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  <front>
    <journal-meta><journal-id journal-id-type="publisher">GMD</journal-id><journal-title-group>
    <journal-title>Geoscientific Model Development</journal-title>
    <abbrev-journal-title abbrev-type="publisher">GMD</abbrev-journal-title><abbrev-journal-title abbrev-type="nlm-ta">Geosci. Model Dev.</abbrev-journal-title>
  </journal-title-group><issn pub-type="epub">1991-9603</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/gmd-11-305-2018</article-id><title-group><article-title>Errors and improvements in the use of archived meteorological <?xmltex \hack{\break}?> data for chemical transport modeling: an analysis using GEOS-Chem v11-01 driven by GEOS-5 meteorology</article-title><alt-title>Transport errors in off-line CTMs</alt-title>
      </title-group><?xmltex \runningtitle{Transport errors in off-line CTMs}?><?xmltex \runningauthor{K.~Yu et al.}?>
      <contrib-group>
        <contrib contrib-type="author" corresp="yes" rid="aff1">
          <name><surname>Yu</surname><given-names>Karen</given-names></name>
          <email>kyu@seas.harvard.edu</email>
        <ext-link>https://orcid.org/0000-0003-1307-3738</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2 aff3">
          <name><surname>Keller</surname><given-names>Christoph A.</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1 aff4">
          <name><surname>Jacob</surname><given-names>Daniel J.</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff3">
          <name><surname>Molod</surname><given-names>Andrea M.</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Eastham</surname><given-names>Sebastian D.</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-2476-4801</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Long</surname><given-names>Michael S.</given-names></name>
          
        </contrib>
        <aff id="aff1"><label>1</label><institution>School of Engineering and Applied Sciences, Harvard University, Cambridge, MA, USA</institution>
        </aff>
        <aff id="aff2"><label>2</label><institution>Universities Space Research Association, Columbia, MD, USA</institution>
        </aff>
        <aff id="aff3"><label>3</label><institution>NASA Goddard Space Flight Center, Greenbelt, MD, USA</institution>
        </aff>
        <aff id="aff4"><label>4</label><institution>Department of Earth and Planetary Sciences, Harvard University, Cambridge, MA, USA</institution>
        </aff>
      </contrib-group>
      <author-notes><corresp id="corr1">Karen Yu (kyu@seas.harvard.edu)</corresp></author-notes><pub-date><day>23</day><month>January</month><year>2018</year></pub-date>
      
      <volume>11</volume>
      <issue>1</issue>
      <fpage>305</fpage><lpage>319</lpage>
      <history>
        <date date-type="received"><day>20</day><month>May</month><year>2017</year></date>
           <date date-type="rev-request"><day>6</day><month>July</month><year>2017</year></date>
           <date date-type="rev-recd"><day>24</day><month>November</month><year>2017</year></date>
           <date date-type="accepted"><day>8</day><month>December</month><year>2017</year></date>
      </history>
      <permissions>
        <copyright-statement>Copyright: © 2018 Karen Yu et al.</copyright-statement>
        <copyright-year>2018</copyright-year>
      <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://gmd.copernicus.org/articles/11/305/2018/gmd-11-305-2018.html">This article is available from https://gmd.copernicus.org/articles/11/305/2018/gmd-11-305-2018.html</self-uri><self-uri xlink:href="https://gmd.copernicus.org/articles/11/305/2018/gmd-11-305-2018.pdf">The full text article is available as a PDF file from https://gmd.copernicus.org/articles/11/305/2018/gmd-11-305-2018.pdf</self-uri>
      <abstract><title>Abstract</title>
    <p id="d1e148">Global simulations of atmospheric chemistry are commonly conducted with
off-line chemical transport models (CTMs) driven by archived meteorological
data from general circulation models (GCMs). The off-line approach has
the advantages of simplicity and expediency, but it incurs errors due to temporal
averaging in the meteorological archive and the inability to reproduce the
GCM transport algorithms exactly. The CTM simulation is also often conducted
at coarser grid resolution than the parent GCM. Here we investigate this
cascade of CTM errors by using <inline-formula><mml:math id="M1" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">222</mml:mn></mml:msup></mml:math></inline-formula>Rn–<inline-formula><mml:math id="M2" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">210</mml:mn></mml:msup></mml:math></inline-formula>Pb–<inline-formula><mml:math id="M3" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">7</mml:mn></mml:msup></mml:math></inline-formula>Be chemical tracer
simulations off-line in the GEOS-Chem CTM at rectilinear
0.25<inline-formula><mml:math id="M4" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M5" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 0.3125<inline-formula><mml:math id="M6" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> (<inline-formula><mml:math id="M7" display="inline"><mml:mo lspace="0mm">≈</mml:mo></mml:math></inline-formula> 25 km) and
2<inline-formula><mml:math id="M8" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M9" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 2.5<inline-formula><mml:math id="M10" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> (<inline-formula><mml:math id="M11" display="inline"><mml:mo lspace="0mm">≈</mml:mo></mml:math></inline-formula> 200 km) resolutions and
online in the parent GEOS-5 GCM at cubed-sphere c360 (<inline-formula><mml:math id="M12" display="inline"><mml:mo lspace="0mm">≈</mml:mo></mml:math></inline-formula> 25 km) and
c48 (<inline-formula><mml:math id="M13" display="inline"><mml:mo lspace="0mm">≈</mml:mo></mml:math></inline-formula> 200 km) horizontal resolutions. The c360 GEOS-5 GCM
meteorological archive, updated every 3 h and remapped to
0.25<inline-formula><mml:math id="M14" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M15" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 0.3125<inline-formula><mml:math id="M16" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>, is the standard operational product
generated by the NASA Global Modeling and Assimilation Office (GMAO) and used
as input by GEOS-Chem. We find that the GEOS-Chem <inline-formula><mml:math id="M17" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">222</mml:mn></mml:msup></mml:math></inline-formula>Rn simulation at
native 0.25<inline-formula><mml:math id="M18" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M19" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 0.3125<inline-formula><mml:math id="M20" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> resolution is affected by
vertical transport errors of up to 20 % relative to the GEOS-5 c360 online
simulation, in part due to loss of transient organized vertical motions in
the GCM (resolved convection) that are temporally averaged out in the 3 h
meteorological archive. There is also significant error caused by operational
remapping of the meteorological archive from a cubed-sphere to a rectilinear
grid. Decreasing the GEOS-Chem resolution from
0.25<inline-formula><mml:math id="M21" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M22" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 0.3125<inline-formula><mml:math id="M23" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> to
2<inline-formula><mml:math id="M24" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M25" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 2.5<inline-formula><mml:math id="M26" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> induces further weakening of vertical
transport as transient vertical motions are averaged out spatially and
temporally. The resulting <inline-formula><mml:math id="M27" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">222</mml:mn></mml:msup></mml:math></inline-formula>Rn concentrations simulated by the
coarse-resolution GEOS-Chem are overestimated by up to 40 % in surface air
relative to the online c360 simulations and underestimated by up to 40 %
in the upper troposphere, while the tropospheric lifetimes of <inline-formula><mml:math id="M28" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">210</mml:mn></mml:msup></mml:math></inline-formula>Pb and
<inline-formula><mml:math id="M29" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">7</mml:mn></mml:msup></mml:math></inline-formula>Be against aerosol deposition are affected by 5–10 %. The lost
vertical transport in the coarse-resolution GEOS-Chem simulation can be
partly restored by recomputing the convective mass fluxes at the appropriate
resolution to replace the archived convective mass fluxes and by correcting
for bias in the spatial averaging of boundary layer mixing depths.</p>
  </abstract>
    </article-meta>
  </front>
<body>
      

<sec id="Ch1.S1" sec-type="intro">
  <label>1</label><title>Introduction</title>
      <p id="d1e405">Accurate simulation of transport is crucial for global models of atmospheric
composition. Transport information is provided by general circulation models (GCMs)
that solve the conservation equations for air mass, momentum, heat,
and water and may assimilate meteorological observations to reproduce a
specific period. GCMs compute grid-resolved winds, sub-grid turbulence, and
convection properties that determine the transport of chemical species
through the corresponding continuity equations <xref ref-type="bibr" rid="bib1.bibx6" id="paren.1"/>. These
equations can be solved “online” as part of the GCM or<?pagebreak page306?> “off-line” by
using archived winds and turbulence statistics to drive a separate chemical
transport model (CTM). The off-line approach has the advantages of simplicity and
economy, but it introduces differences due to temporal (and sometimes
spatial) averaging in the meteorological archive and due to inability to
exactly replicate the GCM transport algorithms. Since the CTM aims to
replicate the original transport of the GCM, any deviation from the GCM
transport can be viewed as an error. Here we use chemical tracers to
investigate the cascade of errors involved in successively degrading a global
online simulation with high spatial resolution through various stages to an
off-line simulation with coarse horizontal spatial resolution and coarse
temporal resolution of input data.</p>
      <p id="d1e411">Whether online or off-line, a model of atmospheric composition computes the
concentrations of atmospheric species by solving the relevant chemical
continuity (mass conservation) equations. In an Eulerian (fixed frame of
reference) framework,

              <disp-formula id="Ch1.E1" content-type="numbered"><label>1</label><mml:math id="M30" display="block"><mml:mstyle class="stylechange" displaystyle="true"/><mml:mrow><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mo>∂</mml:mo><mml:msub><mml:mi mathvariant="italic">ρ</mml:mi><mml:mi>i</mml:mi></mml:msub></mml:mrow><mml:mrow><mml:mo>∂</mml:mo><mml:mi>t</mml:mi></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>=</mml:mo><mml:mo>-</mml:mo><mml:mi mathvariant="normal">∇</mml:mi><mml:mo>⋅</mml:mo><mml:mfenced open="(" close=")"><mml:mrow><mml:msub><mml:mi mathvariant="italic">ρ</mml:mi><mml:mi>i</mml:mi></mml:msub><mml:mi mathvariant="bold-italic">v</mml:mi></mml:mrow></mml:mfenced><mml:mo>+</mml:mo><mml:mi mathvariant="normal">∇</mml:mi><mml:mo>⋅</mml:mo><mml:mfenced open="(" close=")"><mml:mrow><mml:mi mathvariant="bold">K</mml:mi><mml:msub><mml:mi mathvariant="italic">ρ</mml:mi><mml:mi mathvariant="normal">a</mml:mi></mml:msub><mml:mi mathvariant="normal">∇</mml:mi><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:msub><mml:mi mathvariant="italic">ρ</mml:mi><mml:mi>i</mml:mi></mml:msub></mml:mrow><mml:mrow><mml:msub><mml:mi mathvariant="italic">ρ</mml:mi><mml:mi mathvariant="normal">a</mml:mi></mml:msub></mml:mrow></mml:mfrac></mml:mstyle></mml:mrow></mml:mfenced><mml:mo>+</mml:mo><mml:msub><mml:mi>P</mml:mi><mml:mi>i</mml:mi></mml:msub><mml:mo>-</mml:mo><mml:msub><mml:mi>L</mml:mi><mml:mi>i</mml:mi></mml:msub><mml:mo>.</mml:mo></mml:mrow></mml:math></disp-formula>

