknowledge financial support from the Australian National Data Service
(ANDS – Project HVC15) and the University of Wollongong (UOW) to
Alexandru T. Codilean and Timothy J. Cohen. Henry Munack benefited from an
Endeavour Postdoctoral Research Fellowship granted by the Australian
Government. A prototype of OCTOPUS was built while Alexandru T. Codilean
worked at the Deutsches GeoForschungsZentrum (GFZ). We thank Monika Oakman,
Ben Cornwell, Peter Newnam, Clare Job, Gabriel Enge, Heidi Brown,
Alan Glixman, and Keith Russell for their support during this project. We
also thank the CRN and luminescence communities for generously sharing their
data. We thank Greg Balco, Zsófia Ruszkiczay-Rüdiger,
Sebastian Kreutzer, and István Gábor Hatvani for careful reviews of
the discussion paper. We also thank Ingrid Ward, Todd Ehlers, and
Vincent Godard for providing comments on the discussion
paper.<?xmltex \hack{\newline}?><?xmltex \hack{\newline}?> Edited by: Attila Demény<?xmltex \hack{\newline}?> Reviewed by: Greg
Balco, Sebastian Kreutzer, Zsófia Ruszkiczay-Rüdiger, and István
Gábor Hatvani</p></ack><ref-list>
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    <!--<article-title-html>OCTOPUS: an open cosmogenic isotope and luminescence database</article-title-html>
<abstract-html><p>We present a database of cosmogenic radionuclide and luminescence measurements
in fluvial sediment. With support from the Australian National Data Service
(ANDS) we have built infrastructure for hosting and maintaining the data at
the University of Wollongong and making this available to the research
community via an Open Geospatial Consortium (OGC)-compliant web service. The
cosmogenic radionuclide (CRN) part of the database consists of <sup>10</sup>Be
and <sup>26</sup>Al measurements in modern fluvial sediment samples from
across the globe, along with ancillary geospatial vector and raster layers,
including sample site, basin outline, digital elevation model, gradient
raster, flow-direction and flow-accumulation rasters, atmospheric pressure
raster, and CRN production scaling and topographic shielding factor rasters.
Sample metadata are comprehensive and include all necessary information for
the recalculation of denudation rates using CAIRN, an open-source
program for calculating
basin-wide denudation rates from <sup>10</sup>Be and <sup>26</sup>Al data.
Further all data have been recalculated and harmonised using the same
program. The luminescence part of the database consists of
thermoluminescence (TL) and optically stimulated luminescence (OSL)
measurements in fluvial sediment samples from stratigraphic sections and
sediment cores from across the Australian continent and includes ancillary
vector and raster geospatial data. The database can be interrogated and
downloaded via a custom-built web map service. More advanced interrogation
and exporting to various data formats, including the ESRI Shapefile and
Google Earth's KML, is also possible via the Web Feature Service (WFS)
capability running on the OCTOPUS server. Use of open standards also ensures
that data layers are visible to other OGC-compliant data-sharing services.
OCTOPUS and its associated data curation framework provide the opportunity
for researchers to reuse previously published but otherwise unusable CRN and
luminescence data. This delivers the potential to harness old but valuable
data that would otherwise be lost to the research community. OCTOPUS can be
accessed at <a href="https://earth.uow.edu.au" target="_blank">https://earth.uow.edu.au</a> (last access: 28 November 2018).
The individual data collections can also be accessed via the following DOIs:
<a href="https://doi.org/10.4225/48/5a8367feac9b2" target="_blank">https://doi.org/10.4225/48/5a8367feac9b2</a> (CRN International),
<a href="https://doi.org/10.4225/48/5a836cdfac9b5" target="_blank">https://doi.org/10.4225/48/5a836cdfac9b5</a> (CRN Australia), and
<a href="https://doi.org/10.4225/48/5a836db1ac9b6" target="_blank">https://doi.org/10.4225/48/5a836db1ac9b6</a> (OSL &amp; TL Australia).</p></abstract-html>
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