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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-12-1067-2019</article-id><title-group><article-title>LIVVkit 2.1: automated and extensible ice sheet model validation</article-title><alt-title>Software for ice sheet model validation</alt-title>
      </title-group><?xmltex \runningtitle{Software for ice sheet model validation}?><?xmltex \runningauthor{K.~J.~Evans et al.}?>
      <contrib-group>
        <contrib contrib-type="author" corresp="yes" rid="aff1">
          <name><surname>Evans</surname><given-names>Katherine J.</given-names></name>
          <email>evanskj@ornl.gov</email>
        <ext-link>https://orcid.org/0000-0001-8174-6450</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Kennedy</surname><given-names>Joseph H.</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-9348-693X</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Lu</surname><given-names>Dan</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2">
          <name><surname>Forrester</surname><given-names>Mary M.</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff3">
          <name><surname>Price</surname><given-names>Stephen</given-names></name>
          
        <ext-link>https://orcid.org/0000-0001-6878-2553</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff3 aff8">
          <name><surname>Fyke</surname><given-names>Jeremy</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-4522-3019</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff4">
          <name><surname>Bennett</surname><given-names>Andrew R.</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff3">
          <name><surname>Hoffman</surname><given-names>Matthew J.</given-names></name>
          
        <ext-link>https://orcid.org/0000-0001-5076-0540</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff5">
          <name><surname>Tezaur</surname><given-names>Irina</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff6">
          <name><surname>Zender</surname><given-names>Charles S.</given-names></name>
          
        <ext-link>https://orcid.org/0000-0003-0129-8024</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff7">
          <name><surname>Vizcaíno</surname><given-names>Miren</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-9553-7104</ext-link></contrib>
        <aff id="aff1"><label>1</label><institution>Computational Earth Sciences Group, Oak Ridge National Laboratory, Oak Ridge, TN, USA</institution>
        </aff>
        <aff id="aff2"><label>2</label><institution>Department of Geology and Geological Engineering, Colorado School of Mines, Golden, CO, USA</institution>
        </aff>
        <aff id="aff3"><label>3</label><institution>Fluid Dynamics and Solid Mechanics Group, Los Alamos National Laboratory, Los Alamos, NM, USA</institution>
        </aff>
        <aff id="aff4"><label>4</label><institution>Department of Civil and Environmental Engineering, University of Washington, Seattle, WA, USA</institution>
        </aff>
        <aff id="aff5"><label>5</label><institution>Sandia National Laboratories, Albuquerque, NM, USA</institution>
        </aff>
        <aff id="aff6"><label>6</label><institution>Departments of Earth System Science and Computer Science, University of California, Irvine, CA, USA</institution>
        </aff>
        <aff id="aff7"><label>7</label><institution>Department of Geoscience and Remote Sensing, Delft University of Technology, Delft, the Netherlands</institution>
        </aff>
        <aff id="aff8"><label>a</label><institution>now at: Associated Engineering, Vernon, BC, Canada</institution>
        </aff>
      </contrib-group>
      <author-notes><corresp id="corr1">Katherine J. Evans (evanskj@ornl.gov)</corresp></author-notes><pub-date><day>22</day><month>March</month><year>2019</year></pub-date>
      
      <volume>12</volume>
      <issue>3</issue>
      <fpage>1067</fpage><lpage>1086</lpage>
      <history>
        <date date-type="received"><day>9</day><month>March</month><year>2018</year></date>
           <date date-type="rev-request"><day>29</day><month>March</month><year>2018</year></date>
           <date date-type="rev-recd"><day>18</day><month>December</month><year>2018</year></date>
           <date date-type="accepted"><day>13</day><month>February</month><year>2019</year></date>
      </history>
      <permissions>
        <copyright-statement>Copyright: © 2019 Katherine J. Evans et al.</copyright-statement>
        <copyright-year>2019</copyright-year>
      <license license-type="open-access"><license-p>This work is licensed under the Creative Commons Attribution 4.0 International License. To view a copy of this licence, visit <ext-link ext-link-type="uri" xlink:href="https://creativecommons.org/licenses/by/4.0/">https://creativecommons.org/licenses/by/4.0/</ext-link></license-p></license></permissions><self-uri xlink:href="https://gmd.copernicus.org/articles/12/1067/2019/gmd-12-1067-2019.html">This article is available from https://gmd.copernicus.org/articles/12/1067/2019/gmd-12-1067-2019.html</self-uri><self-uri xlink:href="https://gmd.copernicus.org/articles/12/1067/2019/gmd-12-1067-2019.pdf">The full text article is available as a PDF file from https://gmd.copernicus.org/articles/12/1067/2019/gmd-12-1067-2019.pdf</self-uri>
      <abstract><title>Abstract</title>
    <p id="d1e220">A collection of scientific analyses, metrics, and visualizations for robust
validation of ice sheet models is presented using the Land Ice Verification
and Validation toolkit (LIVVkit), version 2.1, and the LIVVkit Extensions
repository (LEX), version 0.1. This software collection targets stand-alone
ice sheet or coupled Earth system models, and handles datasets and analyses
that require high-performance computing and storage. LIVVkit aims to enable
efficient and fully reproducible workflows for postprocessing, analysis, and
visualization of observational and model-derived datasets in a shareable
format, whereby all data, methodologies, and output are distributed to users
for evaluation. Extending from the initial LIVVkit software framework, we
demonstrate Greenland ice sheet simulation validation metrics using the
coupled Community Earth System Model (CESM) as well as an idealized
stand-alone high-resolution Community Ice Sheet Model, version 2 (CISM2),
coupled to the Albany/FELIX velocity solver (CISM-Albany or CISM-A). As one
example of the capability, LIVVkit analyzes the degree to which models
capture the surface mass balance (SMB) and identifies potential sources of
bias, using recently available in situ and remotely sensed data as
comparison. Related fields within atmosphere and land surface models, e.g.,
surface temperature, radiation, and cloud cover, are also diagnosed. Applied
to the CESM1.0, LIVVkit identifies a positive SMB bias that is focused
largely around Greenland's southwest region that is due to insufficient
ablation.</p>
  </abstract>
    </article-meta>
  <notes notes-type="copyrightstatement">
  