        Here <inline-formula><mml:math id="M31" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">ρ</mml:mi><mml:mi>i</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is the mass density of species <inline-formula><mml:math id="M32" display="inline"><mml:mi>i</mml:mi></mml:math></inline-formula>, <inline-formula><mml:math id="M33" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">ρ</mml:mi><mml:mi mathvariant="normal">a</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is the air
density, <inline-formula><mml:math id="M34" display="inline"><mml:mi mathvariant="bold-italic">v</mml:mi></mml:math></inline-formula> is the wind vector, <inline-formula><mml:math id="M35" display="inline"><mml:mi mathvariant="normal">∇</mml:mi></mml:math></inline-formula> <inline-formula><mml:math id="M36" display="inline"><mml:mo>⋅</mml:mo></mml:math></inline-formula> (<inline-formula><mml:math id="M37" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">ρ</mml:mi><mml:mi>i</mml:mi></mml:msub><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mi mathvariant="bold-italic">v</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>
represents the advection term (flux divergence), and <inline-formula><mml:math id="M38" display="inline"><mml:mrow><mml:msub><mml:mi>P</mml:mi><mml:mi>i</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M39" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M40" display="inline"><mml:mrow><mml:msub><mml:mi>L</mml:mi><mml:mi>i</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>
accounts for local production and loss from chemical reactions.
Small-scale turbulent transport is parameterized in Eq. (1) as an eddy
diffusion term where <inline-formula><mml:math id="M41" display="inline"><mml:mi mathvariant="bold">K</mml:mi></mml:math></inline-formula> is an eddy diffusivity tensor. Additional
parameterizations are applied for convection, which is sub-grid on the
horizontal scale but organized (nonlocal) on the vertical scale. Unlike the
Navier–Stokes conservation equation for momentum, where nonlinear dependence
on momentum introduces chaos in the solution, the chemical continuity
equation has stable solutions when <inline-formula><mml:math id="M42" display="inline"><mml:mi mathvariant="bold-italic">v</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math id="M43" display="inline"><mml:mi mathvariant="bold">K</mml:mi></mml:math></inline-formula> are
specified. This is an important motivation for decoupling the CTM from the
GCM and using archives of <inline-formula><mml:math id="M44" display="inline"><mml:mi mathvariant="bold-italic">v</mml:mi></mml:math></inline-formula>, <inline-formula><mml:math id="M45" display="inline"><mml:mi mathvariant="bold">K</mml:mi></mml:math></inline-formula>, and convection
diagnostics to drive the off-line transport.</p>
      <p id="d1e633">A GCM typically uses a time step of the order of minutes to integrate the
conservation equations for atmospheric dynamics. In an online model, the
chemical continuity equations can be integrated using updated winds on the
same time step. But archiving winds at that resolution for off-line CTM
applications is impractical in terms of data storage. Instead, meteorological
archives for use in CTMs are typically available as temporal averages every
few hours, losing information on eddy motions on shorter timescales that
might affect chemical transport. <xref ref-type="bibr" rid="bib1.bibx45" id="text.2"/> found that 6 h archiving
of GCM meteorological fields did not induce significant off-line chemical
transport error but 24 h archiving did. <xref ref-type="bibr" rid="bib1.bibx11" id="text.3"/> confirmed that
CTMs using meteorology archived at 6 h intervals could reproduce the
transport of the originating GCM. These older GCMs used grid resolutions of
hundreds of kilometers, whereas current GCMs use tens of kilometers. The error from temporal
averaging increases with increasing grid resolution, particularly as the GCM
becomes fine enough to partly resolve convective scales <xref ref-type="bibr" rid="bib1.bibx21" id="paren.4"/>.</p>
      <p id="d1e645">Deep convection is of particular concern for off-line CTM applications.
Vertical convective motions driven by buoyancy are sub-grid on the horizontal
scale but organized on the vertical scale, transporting air across several
vertical model levels in a single time step. Deep convection enables the
transport of short-lived species to high altitudes and scavenges
water-soluble species (such as aerosol particles) in the cloud updrafts.
Convective parameterizations used in GCMs diagnose cloud updrafts,
downdrafts, detrainment and entrainment, and compensatory large-scale subsidence
on the grid scale <xref ref-type="bibr" rid="bib1.bibx6" id="paren.5"/>. It is common practice to use
temporally averaged convective mass fluxes from the GCM archives to drive
off-line models, but the exact timing of events is then lost. A compounding
problem is that current GCMs have sufficiently fine resolution to partly
resolve convective systems on the grid scale, so the parameterized
convection is suppressed in scale-aware schemes <xref ref-type="bibr" rid="bib1.bibx20 bib1.bibx40" id="paren.6"/>.
Typical convective systems persist for less than 1 h, and the
corresponding advective transport is averaged out in a multi-hour wind archive.</p>
      <p id="d1e655">Spatial averaging of the meteorological archive is yet another concern. CTM
simulations of oxidant–aerosol chemistry and/or aerosol microphysics may
require over 100 coupled species. The computational costs are large. A way to
reduce costs is to degrade spatial resolution. It is thus common practice in
CTM applications to average the GCM meteorological fields onto coarser grids
for input to the CTM and operate the CTM at that coarser resolution. But the
averaging may introduce transport biases. For example, vertical eddy fluxes
resolved at the native 0.25<inline-formula><mml:math id="M46" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M47" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 0.3125<inline-formula><mml:math id="M48" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> GCM resolution may
be lost by averaging to the coarser grid.</p>
      <p id="d1e683">Here we examine how the off-line archiving of GCM meteorological data, including
temporal and spatial averaging, affects the simulation of transport in the
GEOS-Chem CTM, and we recommend some corrections for these errors. We use for
this purpose the <inline-formula><mml:math id="M49" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">222</mml:mn></mml:msup></mml:math></inline-formula>Rn–<inline-formula><mml:math id="M50" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">210</mml:mn></mml:msup></mml:math></inline-formula>Pb–<inline-formula><mml:math id="M51" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">7</mml:mn></mml:msup></mml:math></inline-formula>Be tracer suite, which
provides a standard basis for evaluating transport and aerosol scavenging in
CTMs <xref ref-type="bibr" rid="bib1.bibx25 bib1.bibx35 bib1.bibx10 bib1.bibx53" id="paren.7"/>. The
GEOS-Chem CTM, originally described by <xref ref-type="bibr" rid="bib1.bibx5" id="text.8"/>, is an open-source
global model of atmospheric composition used by a large research community
for a wide range of applications. The experiments described here rely on
assimilated meteorological data archived every 3 h from the NASA Goddard
Earth Observation System (GEOS) Data Assimilation System
<xref ref-type="bibr" rid="bib1.bibx47 bib1.bibx18" id="paren.9"><named-content content-type="pre">DAS;</named-content></xref> on a cubed-sphere grid
interpolated to 0.25<inline-formula><mml:math id="M52" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M53" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 0.3125<inline-formula><mml:math id="M54" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> (<inline-formula><mml:math id="M55" display="inline"><mml:mo lspace="0mm">≈</mml:mo></mml:math></inline-formula> 25 km)
horizontal resolution. The GEOS DAS uses the underlying GCM described in
<xref ref-type="bibr" rid="bib1.bibx46" id="text.10"/> and <xref ref-type="bibr" rid="bib1.bibx40" id="text.11"/>. GEOS-Chem CTM simulations can be
conducted at that native resolution, but global simulations generally use
degraded 2<inline-formula><mml:math id="M56" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M57" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 2.5<inline-formula><mml:math id="M58" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> (<inline-formula><mml:math id="M59" display="inline"><mml:mo lspace="0mm">≈</mml:mo></mml:math></inline-formula> 200 km) resolution for
computational expediency. The GEOS-Chem chemical module (solving
<inline-formula><mml:math id="M60" display="inline"><mml:mstyle displaystyle="false"><mml:mfrac style="text"><mml:mrow><mml:mo>∂</mml:mo><mml:msub><mml:mi mathvariant="italic">ρ</mml:mi><mml:mi>i</mml:mi></mml:msub></mml:mrow><mml:mrow><mml:mo>∂</mml:mo><mml:mi>t</mml:mi></mml:mrow></mml:mfrac></mml:mstyle></mml:math></inline-formula> <inline-formula><mml:math id="M61" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M62" display="inline"><mml:mrow><mml:msub><mml:mi>P</mml:mi><mml:mi>i</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M63" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M64" display="inline"><mml:mrow><mml:msub><mml:mi>L</mml:mi><mml:mi>i</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>) has recently been integrated
within the<?pagebreak page307?> GEOS GCM so that simulations with detailed chemistry can be
conducted either online or off-line using the exact same module <xref ref-type="bibr" rid="bib1.bibx38" id="paren.12"/>.</p>
</sec>
<sec id="Ch1.S2">
  <label>2</label><title>Model descriptions</title>
<sec id="Ch1.S2.SS1">
  <label>2.1</label><title>GEOS-5 GCM</title>
      <p id="d1e871">The Goddard Earth Observing System Model version 5 (GEOS-5) is a GCM
developed by the NASA Global Modeling and Analysis Office (GMAO)
<xref ref-type="bibr" rid="bib1.bibx46 bib1.bibx40" id="paren.13"/>. Advection is driven by the finite-volume
dynamical core of <xref ref-type="bibr" rid="bib1.bibx44" id="text.14"/>, which uses sub-stepping to ensure that
the Courant number does not exceed unity. Boundary layer mixing is based on
the nonlocal scheme of <xref ref-type="bibr" rid="bib1.bibx37" id="text.15"/> and the Richardson-number-based
scheme of <xref ref-type="bibr" rid="bib1.bibx39" id="text.16"/>. The convective parameterization is the Relaxed
Arakawa–Schubert (RAS) scheme <xref ref-type="bibr" rid="bib1.bibx41" id="paren.17"/> with a scheme for the
generation and reevaporation of precipitation <xref ref-type="bibr" rid="bib1.bibx3" id="paren.18"/>. RAS
computes the effect of multiple individual cloud plumes released
sequentially using a resolution-dependent stochastic trigger function
<xref ref-type="bibr" rid="bib1.bibx2" id="paren.19"/>. GEOS-5 has 72 vertical levels up to 0.01 hPa on a
hybrid eta (sigma-pressure) grid. The horizontal grid is cubed-sphere
<xref ref-type="bibr" rid="bib1.bibx44" id="paren.20"/> and can operate at a range of resolutions. The integration
of the model equations on the cubed-sphere grid eliminates the problem of
large Courant numbers near the poles and permits straightforward domain
decomposition for distributed-memory environments. The cubed-sphere grid has
been used in other GCMs, such as the Geophysical Fluid Dynamics Laboratory (GFDL)
Atmospheric Model 3 (AM3) <xref ref-type="bibr" rid="bib1.bibx12" id="paren.21"/>.</p>
      <p id="d1e902">We use here the operational GEOS-5 product
(<uri>https://gmao.gsfc.nasa.gov/GMAO_products/NRT_products.php</uri>) generated at a
cubed-sphere c360 (<inline-formula><mml:math id="M65" display="inline"><mml:mo lspace="0mm">≈</mml:mo></mml:math></inline-formula> 25 km) horizontal resolution. The data combines
the GEOS-5 GCM with observations using a hybrid ensemble Kalman filter
three-dimensional variational (3D-Var hybrid) system <xref ref-type="bibr" rid="bib1.bibx48" id="paren.22"/>. The
internal GCM time step for advection and convection is 7.5 min. Output
from the c360 simulation is mapped onto a 0.25<inline-formula><mml:math id="M66" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M67" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 0.3125<inline-formula><mml:math id="M68" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>
latitude <inline-formula><mml:math id="M69" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> longitude rectilinear grid to produce the GEOS forward-processing (GEOS-FP) archive released operationally by GMAO. The archived
data relevant to CTM transport and scavenging include 3-D winds, convective
mass fluxes, precipitation fields, and 2-D surface pressures and boundary
layer mixing depths. The 3-D data are archived as 3 h averages and the 2-D
data as 1 h averages.</p>
      <p id="d1e951">GEOS operational meteorological products have been widely used for off-line
CTM applications including by the University of Maryland (UMD) CTM
<xref ref-type="bibr" rid="bib1.bibx1" id="paren.23"/>, GEOS-Chem <xref ref-type="bibr" rid="bib1.bibx5" id="paren.24"/>, Global Modeling Initiative (GMI)
CTM <xref ref-type="bibr" rid="bib1.bibx13 bib1.bibx14" id="paren.25"/>, Integrated Massively Parallel
Atmospheric Chemical Transport (IMPACT) model <xref ref-type="bibr" rid="bib1.bibx49" id="paren.26"/>, MOZART
<xref ref-type="bibr" rid="bib1.bibx16" id="paren.27"/>, CAM-Chem <xref ref-type="bibr" rid="bib1.bibx30" id="paren.28"/>, and the GEOS CTM
<xref ref-type="bibr" rid="bib1.bibx28" id="paren.29"/>. Chemical transport simulations can also be performed
online within the GEOS-5 GCM <xref ref-type="bibr" rid="bib1.bibx9 bib1.bibx42 bib1.bibx38 bib1.bibx50 bib1.bibx32" id="paren.30"/>.
Although we use GEOS-Chem in our comparisons against online GEOS-5 GCM results,
the issues discussed in this paper are more generally pertinent to CTMs driven
by archived GCM meteorological data.</p>
</sec>
<sec id="Ch1.S2.SS2">
  <label>2.2</label><title>GEOS-Chem CTM</title>
      <p id="d1e987">We use two versions of GEOS-Chem: the standard version 11-01 released in
February 2017 (<uri>http://wiki.seas.harvard.edu/geos-chem/index.php/GEOS-Chem_v11-01</uri>) and a
beta high-performance version (GCHP) designed for massively parallel
computing environments
(<uri>http://wiki.seas.harvard.edu/geos-chem/index.php/GEOS-Chem_HP</uri>). The
standard GEOS-Chem operates on the rectilinear grid from the GEOS-5 archive,
while GCHP operates on the GEOS-5 cubed-sphere grid. Both versions use the
same archived meteorological data and modules except for advection. GCHP uses
an off-line version of the same <xref ref-type="bibr" rid="bib1.bibx44" id="text.31"/> dynamical core as GEOS-5,
while the standard GEOS-Chem uses a dynamical core developed for off-line
applications on a rectilinear grid <xref ref-type="bibr" rid="bib1.bibx34" id="paren.32"/>. The
<xref ref-type="bibr" rid="bib1.bibx34" id="text.33"/> scheme averages winds, surface pressures, and mixing
ratios over the two highest latitude bands to compensate for the polar
singularity. Vertical advection is computed in both cases from the change in
surface pressure, but vertical advection in the standard rectilinear
GEOS-Chem is lower order than in GEOS-5 and GCHP. In the standard rectilinear
GEOS-Chem, a pressure fixer <xref ref-type="bibr" rid="bib1.bibx23" id="paren.34"/> is used to correct for
inconsistencies between horizontal wind divergence and pressure tendencies
resulting from the temporal averaging in the meteorological archive, whereas
GCHP enforces mass consistency by applying a global scaling factor.</p>
      <p id="d1e1009">Convective transport in GEOS-Chem is simulated with a single-plume scheme
using the archived 3 h net updraft and detrainment convective mass fluxes
summing over all RAS plumes within a given grid column <xref ref-type="bibr" rid="bib1.bibx52" id="paren.35"/>.
Although GEOS-Chem reproduces the bulk 3 h convective transport in the GEOS-5
GCM, the precise timing and interactions between RAS convective plumes are not
resolved since that information is not in the archive. Bulk convective
transport using archived mass fluxes is a standard procedure in other CTMs
driven by GEOS-5 meteorology, such as the GMI CTM, and CTMs driven by
other meteorology, such as TOMCAT <xref ref-type="bibr" rid="bib1.bibx17" id="paren.36"><named-content content-type="post">driven by ECMWF reanalysis data</named-content></xref>.</p>
      <?pagebreak page308?><p id="d1e1020">Boundary layer mixing in GEOS-Chem uses the nonlocal parameterization of
<xref ref-type="bibr" rid="bib1.bibx22" id="text.37"/> adapted for GEOS-Chem by <xref ref-type="bibr" rid="bib1.bibx33" id="text.38"/>. It draws on
the archived GEOS-5 mixing depths, temperature, latent and sensible heat
fluxes, and specific humidity. The mixing depths in the GEOS-5 archive are a
diagnostic quantity, and thus boundary layer mixing in GEOS-Chem may differ
from that in the GEOS-5 GCM.</p>
      <p id="d1e1029">GEOS-Chem applications typically use the native horizontal resolution of the
GEOS products for nested simulations over continental-scale domains
<xref ref-type="bibr" rid="bib1.bibx51 bib1.bibx8 bib1.bibx26" id="paren.39"/> but a coarser
2<inline-formula><mml:math id="M70" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M71" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 2.5<inline-formula><mml:math id="M72" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> horizontal resolution for global simulations.
The 2<inline-formula><mml:math id="M73" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M74" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 2.5<inline-formula><mml:math id="M75" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> meteorological archive is generated by
averaging the original GEOS-5 archive over the corresponding grid. As part of
this work, we developed a capability to conduct global GEOS-Chem simulations
for passive tracers at native 0.25<inline-formula><mml:math id="M76" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M77" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 0.3125<inline-formula><mml:math id="M78" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> horizontal
resolution. This allows us to separate the contributions of off-line
archiving and degraded resolution to model errors.</p>
</sec>
</sec>
<sec id="Ch1.S3">
  <label>3</label><title>Simulation ensemble</title>
<sec id="Ch1.S3.SS1">
  <label>3.1</label><?xmltex \opttitle{The ${}^{{222}}$Rn--${}^{{210}}$Pb--${}^{{7}}$Be system}?><title>The <inline-formula><mml:math id="M79" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">222</mml:mn></mml:msup></mml:math></inline-formula>Rn–<inline-formula><mml:math id="M80" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">210</mml:mn></mml:msup></mml:math></inline-formula>Pb–<inline-formula><mml:math id="M81" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">7</mml:mn></mml:msup></mml:math></inline-formula>Be system</title>
      <p id="d1e1155">The natural tracer suite <inline-formula><mml:math id="M82" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">222</mml:mn></mml:msup></mml:math></inline-formula>Rn–<inline-formula><mml:math id="M83" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">210</mml:mn></mml:msup></mml:math></inline-formula>Pb–<inline-formula><mml:math id="M84" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">7</mml:mn></mml:msup></mml:math></inline-formula>Be provides a
standard test of vertical transport and scavenging in global models, with
capability to compare to observations <xref ref-type="bibr" rid="bib1.bibx35" id="paren.40"/>. <inline-formula><mml:math id="M85" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">222</mml:mn></mml:msup></mml:math></inline-formula>Rn is
emitted ubiquitously by soils. Its sole sink is radioactive decay to
<inline-formula><mml:math id="M86" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">210</mml:mn></mml:msup></mml:math></inline-formula>Pb with a half-life of 3.8 days, making it a sensitive tracer for
vertical transport in the troposphere <xref ref-type="bibr" rid="bib1.bibx36 bib1.bibx24 bib1.bibx25 bib1.bibx1" id="paren.41"/>.
<inline-formula><mml:math id="M87" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">210</mml:mn></mml:msup></mml:math></inline-formula>Pb (half-life 22.3 years) attaches to aerosol particles
and provides a diagnostic for aerosol lifetime against deposition
<xref ref-type="bibr" rid="bib1.bibx4" id="paren.42"/>. <inline-formula><mml:math id="M88" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">7</mml:mn></mml:msup></mml:math></inline-formula>Be (half-life 53.3 days) is produced in the
upper troposphere and lower stratosphere from the interaction of cosmic rays
with atmospheric oxygen and nitrogen <xref ref-type="bibr" rid="bib1.bibx29" id="paren.43"/> and attaches to aerosol
particles and is removed by deposition in the same way as <inline-formula><mml:math id="M89" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">210</mml:mn></mml:msup></mml:math></inline-formula>Pb. The
high-altitude source of <inline-formula><mml:math id="M90" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">7</mml:mn></mml:msup></mml:math></inline-formula>Be complements <inline-formula><mml:math id="M91" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">210</mml:mn></mml:msup></mml:math></inline-formula>Pb by testing the
model representation of subsidence and stratosphere–troposphere exchange
<xref ref-type="bibr" rid="bib1.bibx27 bib1.bibx10" id="paren.44"/>.</p>
      <p id="d1e1265">Here we use the <inline-formula><mml:math id="M92" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">222</mml:mn></mml:msup></mml:math></inline-formula>Rn–<inline-formula><mml:math id="M93" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">210</mml:mn></mml:msup></mml:math></inline-formula>Pb–<inline-formula><mml:math id="M94" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">7</mml:mn></mml:msup></mml:math></inline-formula>Be simulation originally
developed for GEOS-Chem by <xref ref-type="bibr" rid="bib1.bibx35" id="normal.45"/>. <inline-formula><mml:math id="M95" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">222</mml:mn></mml:msup></mml:math></inline-formula>Rn is emitted uniformly
from land excluding ice at a rate of 1.0 atoms cm<inline-formula><mml:math id="M96" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> s<inline-formula><mml:math id="M97" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> under
nonfreezing conditions and 0.3 atoms cm<inline-formula><mml:math id="M98" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> s<inline-formula><mml:math id="M99" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> under freezing
conditions. The <inline-formula><mml:math id="M100" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">7</mml:mn></mml:msup></mml:math></inline-formula>Be source function depends only on altitude and
latitude. <inline-formula><mml:math id="M101" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">210</mml:mn></mml:msup></mml:math></inline-formula>Pb and <inline-formula><mml:math id="M102" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">7</mml:mn></mml:msup></mml:math></inline-formula>Be are removed by aerosol wet and dry
deposition, in addition to radioactive decay (negligible for <inline-formula><mml:math id="M103" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">210</mml:mn></mml:msup></mml:math></inline-formula>Pb).
Dry deposition is a minor sink. Wet deposition includes scavenging in
convective updrafts following the approach of <xref ref-type="bibr" rid="bib1.bibx4" id="text.46"/>, and
first-order in-cloud and below-cloud scavenging for anvil and large-scale
(grid-resolved) precipitation following the approach of <xref ref-type="bibr" rid="bib1.bibx19" id="text.47"/>.
Aerosol can be released below cloud if precipitation evaporates. The
scavenging parameterizations of <xref ref-type="bibr" rid="bib1.bibx35" id="text.48"/> are intended to be applicable
to GEOS-Chem at all resolutions because convective mass fluxes (from the
GEOS-5 archive) do not change with resolution and because first-order
rainout or washout assumes precipitating fractions of grid boxes that are set in
all cases by a fixed rate of conversion of cloud water to precipitation <xref ref-type="bibr" rid="bib1.bibx19" id="paren.49"/>.</p>
      <p id="d1e1405">A recent study by <xref ref-type="bibr" rid="bib1.bibx53" id="text.50"/> uses GEOS-Chem with an updated
<inline-formula><mml:math id="M104" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">222</mml:mn></mml:msup></mml:math></inline-formula>Rn source function to evaluate with observations worldwide. Here
our focus is not on comparison to observations but on the effect of CTM model
differences relative to a reference simulation. Since the averaging and remapping
of meteorological fields in the CTM represents a degradation of the
information from the reference simulation, we view for our purpose the
reference simulation as the “truth” against which the different CTM
simulations can be compared.</p>
</sec>
<sec id="Ch1.S3.SS2">
  <label>3.2</label><title>Simulations performed</title>
      <p id="d1e1428">We conducted a number of online and off-line
<inline-formula><mml:math id="M105" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">222</mml:mn></mml:msup></mml:math></inline-formula>Rn–<inline-formula><mml:math id="M106" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">210</mml:mn></mml:msup></mml:math></inline-formula>Pb–<inline-formula><mml:math id="M107" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">7</mml:mn></mml:msup></mml:math></inline-formula>Be simulations for different spatial
resolutions and configurations, as illustrated in Figure <xref ref-type="fig" rid="Ch1.F1"/>
and explained below. All simulations were conducted for 2 months starting
from zero concentrations on 1 June 2013. We report and compare monthly mean
results for July 2013 after a 1-month (June) spin-up. We limited the
analysis to 1 month because of computational and storage requirements for
the high-resolution simulations and with the expectation that 1 month in
Northern Hemisphere summer is a sufficient time window to diagnose systematic
differences in vertical tropospheric transport as revealed by the
<inline-formula><mml:math id="M108" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">222</mml:mn></mml:msup></mml:math></inline-formula>Rn–<inline-formula><mml:math id="M109" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">210</mml:mn></mml:msup></mml:math></inline-formula>Pb–<inline-formula><mml:math id="M110" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">7</mml:mn></mml:msup></mml:math></inline-formula>Be system. The zero initialization allows for
sensitive analysis of differences but implies that concentrations are not in
steady state and should not be compared to observations, in particular for
<inline-formula><mml:math id="M111" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">210</mml:mn></mml:msup></mml:math></inline-formula>Pb and <inline-formula><mml:math id="M112" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">7</mml:mn></mml:msup></mml:math></inline-formula>Be. For example, observed and steady-state GEOS-Chem
<inline-formula><mml:math id="M113" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">210</mml:mn></mml:msup></mml:math></inline-formula>Pb concentrations in the stratosphere are higher than in the
troposphere <xref ref-type="bibr" rid="bib1.bibx35" id="paren.51"/>, but in our simulations they are much lower.
Stratospheric concentrations of <inline-formula><mml:math id="M114" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">222</mml:mn></mml:msup></mml:math></inline-formula>Rn and <inline-formula><mml:math id="M115" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">210</mml:mn></mml:msup></mml:math></inline-formula>Pb should not be
compared across simulations since the injection of <inline-formula><mml:math id="M116" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">222</mml:mn></mml:msup></mml:math></inline-formula>Rn into the
stratosphere may be driven by sporadic deep convection <xref ref-type="bibr" rid="bib1.bibx31" id="paren.52"/>.
The stratosphere is not discussed in what follows.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F1" specific-use="star"><?xmltex \currentcnt{1}?><label>Figure 1</label><caption><p id="d1e1551">Ensemble of global <inline-formula><mml:math id="M117" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">222</mml:mn></mml:msup></mml:math></inline-formula>Rn–<inline-formula><mml:math id="M118" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">210</mml:mn></mml:msup></mml:math></inline-formula>Pb–<inline-formula><mml:math id="M119" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">7</mml:mn></mml:msup></mml:math></inline-formula>Be simulations
conducted in this work. The blue and green boxes identify simulations
originating from reference high-resolution (c360) and coarse-resolution (c48)
GEOS-5 meteorological products, respectively.</p></caption>
          <?xmltex \igopts{width=455.244094pt}?><graphic xlink:href="https://gmd.copernicus.org/articles/11/305/2018/gmd-11-305-2018-f01.pdf"/>

        </fig>

      <p id="d1e1587">Simulation 1 is conducted online using a version of GEOS-5 similar to the
one used in <xref ref-type="bibr" rid="bib1.bibx40" id="text.53"/> at c360 resolution. For <inline-formula><mml:math id="M120" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">222</mml:mn></mml:msup></mml:math></inline-formula>Rn, it
defines the reference simulation; all other simulations in
Fig. <xref ref-type="fig" rid="Ch1.F1"/> (blue boxes) successively degrade some aspect of
that reference simulation. This is not the case for <inline-formula><mml:math id="M121" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">210</mml:mn></mml:msup></mml:math></inline-formula>Pb and
<inline-formula><mml:math id="M122" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">7</mml:mn></mml:msup></mml:math></inline-formula>Be because the scheme for aerosol wet scavenging in the GEOS-5 GCM is
less advanced than in GEOS-Chem. In particular, aerosol scavenging in the<?pagebreak page309?> GCM
is not coupled to sub-grid transport in deep convective updrafts, and this can
severely overestimate the transport of aerosols to the upper troposphere
<xref ref-type="bibr" rid="bib1.bibx4" id="paren.54"/>. Thus we do not show <inline-formula><mml:math id="M123" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">210</mml:mn></mml:msup></mml:math></inline-formula>Pb and <inline-formula><mml:math id="M124" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">7</mml:mn></mml:msup></mml:math></inline-formula>Be results
from the online simulations.</p>
      <p id="d1e1645">Simulation 2 is also conducted online at c360 resolution but with the bulk
convective algorithm of GEOS-Chem and 3 h averaged convective mass fluxes
from simulation 1. This allows us to separately examine the effect of using
archived fields on convection and advection. Simulation 2 is used to generate
the meteorological archive (3 h for winds and convective mass fluxes, 1 h for
mixing depths) for the off-line GEOS-Chem simulations. This off-line archive
mimics the operational GEOS-FP archive by using the same temporal averaging
windows and remapping the cubed-sphere meteorological data to a
0.25<inline-formula><mml:math id="M125" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M126" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 0.3125<inline-formula><mml:math id="M127" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> rectilinear grid.</p>
      <p id="d1e1673">Simulation 3 is the standard off-line high-resolution GEOS-Chem on a
0.25<inline-formula><mml:math id="M128" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M129" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 0.3125<inline-formula><mml:math id="M130" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> rectilinear grid. It uses an archive of
winds, mixing depths, and convective mass fluxes generated from simulation 2
that mimics the GEOS-5 operational product. Errors in the <inline-formula><mml:math id="M131" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">222</mml:mn></mml:msup></mml:math></inline-formula>Rn
simulation compared to simulation 2 include the temporal averaging of winds
and mixing depths, the remapping of the meteorological archive to a
rectilinear grid, and the use of a lower-order advection core and a different
boundary layer mixing scheme. For <inline-formula><mml:math id="M132" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">210</mml:mn></mml:msup></mml:math></inline-formula>Pb and <inline-formula><mml:math id="M133" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">7</mml:mn></mml:msup></mml:math></inline-formula>Be, simulation 3
represents our best-case reference simulation.</p>
      <p id="d1e1729">Simulation 4 is the standard off-line coarse-resolution GEOS-Chem on a
2<inline-formula><mml:math id="M134" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M135" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 2.5<inline-formula><mml:math id="M136" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> grid. It uses the off-line meteorological
archive from simulation 2 but degraded to 2<inline-formula><mml:math id="M137" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M138" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 2.5<inline-formula><mml:math id="M139" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>
resolution. Comparison with simulation 3 shows the error from degraded
horizontal resolution. Comparison to simulation 1 (for <inline-formula><mml:math id="M140" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">222</mml:mn></mml:msup></mml:math></inline-formula>Rn) shows
the compounded errors in going from the original online GEOS-5 simulation to
the off-line, coarse-resolution simulation.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F2" specific-use="star"><?xmltex \currentcnt{2}?><label>Figure 2</label><caption><p id="d1e1794">Off-line transport errors in <inline-formula><mml:math id="M141" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">222</mml:mn></mml:msup></mml:math></inline-formula>Rn concentrations simulated at
c360 (<inline-formula><mml:math id="M142" display="inline"><mml:mo lspace="0mm">≈</mml:mo></mml:math></inline-formula> 25 km) resolution. <bold>(a)</bold> Zonal mean concentrations
of <inline-formula><mml:math id="M143" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">222</mml:mn></mml:msup></mml:math></inline-formula>Rn from the online GEOS-5 reference simulation with c360
cubed-sphere resolution (simulation 1). Values are monthly means for
July 2013 after a 1-month spin-up from zero concentrations and are expressed
in mixing ratio units of millibecquerels per standard cubic meter (at
0 <inline-formula><mml:math id="M144" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C and 1 atm pressure) or mBq SCM<inline-formula><mml:math id="M145" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>. <bold>(b)</bold> Errors due
to the use of simplified off-line GEOS-Chem convection shown as percentage
differences between simulation 2 and simulation 1. <bold>(c)</bold> Errors in the
high-resolution GEOS-Chem simulation at
0.25<inline-formula><mml:math id="M146" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M147" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 0.3125<inline-formula><mml:math id="M148" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> (<inline-formula><mml:math id="M149" display="inline"><mml:mo lspace="0mm">≈</mml:mo></mml:math></inline-formula> 25 km) resolution due
to off-line archiving of winds and mixing depths, remapping to rectilinear
grid, and use of different transport schemes shown as percentage differences
between simulation 3 and simulation 2. The abscissa is on a sine latitude
(equal area) scale. Stratospheric results are not shown (see text). Here and
in other figures, solid color contours provide finer gradation of the labeled
line contours.</p></caption>
          <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://gmd.copernicus.org/articles/11/305/2018/gmd-11-305-2018-f02.png"/>

        </fig>

      <p id="d1e1892">Although global GEOS-Chem simulations may be conducted at coarse
2<inline-formula><mml:math id="M150" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M151" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 2.5<inline-formula><mml:math id="M152" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> resolution, they use driving meteorological
fields generated from the original GEOS-5 simulation at c360
(<inline-formula><mml:math id="M153" display="inline"><mml:mo lspace="0mm">≈</mml:mo></mml:math></inline-formula> 0.25<inline-formula><mml:math id="M154" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M155" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 0.3125<inline-formula><mml:math id="M156" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>) resolution. This is an
important distinction from a simulation that would be driven by a coarser
meteorological model. To investigate that effect, we also conducted an
online simulation 5 using GEOS-5 meteorology at c48 resolution
(<inline-formula><mml:math id="M157" display="inline"><mml:mo lspace="0mm">≈</mml:mo></mml:math></inline-formula> 2<inline-formula><mml:math id="M158" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M159" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 2.5<inline-formula><mml:math id="M160" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>). We then used the meteorological data from
simulation 5, archived on the<?pagebreak page310?> cubed-sphere grid, to drive an off-line c48
simulation using the high-performance version of GEOS-Chem on that grid
(simulation 6) and an off-line 2<inline-formula><mml:math id="M161" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M162" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 2.5<inline-formula><mml:math id="M163" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> simulation using
the standard GEOS-Chem on a rectilinear grid (simulation 7). A comparison of
simulations 6 and 7 diagnoses the error from remapping the meteorological
archive from its native cubed-sphere to a rectilinear grid. Except for
temporal averaging, the off-line archive for simulation 6 is fully consistent
with the c48 online simulation 5 (no remapping). The c48 resolution allowed
us to conduct a cubed-sphere off-line (GCHP) simulation, which we were not
able to do at c360 resolution due to computational limitations.</p>
      <p id="d1e2012">Together, simulations 1–7 allow us to examine and isolate different sources
of error in simulations of chemical transport including meteorological grid
resolution, off-line meteorological archiving (temporal averaging), remapping
of the meteorological archive, spatial degradation of that archive, and
differences between off-line and online transport schemes. Salient results
are discussed in the next section. We use monthly average zonal mean profiles
vs. altitude and latitude as our comparison metric, following standard
practice for <inline-formula><mml:math id="M164" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">222</mml:mn></mml:msup></mml:math></inline-formula>Rn model intercomparisons <xref ref-type="bibr" rid="bib1.bibx25" id="paren.55"/>. Another
comparison metric for <inline-formula><mml:math id="M165" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">210</mml:mn></mml:msup></mml:math></inline-formula>Pb and <inline-formula><mml:math id="M166" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">7</mml:mn></mml:msup></mml:math></inline-formula>Be is the global tropospheric
lifetime against deposition <xref ref-type="bibr" rid="bib1.bibx35" id="paren.56"/>. Throughout this paper, we refer
to “archiving” as the temporal averaging of meteorological fields for use
in off-line simulations, “remapping” as the cubed-sphere to rectilinear
transformation of these fields, and “spatial averaging” as the further
degradation of these fields from a fine to a coarse off-line grid.</p>
</sec>
</sec>
<sec id="Ch1.S4">
  <label>4</label><title>Simulation results</title>
      <p id="d1e2057">Figure <xref ref-type="fig" rid="Ch1.F2"/>a shows the zonal July mean profile of
<inline-formula><mml:math id="M167" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">222</mml:mn></mml:msup></mml:math></inline-formula>Rn concentrations as a function of latitude and altitude from
simulation 1. The latitudinal distribution reflects the continental source.
The <inline-formula><mml:math id="M168" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">222</mml:mn></mml:msup></mml:math></inline-formula>Rn lifetime is much shorter than the vertical mixing time of
the troposphere (<inline-formula><mml:math id="M169" display="inline"><mml:mo lspace="0mm">∼</mml:mo></mml:math></inline-formula>1 month), resulting in strong vertical gradients. The
zonal mean concentration patterns are typical of those found in other models <xref ref-type="bibr" rid="bib1.bibx25" id="paren.57"/>.</p>
<sec id="Ch1.S4.SS1">
  <label>4.1</label><title>Errors from use of off-line convection scheme</title>
      <p id="d1e2097">Figure <xref ref-type="fig" rid="Ch1.F2"/>b shows the percentage differences
in zonal mean <inline-formula><mml:math id="M170" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">222</mml:mn></mml:msup></mml:math></inline-formula>Rn profiles between simulation 2 (off-line GEOS-Chem
convection scheme) and simulation 1. Simulation 2 has up to 10 % higher
<inline-formula><mml:math id="M171" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">222</mml:mn></mml:msup></mml:math></inline-formula>Rn concentrations in the equatorial lower troposphere and up to 7 %
lower <inline-formula><mml:math id="M172" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">222</mml:mn></mml:msup></mml:math></inline-formula>Rn concentrations in the middle to upper troposphere. The
combination of using the GEOS-Chem convection scheme and temporally
averaged convective mass fluxes results in slightly reduced vertical
transport compared to the original GEOS-5 convection.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F3" specific-use="star"><?xmltex \currentcnt{3}?><label>Figure 3</label><caption><p id="d1e2131">Off-line transport errors in <inline-formula><mml:math id="M173" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">222</mml:mn></mml:msup></mml:math></inline-formula>Rn concentrations simulated at
c48 (<inline-formula><mml:math id="M174" display="inline"><mml:mo lspace="0mm">≈</mml:mo></mml:math></inline-formula> 200 km) resolution. <bold>(a)</bold> Zonal monthly mean
concentrations of <inline-formula><mml:math id="M175" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">222</mml:mn></mml:msup></mml:math></inline-formula>Rn for July 2013 from the online GEOS-5 simulation
with c48 cubed-sphere resolution (simulation 5). <bold>(b)</bold> Errors due to
off-line archiving of meteorological fields (no remapping) shown as
percentage differences between simulation 6 and simulation 5.
<bold>(c)</bold> Errors due to remapping of the meteorological archive from c48
to 2<inline-formula><mml:math id="M176" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M177" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 2.5<inline-formula><mml:math id="M178" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> (rectilinear, <inline-formula><mml:math id="M179" display="inline"><mml:mo>≈</mml:mo></mml:math></inline-formula> 200 km) and
using a lower-order advection scheme shown as percentage differences
between simulation 7 and simulation 6.</p></caption>
          <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://gmd.copernicus.org/articles/11/305/2018/gmd-11-305-2018-f03.png"/>

        </fig>

      <p id="d1e2207">The GEOS-Chem convection scheme operates as a single convective plume in each
grid column on the basis of the 3 h archive of GEOS-5 convective updraft
and detrainment data. We find in a sensitivity simulation that using 15 min
or 3 h averages of convective mass fluxes makes no significant difference.
Thus the differences in Fig. <xref ref-type="fig" rid="Ch1.F2"/> arise mainly from the bulk
convective transport scheme used in GEOS-Chem, which simplifies the RAS
ensemble-plume parameterization to a single plume. One explanation for why a
multi-plume parameterization might produce a different transport pattern is
that each sequential plume acts on a different concentration<?pagebreak page311?> gradient that
has been modified by the previous plume until the moisture and temperature
fields are balanced. A tall plume followed by a series of short plumes will
transport more tracer higher than a series of shorter plumes followed by a tall plume.</p>
</sec>
<sec id="Ch1.S4.SS2">
  <label>4.2</label><title>Errors from off-line vs. online simulation</title>
      <p id="d1e2220">Figure <xref ref-type="fig" rid="Ch1.F2"/>c shows the percentage differences
between simulation 3 (off-line) and simulation 2 (online). The off-line
simulation has higher <inline-formula><mml:math id="M180" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">222</mml:mn></mml:msup></mml:math></inline-formula>Rn concentrations in the mid-troposphere
(700–500 hPa) and lower concentrations in the upper troposphere (above
500 hPa), with some differences exceeding 20 %. Encapsulated in this comparison
are the effects of remapping the archived meteorological fields to
a rectilinear grid using a different advection scheme, using a different
boundary layer mixing scheme, and using 3 h averaged wind fields. Large
relative differences in polar grid cells may reflect the averaging of
concentrations in the polar latitudes in the rectilinear advection scheme
<xref ref-type="bibr" rid="bib1.bibx34" id="paren.58"/> and the transition to semi-Lagrangian advection
when the Courant number exceeds unity. <inline-formula><mml:math id="M181" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">222</mml:mn></mml:msup></mml:math></inline-formula>Rn concentrations are very
low in these polar grid cells so that absolute differences are small.</p>
      <p id="d1e2246">To better understand the contributions from different sources of error in the
off-line simulation, we examine simulations 5–7, which show a similar
transition from online to off-line, but starting at c48 resolution in the
GEOS-5 model and with the intermediate addition of a c48 off-line GCHP
simulation (custom cubed-sphere archive, no remapping). In this way we can
diagnose the effects of using archived meteorology separately from the
effects of the advection core and remapping error associated with conversion
to a rectilinear (here 2<inline-formula><mml:math id="M182" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M183" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 2.5<inline-formula><mml:math id="M184" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>) grid. Figure <xref ref-type="fig" rid="Ch1.F3"/>a shows the zonal mean <inline-formula><mml:math id="M185" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">222</mml:mn></mml:msup></mml:math></inline-formula>Rn concentrations for
c48 resolution, which have a similar pattern to the c360 results. Figure <xref ref-type="fig" rid="Ch1.F3"/>b and c additively separate out the
contributions from off-line archiving (simulation 6 vs. simulation 5) and
the remapping and transport scheme (simulation 7 vs. simulation 6). Off-line
archiving results in overall weaker vertical transport, as might be expected
from transient motions averaged out in the meteorological archive. The bias
is about 5 % in surface air but can exceed 20 % in the upper troposphere.
There is still a bias over Antarctica even though the off-line cubed-sphere
geometry does not have a polar singularity; this may reflect the cumulative
effect of meridional transport differences affecting a region particularly
remote from sources. The combination of remapping to the rectilinear grid and
using the <xref ref-type="bibr" rid="bib1.bibx34" id="text.59"/> advection scheme (right panel) also incurs
differences of about 5 % in surface air and up to 20 % in the upper
troposphere. We would expect to see larger remapping errors associated with
smaller grids, especially over the polar regions. The errors from simulations 6
and 7 compound for surface air but tend to cancel in the upper troposphere.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F4"><?xmltex \currentcnt{4}?><label>Figure 4</label><caption><p id="d1e2293">Effect of grid resolution on simulated zonal mean <inline-formula><mml:math id="M186" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">222</mml:mn></mml:msup></mml:math></inline-formula>Rn
concentrations for July 2013. <bold>(a)</bold> Percentage differences between
online GEOS-5 simulations at c48 resolution (simulation 5) and c360
resolution (simulation 2). <bold>(b)</bold> Percentage differences between
off-line GEOS-Chem simulations at 2<inline-formula><mml:math id="M187" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M188" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 2.5<inline-formula><mml:math id="M189" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>
resolution (simulation 4) and 0.25<inline-formula><mml:math id="M190" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M191" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 0.3125<inline-formula><mml:math id="M192" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>
resolution (simulation 3).</p></caption>
          <?xmltex \igopts{width=236.157874pt}?><graphic xlink:href="https://gmd.copernicus.org/articles/11/305/2018/gmd-11-305-2018-f04.png"/>

        </fig>

</sec>
<sec id="Ch1.S4.SS3">
  <label>4.3</label><title>Errors from grid resolution</title>
      <p id="d1e2376">Figure <xref ref-type="fig" rid="Ch1.F4"/> shows the effect of grid resolution on zonal mean
<inline-formula><mml:math id="M193" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">222</mml:mn></mml:msup></mml:math></inline-formula>Rn profiles in GEOS-5 (online, with resolution affecting
meteorology) and GEOS-Chem (off-line, using the same meteorological archive
in both cases). Figure 4b shows the percentage difference between
simulation 5 (online c48) and simulation 2 (online c360). The c360
meteorological simulation has sufficient spatial resolution to resolve large
convective systems and thus has much less parameterized convection than the
c48 simulation. The higher <inline-formula><mml:math id="M194" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">222</mml:mn></mml:msup></mml:math></inline-formula>Rn concentrations in the tropical upper
troposphere in c48 and lower concentrations in the extratropical upper
troposphere most likely reflect differences in vertical transport
properties between the resolved and parameterized convective formulations.
Thus the higher concentrations in the tropical middle to upper troposphere at c48
can be attributed to the<?pagebreak page312?> convective fluxes that are not represented by the
resolved transport at c360. The lower concentrations near the tropopause can
be attributed to the known insufficiency of convective transport for reaching
that level <xref ref-type="bibr" rid="bib1.bibx43" id="paren.60"/>. The lower concentrations in the extratropical
upper troposphere may be due to inability to diagnose organized vertical
motion as convection. The higher concentrations over Antarctica at c48 may be
due to numerical diffusion during the slow long-range meridional transport
from lower latitudes <xref ref-type="bibr" rid="bib1.bibx15" id="paren.61"/>. While these differences are large,
absolute concentrations are very low over the poles due to the short lifetime
of <inline-formula><mml:math id="M195" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">222</mml:mn></mml:msup></mml:math></inline-formula>Rn and lack of emission over ice and snow.</p>
      <p id="d1e2415">Degrading model resolution has different effects in GEOS-Chem,
in which the coarse 2<inline-formula><mml:math id="M196" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M197" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 2.5<inline-formula><mml:math id="M198" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> simulation uses the same
0.25<inline-formula><mml:math id="M199" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M200" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 0.3125<inline-formula><mml:math id="M201" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> meteorological archive as the
high-resolution simulation but with spatial averaging of the meteorological
fields. The coarse simulation results in decreased vertical transport to the
upper troposphere at all latitudes, with maximum effect (up to 40 %) in the
subsiding subtropics. This may be simply explained by the averaging out of
vertical eddy motions on the coarser grid, including organized vertical
motions across multiple levels that the online c48 simulation would simulate
with stronger parameterized convection. This systematic bias in the
coarse-resolution GEOS-Chem may thus be correctable through the addition of
convective motions. We explore this idea in the next section.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F5"><?xmltex \currentcnt{5}?><label>Figure 5</label><caption><p id="d1e2471">Simulated GEOS-Chem zonal mean concentrations of <inline-formula><mml:math id="M202" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">210</mml:mn></mml:msup></mml:math></inline-formula>Pb and
<inline-formula><mml:math id="M203" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">7</mml:mn></mml:msup></mml:math></inline-formula>Be at 0.25<inline-formula><mml:math id="M204" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M205" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 0.3125<inline-formula><mml:math id="M206" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> grid resolution
(simulation 3; <bold>a, b</bold>) and the effect of degrading grid resolution to
2<inline-formula><mml:math id="M207" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M208" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 2.5<inline-formula><mml:math id="M209" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> (simulation 4; <bold>c, d</bold>).
Concentrations are monthly means for July 2013 after a 1-month spin-up from
zero concentrations and are expressed in mixing ratio units of millibecquerels per standard cubic meter (at 0 <inline-formula><mml:math id="M210" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C and 1 atm pressure) or
mBq SCM<inline-formula><mml:math id="M211" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>. <bold>(c, d)</bold> Percentage differences between
simulation 4 and simulation 3.</p></caption>
          <?xmltex \igopts{width=236.157874pt}?><graphic xlink:href="https://gmd.copernicus.org/articles/11/305/2018/gmd-11-305-2018-f05.png"/>

        </fig>

</sec>
<sec id="Ch1.S4.SS4">
  <label>4.4</label><?xmltex \opttitle{Errors from grid resolution for ${}^{{210}}$Pb and ${}^{{7}}$Be}?><title>Errors from grid resolution for <inline-formula><mml:math id="M212" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">210</mml:mn></mml:msup></mml:math></inline-formula>Pb and <inline-formula><mml:math id="M213" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">7</mml:mn></mml:msup></mml:math></inline-formula>Be</title>
      <p id="d1e2608">Figure <xref ref-type="fig" rid="Ch1.F5"/> (top panels) shows the zonal mean concentrations of
<inline-formula><mml:math id="M214" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">210</mml:mn></mml:msup></mml:math></inline-formula>Pb and <inline-formula><mml:math id="M215" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">7</mml:mn></mml:msup></mml:math></inline-formula>Be from the GEOS-Chem simulation at
0.25<inline-formula><mml:math id="M216" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M217" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 0.3125<inline-formula><mml:math id="M218" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> (simulation 3). The <inline-formula><mml:math id="M219" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">210</mml:mn></mml:msup></mml:math></inline-formula>Pb
distribution is shifted to higher altitudes relative to <inline-formula><mml:math id="M220" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">222</mml:mn></mml:msup></mml:math></inline-formula>Rn,
reflecting the effect of scavenging in the lower troposphere. <inline-formula><mml:math id="M221" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">7</mml:mn></mml:msup></mml:math></inline-formula>Be shows
preferential subsidence in the dry subtropics and is depleted in the lower
troposphere by scavenging. <inline-formula><mml:math id="M222" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">7</mml:mn></mml:msup></mml:math></inline-formula>Be concentrations are low throughout the
tropical troposphere due to dominant upwelling of <inline-formula><mml:math id="M223" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">7</mml:mn></mml:msup></mml:math></inline-formula>Be-depleted surface air.</p>
      <p id="d1e2702">Mean tropospheric lifetimes against deposition in the
0.25<inline-formula><mml:math id="M224" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M225" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 0.3125<inline-formula><mml:math id="M226" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> simulation are 6.7 days for <inline-formula><mml:math id="M227" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">210</mml:mn></mml:msup></mml:math></inline-formula>Pb
and 17 days for <inline-formula><mml:math id="M228" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">7</mml:mn></mml:msup></mml:math></inline-formula>Be. <xref ref-type="bibr" rid="bib1.bibx35" id="text.62"/> previously inferred <inline-formula><mml:math id="M229" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">210</mml:mn></mml:msup></mml:math></inline-formula>Pb and
<inline-formula><mml:math id="M230" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">7</mml:mn></mml:msup></mml:math></inline-formula>Be tropospheric residence times of 9 and 21 days, respectively, from an
earlier version of GEOS-Chem evaluated with observations. A more recent
evaluation by <xref ref-type="bibr" rid="bib1.bibx53" id="text.63"/> using GEOS-Chem version 11-01 and an
updated <inline-formula><mml:math id="M231" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">222</mml:mn></mml:msup></mml:math></inline-formula>Rn source finds that a residence time for <inline-formula><mml:math id="M232" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">210</mml:mn></mml:msup></mml:math></inline-formula>Pb of
7 <inline-formula><mml:math id="M233" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 1 days better matches the observational constraints.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F6" specific-use="star"><?xmltex \currentcnt{6}?><label>Figure 6</label><caption><p id="d1e2801">Errors in off-line coarse-resolution
(2<inline-formula><mml:math id="M234" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M235" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 2.5<inline-formula><mml:math id="M236" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>) simulations of <inline-formula><mml:math id="M237" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">222</mml:mn></mml:msup></mml:math></inline-formula>Rn concentrations
relative to the reference online c360 GEOS-5 simulation (simulation 1).
Values are percentage differences in zonal mean concentrations for July 2013.
<bold>(a)</bold> Errors for the baseline 2<inline-formula><mml:math id="M238" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M239" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 2.5<inline-formula><mml:math id="M240" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>
GEOS-Chem simulation. <bold>(b)</bold> Errors for the same baseline but
with adjusted RAS convective mass fluxes (see text). <bold>(c)</bold> Errors for the same baseline with adjusted RAS convective mass fluxes and
maximum mixing depths for each coarse-resolution grid cell
(cf. Fig.  <xref ref-type="fig" rid="Ch1.F9"/>).</p></caption>
          <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://gmd.copernicus.org/articles/11/305/2018/gmd-11-305-2018-f06.png"/>

        </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F7" specific-use="star"><?xmltex \currentcnt{7}?><label>Figure 7</label><caption><p id="d1e2884"><inline-formula><mml:math id="M241" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">222</mml:mn></mml:msup></mml:math></inline-formula>Rn concentrations at 900 hPa <bold>(a–c)</bold> and
500 hPa <bold>(d–f)</bold> from the reference online c360 GEOS-5 simulation
(simulation 1; <bold>a, d</bold>) and off-line 2<inline-formula><mml:math id="M242" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M243" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 2.5<inline-formula><mml:math id="M244" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>
GEOS-Chem simulation (simulation 4; <bold>b, e</bold>). <bold>(c, f)</bold> The
percent difference in <inline-formula><mml:math id="M245" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">222</mml:mn></mml:msup></mml:math></inline-formula>Rn concentrations in simulation 4 relative to
simulation 1.</p></caption>
          <?xmltex \igopts{width=497.923228pt}?><graphic xlink:href="https://gmd.copernicus.org/articles/11/305/2018/gmd-11-305-2018-f07.png"/>

        </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F8" specific-use="star"><?xmltex \currentcnt{8}?><label>Figure 8</label><caption><p id="d1e2953">Convective mass fluxes for July 2013 produced by the GEOS-5 GCM at
cubed-sphere c360 (<inline-formula><mml:math id="M246" display="inline"><mml:mo lspace="0mm">≈</mml:mo></mml:math></inline-formula> 25 km) and c48 (<inline-formula><mml:math id="M247" display="inline"><mml:mo lspace="0mm">≈</mml:mo></mml:math></inline-formula> 200 km) resolution
using the Relaxed Arakawa–Schubert (RAS) scheme and by the
2<inline-formula><mml:math id="M248" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M249" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 2.5<inline-formula><mml:math id="M250" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> (<inline-formula><mml:math id="M251" display="inline"><mml:mo lspace="0mm">≈</mml:mo></mml:math></inline-formula> 200 km) GEOS-Chem simulation
using the RAS scheme with c360 and c48 GEOS-5 meteorology.
<bold>(a)</bold> Vertical profile of global mean convective mass flux.
<bold>(b)</bold> Zonal mean convective mass flux at 500 hPa as a function of
latitude.</p></caption>
          <?xmltex \igopts{width=284.527559pt}?><graphic xlink:href="https://gmd.copernicus.org/articles/11/305/2018/gmd-11-305-2018-f08.pdf"/>

        </fig>

      <p id="d1e3015">The bottom panels show the effects of degrading the GEOS-Chem resolution to
2<inline-formula><mml:math id="M252" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M253" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 2.5<inline-formula><mml:math id="M254" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>. Overall the results are consistent with our
previous finding for <inline-formula><mml:math id="M255" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">222</mml:mn></mml:msup></mml:math></inline-formula>Rn that degrading the resolution weakens
vertical transport. Tropospheric lifetimes decrease to 6.2 days for
<inline-formula><mml:math id="M256" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">210</mml:mn></mml:msup></mml:math></inline-formula>Pb and increase to 18 days for <inline-formula><mml:math id="M257" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">7</mml:mn></mml:msup></mml:math></inline-formula>Be, with is consistent with the shifts
in vertical distribution to the lower troposphere for <inline-formula><mml:math id="M258" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">210</mml:mn></mml:msup></mml:math></inline-formula>Pb and to the
upper troposphere for <inline-formula><mml:math id="M259" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">7</mml:mn></mml:msup></mml:math></inline-formula>Be. <inline-formula><mml:math id="M260" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">210</mml:mn></mml:msup></mml:math></inline-formula>Pb concentrations are higher in the
tropical upper troposphere in the 2<inline-formula><mml:math id="M261" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M262" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 2.5<inline-formula><mml:math id="M263" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> simulation,
likely due to differences in wet scavenging.</p><?xmltex \hack{\newpage}?>
</sec>
</sec>
<?pagebreak page313?><sec id="Ch1.S5">
  <label>5</label><title>Correcting errors in off-line simulations</title>
      <p id="d1e3135">Our work has shown how a cascade of errors is introduced in the model transport
of chemical tracers when using off-line meteorological archives (as opposed
to online simulation) and when degrading the spatial resolution of these
archives for computational expediency. The compounding effect is illustrated
in Fig. <xref ref-type="fig" rid="Ch1.F6"/>a, which compares the zonal mean
<inline-formula><mml:math id="M264" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">222</mml:mn></mml:msup></mml:math></inline-formula>Rn concentration profiles in the off-line
2<inline-formula><mml:math id="M265" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M266" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 2.5<inline-formula><mml:math id="M267" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> configuration of GEOS-Chem to the online GEOS-5
simulation at c360 (<inline-formula><mml:math id="M268" display="inline"><mml:mo lspace="0mm">≈</mml:mo></mml:math></inline-formula> 25 km) resolution. Concentrations are typically
biased high by <inline-formula><mml:math id="M269" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 20 % at the surface and biased low by <inline-formula><mml:math id="M270" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 40 % in the upper
troposphere. Figure <xref ref-type="fig" rid="Ch1.F7"/> shows the same comparison as Fig. <xref ref-type="fig" rid="Ch1.F6"/>a but for concentrations at 900 and 500 hPa.
We see that the c360 simulation is better able to capture the filamentary
structure of outflow from continental source regions, while these patterns are
not apparent in the 2<inline-formula><mml:math id="M271" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M272" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 2.5<inline-formula><mml:math id="M273" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> simulation. Concentrations
are higher overall for the 2<inline-formula><mml:math id="M274" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M275" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 2.5<inline-formula><mml:math id="M276" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> simulation at 900 hPa
and lower at 500 hPa, which is consistent with the vertical profiles. At 500 hPa, the
fine structure of transport is even more apparent in the high-resolution
simulation. We now examine how some of these errors can be alleviated.</p>
      <p id="d1e3251">We can categorize the errors as resulting from four different sources:
(1) differences in transport algorithms between the off-line and online model
(advection scheme, boundary<?pagebreak page314?> layer mixing, convective parameterization);
(2) remapping of the meteorological archive (as here from a cubed-sphere to a
rectilinear grid); (3) temporal averaging in the meteorological archive
(causing loss of eddy motions, including grid-resolved organized convection,
and requiring a pressure fixer to correct horizontal winds); and (4) spatial
degradation of the meteorological archive (causing further loss of eddy
motions). Our work presented in Sect. 4 shows that all of these general
sources of error are important, and addressing some of them requires
improvement of the off-line archive. For example, an obvious improvement in
our case would be for the GEOS-5 meteorological archive to be available on
the native cubed-sphere grid rather than remapped to a rectilinear grid.
Increasing the temporal frequency of archiving would be another obvious improvement.</p>
      <p id="d1e3254">Here we examine the feasibility of restoring the organized vertical motions
lost in the temporal averaging of the meteorological archive or in the
spatial averaging for coarse-resolution GEOS-Chem simulations.
<xref ref-type="bibr" rid="bib1.bibx7" id="normal.64"/> previously found that vertical motions in a
large-eddy simulation at 200–200 m resolution could be preserved at coarser
resolution by an eddy accumulation method in which upward and downward vertical
winds are averaged separately. We implemented this method by taking the
archived pressure velocity (<inline-formula><mml:math id="M277" display="inline"><mml:mi mathvariant="italic">ω</mml:mi></mml:math></inline-formula>) as 3 h averages from the native
0.25<inline-formula><mml:math id="M278" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M279" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 0.3125<inline-formula><mml:math id="M280" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> meteorological archive and separately
averaging the upwards and downwards values onto the coarse-resolution
2<inline-formula><mml:math id="M281" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M282" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 2.5<inline-formula><mml:math id="M283" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> grid. We then compared these values to the value
computed by GEOS-Chem on the 2<inline-formula><mml:math id="M284" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M285" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 2.5<inline-formula><mml:math id="M286" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> grid, took the
difference as the component of vertical advection lost due to spatial
degradation, and applied this difference as a vertical mass exchange velocity
(i.e., eddy diffusion) between adjacent cells. We found that this made
negligible change to the <inline-formula><mml:math id="M287" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">222</mml:mn></mml:msup></mml:math></inline-formula>Rn simulation, implying that the transport
error on our scales is due more to loss of organized convective motion than
to loss of small-scale eddies.</p>
      <p id="d1e3353"><?xmltex \hack{\newpage}?>Figure <xref ref-type="fig" rid="Ch1.F8"/> shows the mean July 2013 convective mass fluxes from
the c360 and c48 GEOS-5 simulations globally as vertical profiles (panel a) and at 500 hPa as a function of
latitude (panel b). Convective
mass fluxes are highest just above cloud base in the lower troposphere and
highest in the northern tropics (ITCZ). The global convective mass flux is
24 % weaker in the c360 than in the c48 simulation. In the c360 simulation,
parameterized convection is less needed because the organized convective
motions are partly resolved. Similar to the eddy motions, much of this
resolved convective motion is lost when winds produced by a high-resolution
GCM are first temporally averaged in a 3 h archive and then spatially averaged
to a coarse grid.</p>
      <p id="d1e3360">A possible way to compensate for this lost convective motion in the
meteorological archive is to increase parameterized convection in the
off-line CTM. A simple approach would be to increase the archived convective
mass fluxes by an adjustable factor, but this assumes that the archived
fluxes are colocated with the lost convection. A more physical approach is
to recompute the convective mass fluxes on the fly in the off-line CTM
simulation by using the same convective parameterization (here RAS) as in the
parent GCM and applied to the meteorological archive with the scale-aware
settings configured for the CTM resolution. This approach incurs little
additional computational cost because computations associated with the
hydrological cycle in RAS are not performed. It may still underestimate the
GCM convection because the archived meteorological fields used by the CTM
are convectively relaxed temporal averages, but this can be corrected by
adjusting the convective parameterization settings.</p>
      <p id="d1e3363">We implemented the GEOS-5 RAS scheme within GEOS-Chem in lieu of the archived
convective mass fluxes, taking as input water vapor, temperature, mixing
depth, and surface pressure fields from the archived meteorological data. The
RAS scheme outputs the convective air mass flux and<?pagebreak page315?> detrainment flux at every
dynamic time step. We then used these fluxes to drive convective transport in
GEOS-Chem, retaining the GEOS-Chem convective algorithm for consistent
treatment of scavenging. Off-line 2<inline-formula><mml:math id="M288" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M289" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 2.5<inline-formula><mml:math id="M290" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> GEOS-Chem
simulations were conducted in this manner using both c360 and c48 meteorological fields.</p>
      <p id="d1e3391">Figure <xref ref-type="fig" rid="Ch1.F8"/> shows the resulting global mean convective mass fluxes
produced by GEOS-Chem at 2<inline-formula><mml:math id="M291" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M292" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 2.5<inline-formula><mml:math id="M293" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> resolution using RAS to
compute the convective mass flux based on archived meteorological data from
the c360 and c48 meteorological archives. The vertical and latitudinal
distributions closely match those computed in GEOS-5 (simulations 1 and 5,
respectively). With c360 meteorology, the RAS-computed convective mass fluxes
in GEOS-Chem are 30 % higher globally than in GEOS-5 at that resolution
(solid and dashed red lines), responding as desired to the scale-aware
settings corresponding to the coarser resolution of the CTM. With c48
meteorology, the RAS-computed convective mass fluxes in GEOS-Chem are 35 %
weaker globally than in GEOS-5 (solid and dashed blue lines); here the CTM
has the same spatial resolution as the GCM, and the weaker convection is
expected from temporal averaging of the meteorological archive as discussed
above. The larger difference between GEOS-5 and GEOS-Chem convective mass
fluxes below 500 hPa compared to above 500 hPa suggests that convective
motions penetrating higher altitudes are more likely to be retained after
temporal averaging.</p>
      <p id="d1e3421">We can increase convection produced by RAS by applying a temperature
perturbation at the surface. On the scale of global CTMs (hundreds of kilometers),
there is substantial sub-grid variability in moisture and temperature, with
convection occurring preferentially over the more buoyant parts of the grid
cell. Using moisture and temperature fields averaged over these large grid
cells and over time will result in RAS underestimating convection.
Therefore, we add a temperature perturbation proportional to the vertical
temperature gradient at the surface (applied only when surface temperature is
greater than air temperature) to generate increased thermodynamic
instability, an approach that is also used in the GEOS-5 GCM operating at
coarse resolutions. We set a limit of 3.0 K as the maximum allowable
temperature perturbation. This leads to convective mass fluxes that are
2.5 times as much as the archived values.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F9"><?xmltex \currentcnt{9}?><label>Figure 9</label><caption><p id="d1e3426">Effect of averaging high-resolution mixing depths in
coarse-resolution simulations. <bold>(a)</bold> Mixing at high grid
resolution; the vertical extents of the boxes denote mixing depths and
the dashed arrows illustrate the mixing. Red arrows show the induced
circulation for a chemical tracer emitted at the surface.
<bold>(b, c)</bold> Mixing at coarse resolution with mixing depth
taken as the average or the maximum of the high-resolution
values.</p></caption>
        <?xmltex \igopts{width=236.157874pt}?><graphic xlink:href="https://gmd.copernicus.org/articles/11/305/2018/gmd-11-305-2018-f09.pdf"/>

      </fig>

      <p id="d1e3442">Figure <xref ref-type="fig" rid="Ch1.F6"/>b shows the effect of including RAS
in GEOS-Chem at 2<inline-formula><mml:math id="M294" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M295" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 2.5<inline-formula><mml:math id="M296" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> resolution using c360
meteorology. There is substantial improvement in the tropics relative to the
standard GEOS-Chem simulation using archived convective mass fluxes (panel a). Extratropical regions show less improvement, as vertical transport is
driven more by baroclinic instability rather than convection.</p>
      <p id="d1e3472">We further investigated whether spatial averaging of boundary layer mixing
depths from the high-resolution meteorological archive could weaken vertical
transport in coarse-resolution off-line simulations. As shown by the diagram
in Fig. <xref ref-type="fig" rid="Ch1.F9"/>, spatial averaging of mixing depths prevents boundary
layer mixing to higher altitudes that would otherwise take place in part of
the domain. This mixing would then drive a circulation ventilating a larger
fraction of the domain to higher altitudes than specified by the average
mixing depth. To assess the potential magnitude of this effect, we conducted
a sensitivity simulation using the maximum 0.25<inline-formula><mml:math id="M297" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M298" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 0.3125<inline-formula><mml:math id="M299" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>
mixing depth within a 2<inline-formula><mml:math id="M300" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M301" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 2.5<inline-formula><mml:math id="M302" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> grid cell as the mixing
depth for that grid cell. These mixing depths are used in place of the mean
mixing depths in boundary layer mixing and in RAS. The result is shown in Fig. <xref ref-type="fig" rid="Ch1.F6"/>c. The simulation of surface concentrations
is improved although there is overcompensation in the middle troposphere.</p>
</sec>
<sec id="Ch1.S6" sec-type="conclusions">
  <label>6</label><title>Conclusions</title>
      <p id="d1e3538">In this work, we isolated the different sources of transport errors resulting
from performing off-line chemical transport model (CTM) simulations with
archived meteorological data from a general circulation model (GCM). Errors
include temporal averaging and remapping of the meteorological archive,
differences in transport algorithms (sometimes required by lack of
information in the archive), and coarsening of the CTM grid to enable
simulations with a large number of chemically coupled species. We then
explored some possibilities for reducing these errors.</p>
      <p id="d1e3541">We used as a reference an online simulation of the
<inline-formula><mml:math id="M303" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">222</mml:mn></mml:msup></mml:math></inline-formula>Rn–<inline-formula><mml:math id="M304" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">210</mml:mn></mml:msup></mml:math></inline-formula>Pb–<inline-formula><mml:math id="M305" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">7</mml:mn></mml:msup></mml:math></inline-formula>Be chemical tracer suite in the Goddard Earth
Observing System (GEOS-5) GCM at cubed-sphere c360 (<inline-formula><mml:math id="M306" display="inline"><mml:mo lspace="0mm">≈</mml:mo></mml:math></inline-formula> 25 km)
resolution. The operational meteorological archive from GEOS-5, stored as 3 h
averages (1 h for mixing depths) and remapped onto a
0.25<inline-formula><mml:math id="M307" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M308" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 0.3125<inline-formula><mml:math id="M309" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> (<inline-formula><mml:math id="M310" display="inline"><mml:mo lspace="0mm">≈</mml:mo></mml:math></inline-formula> 25 km) rectilinear grid,
provides the standard input to the GEOS-Chem CTM used by a large research
community for atmospheric chemistry applications. These applications often
degrade the meteorological archive to 2<inline-formula><mml:math id="M311" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M312" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 2.5<inline-formula><mml:math id="M313" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>
(<inline-formula><mml:math id="M314" display="inline"><mml:mo lspace="0mm">≈</mml:mo></mml:math></inline-formula> 200 km) horizontal resolution (coarse-resolution GEOS-Chem) to make
global chemical simulations computationally tractable. We conducted an
ensemble of simulations to document the cascade of errors involved in going
from the online GEOS-5<?pagebreak page316?> high-resolution simulation to the off-line GEOS-Chem
coarse-resolution simulation. Although our study focuses on a particular
GCM–CTM combination, our findings have relevance for any CTM driven by
meteorology produced at high resolution. Vertical transport errors are of
particular interest and the <inline-formula><mml:math id="M315" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">222</mml:mn></mml:msup></mml:math></inline-formula>Rn–<inline-formula><mml:math id="M316" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">210</mml:mn></mml:msup></mml:math></inline-formula>Pb–<inline-formula><mml:math id="M317" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">7</mml:mn></mml:msup></mml:math></inline-formula>Be tracer suite
is well suited for that purpose.</p>
      <p id="d1e3671">We first diagnosed the cascade of transport errors in the <inline-formula><mml:math id="M318" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">222</mml:mn></mml:msup></mml:math></inline-formula>Rn
simulation when going from the online c360 GEOS-5 simulation to the off-line
0.25<inline-formula><mml:math id="M319" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M320" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 0.3125<inline-formula><mml:math id="M321" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> GEOS-Chem simulation. The error from using
temporally averaged convective mass fluxes is relatively small. The errors
from using archived winds and from remapping c360 fields to
0.25<inline-formula><mml:math id="M322" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M323" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 0.3125<inline-formula><mml:math id="M324" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> are both more severe, resulting together
in 5–20 % biases. Transport from the boundary layer to the upper troposphere
is too weak in the off-line model and this is due at least in part to loss of
transient organized advective motions (resolved convection) in the 3 h
averaging of the meteorological archive.</p>
      <p id="d1e3734">We then examined the effect of degrading the spatial resolution of the
meteorological archive from 0.25<inline-formula><mml:math id="M325" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M326" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 0.3125<inline-formula><mml:math id="M327" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> to
2<inline-formula><mml:math id="M328" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M329" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 2.5<inline-formula><mml:math id="M330" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> for input to the coarse-resolution GEOS-Chem.
This further weakened vertical transport by up to 40 % as organized vertical
motions in the 0.25<inline-formula><mml:math id="M331" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M332" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 0.3125<inline-formula><mml:math id="M333" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> archive were averaged out
in the 2<inline-formula><mml:math id="M334" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M335" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 2.5<inline-formula><mml:math id="M336" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> archive. The weakened vertical transport
also affected the lifetimes of <inline-formula><mml:math id="M337" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">210</mml:mn></mml:msup></mml:math></inline-formula>Pb and <inline-formula><mml:math id="M338" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">7</mml:mn></mml:msup></mml:math></inline-formula>Be by 5–10 % against deposition.</p>
      <p id="d1e3858">We explored different possibilities for restoring vertical transport in the
off-line coarse-resolution simulation. Archiving eddy vertical winds between
adjacent vertical layers was found to be of negligible benefit, indicating
that the loss of nonlocal organized vertical motions is more important.
The spatial averaging of boundary layer mixing depths leads to underestimates of
vertical transport, and this can be corrected by weighting the averaging
towards higher values. We showed that the loss of vertical organized
convective motions could be corrected to some extent by using the online GCM
convection scheme (here the Relaxed Arakawa–Schubert or RAS) to operate at
the coarse resolution of the CTM using the meteorological archive as input.
This improves vertical transport in the tropics but has little effect at
higher latitudes.</p>
      <p id="d1e3861">Our work has revealed significant vertical transport errors in off-line CTM
applications when using meteorological archives from a GCM operating at high
resolution. Given these large differences in vertical transport, users
examining the effect of convection on a chemical species should take care to
perform their simulations at sufficiently high resolution. Those conducting
simulations of long-lived trace gases such as CO<inline-formula><mml:math id="M339" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> or CH<inline-formula><mml:math id="M340" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> should
also be aware of these errors.</p>
      <p id="d1e3882">As the resolution of the GCMs continues to increase, the amount of transport information
lost in off-line CTMs will also increase. This may be corrected, in order of
priority, by (1) applying scale-dependent convective transport
parameterizations off-line, (2) avoiding remapping of the archive by archiving
on the cubed-sphere grid, (3) using consistent transport algorithms (in the
case of GEOS-Chem, Putman and Lin, 2010, rather than Lin and Rood, 1996), and
(4) increasing the frequency of archiving. Of the list, (1) will only require a
minor increase in computational time, (2) and (4) will increase both data
storage and computational resources, and (3) will require no additional
resources if (2) is done. These improvements will benefit off-line simulations
at all resolutions, including high-resolution nested simulations. We plan to
include these improvements in future versions of the standard GEOS-Chem code.</p>
</sec>

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

      <p id="d1e3889">The GEOS-Chem source code is freely available to the public.
Source code may be downloaded by following the instructions found at
<uri>http://wiki.geos-chem.org/</uri>. At the time of writing, this work used a
modified version of GEOS-Chem version 11-01 (the most recent public release)
as indicated in the text. All developments presented here will be included in
the next public release (version 11-02) of GEOS-Chem
(<uri>http://wiki.seas.harvard.edu/geos-chem/index.php/GEOS-Chem_v11-02</uri>). If
you wish to access the code used in this work prior to the public release of
version 11-02, you may do so at <uri>https://github.com/kyu0110/geoschem_ras</uri>.</p>
  </notes><notes notes-type="competinginterests"><title>Competing interests</title>

      <p id="d1e3904">The authors declare that they have no conflict of interest.</p>
  </notes><ack><title>Acknowledgements</title><p id="d1e3910">This work was funded by the Modeling, Analysis, and Prediction (MAP) program
of the NASA Earth Science Division. <?xmltex \hack{\newline}?><?xmltex \hack{\newline}?>
Edited by: Fiona O'Connor <?xmltex \hack{\newline}?>
Reviewed by: two anonymous referees</p></ack><ref-list>
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    <!--<article-title-html>Errors and improvements in the use of archived meteorological  data for chemical transport modeling: an analysis using GEOS-Chem v11-01 driven by GEOS-5 meteorology</article-title-html>
<abstract-html><p>Global simulations of atmospheric chemistry are commonly conducted with
off-line chemical transport models (CTMs) driven by archived meteorological
data from general circulation models (GCMs). The off-line approach has
the advantages of simplicity and expediency, but it incurs errors due to temporal
averaging in the meteorological archive and the inability to reproduce the
GCM transport algorithms exactly. The CTM simulation is also often conducted
at coarser grid resolution than the parent GCM. Here we investigate this
cascade of CTM errors by using <sup>222</sup>Rn–<sup>210</sup>Pb–<sup>7</sup>Be chemical tracer
simulations off-line in the GEOS-Chem CTM at rectilinear
0.25°&thinsp; × &thinsp;0.3125° ( ≈ &thinsp;25&thinsp;km) and
2°&thinsp; × &thinsp;2.5° ( ≈ &thinsp;200&thinsp;km) resolutions and
online in the parent GEOS-5 GCM at cubed-sphere c360 ( ≈ &thinsp;25&thinsp;km) and
c48 ( ≈ &thinsp;200&thinsp;km) horizontal resolutions. The c360 GEOS-5 GCM
meteorological archive, updated every 3&thinsp;h and remapped to
0.25°&thinsp; × &thinsp;0.3125°, is the standard operational product
generated by the NASA Global Modeling and Assimilation Office (GMAO) and used
as input by GEOS-Chem. We find that the GEOS-Chem <sup>222</sup>Rn simulation at
native 0.25°&thinsp; × &thinsp;0.3125° resolution is affected by
vertical transport errors of up to 20&thinsp;% relative to the GEOS-5 c360 online
simulation, in part due to loss of transient organized vertical motions in
the GCM (resolved convection) that are temporally averaged out in the 3&thinsp;h
meteorological archive. There is also significant error caused by operational
remapping of the meteorological archive from a cubed-sphere to a rectilinear
grid. Decreasing the GEOS-Chem resolution from
0.25°&thinsp; × &thinsp;0.3125° to
2°&thinsp; × &thinsp;2.5° induces further weakening of vertical
transport as transient vertical motions are averaged out spatially and
temporally. The resulting <sup>222</sup>Rn concentrations simulated by the
coarse-resolution GEOS-Chem are overestimated by up to 40&thinsp;% in surface air
relative to the online c360 simulations and underestimated by up to 40&thinsp;%
in the upper troposphere, while the tropospheric lifetimes of <sup>210</sup>Pb and
<sup>7</sup>Be against aerosol deposition are affected by 5–10&thinsp;%. The lost
vertical transport in the coarse-resolution GEOS-Chem simulation can be
partly restored by recomputing the convective mass fluxes at the appropriate
resolution to replace the archived convective mass fluxes and by correcting
for bias in the spatial averaging of boundary layer mixing depths.</p></abstract-html>
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