      <p id="d1e230">This paper has been authored by UT-Battelle, LLC
under contract no. DE-AC05-00OR22725 with the U.S. Department of Energy. The
United States Government retains and the publisher, by accepting the article
for publication, acknowledges that the United States Government retains a
non-exclusive, paid-up, irrevocable, worldwide license to publish or
reproduce the published form of this paper, or allow others to do so,
for United States Government purposes. The Department of Energy will provide
public access to these results of federally sponsored research in accordance
with the DOE Public Access Plan
(<uri>http://energy.gov/downloads/doe-public-access-plan</uri>).</p>
</notes></front>
<body>
      


<sec id="Ch1.S1" sec-type="intro">
  <title>Introduction</title>
      <p id="d1e242">About 10 % of human settlement is currently and will likely continue to
be clustered in regions potentially vulnerable to sea level rise (SLR)
<xref ref-type="bibr" rid="bib1.bibx33" id="paren.1"/>, which will arguably result in some of the most
devastating impacts of climate change. The polar ice sheets, and their
peripheral glaciers, referred to hereafter as “land ice”, represent the
largest potential source of SLR in a warming climate through (1) increased
meltwater runoff that is not compensated by increasing snowfall
<xref ref-type="bibr" rid="bib1.bibx11 bib1.bibx37" id="paren.2"/> and (2) increased ice discharge (calving and
marine melt) <xref ref-type="bibr" rid="bib1.bibx8" id="paren.3"/>. In order to provide credible
predictions of SLR to policymakers and stakeholders, scientists need accurate
representations of land ice as simulated within Earth system models (ESMs).</p>
      <?pagebreak page1068?><p id="d1e254">The scientific community's “best” projections of ice sheet mass change rely
on process-based models and, increasingly, model-ensemble projections from
stand-alone ice sheet models (ISMs) <xref ref-type="bibr" rid="bib1.bibx8" id="paren.4"/>. To
provide optimal results, these ice sheet models must include accurate
representations of ice sheet dynamics, physics, and coupling schemes (e.g.,
to obtain forcing from other components, like the ocean and atmosphere). As
these models are connected to coupled ESMs, coupled-model initialization
procedures and a quantitative understanding of key model sensitivities and
uncertainties <xref ref-type="bibr" rid="bib1.bibx60" id="paren.5"/> are also required. These challenges are
well recognized: there is an ongoing effort within coupled ESMs to develop a
dynamically active ISM <xref ref-type="bibr" rid="bib1.bibx28 bib1.bibx4 bib1.bibx63" id="paren.6"/> as well as
high-resolution and high-fidelity stand-alone ISMs <xref ref-type="bibr" rid="bib1.bibx24 bib1.bibx1" id="paren.7"/>.
Furthermore, the ISM community has organized a number of intercomparisons
under the umbrella of  the Ice Sheet Model
Intercomparison Project (ISMIP6) that are currently underway
<xref ref-type="bibr" rid="bib1.bibx38 bib1.bibx13" id="paren.8"/> to better understand and compare the distribution
of ISM predictions. These could also be used to track model development.</p>
      <p id="d1e272">Of course, there are limitations with all models; they are an imperfect
representation of actual observed behavior. It is critically important to
identify and quantify their most notable biases and discrepancies in order to
maximize the impact of model improvements and to increase confidence in model
predictions. However, the paucity of observational data in the polar regions,
especially data that are specifically relevant to ice sheets themselves, has
prevented a comprehensive assessment of ISM and coupled ESM-ISM skill, and
key climatological forcings that drive ISM evolution. Although technology has
enabled a significant growth in glacier and ice sheet observations via in
situ, airborne, and satellite-based systems in the last decade, this short
time frame can only provide current information because ice sheets, more than
other aspects of the surface climate system, evolve over much longer
timescales. Of course it is not possible to execute experiments in a lab setting
where one could adjust parameters to develop an account of the
sensitivities of the land ice system. While theoretical underpinnings can be
used to develop insight toward model sensitivities (refer to
<xref ref-type="bibr" rid="bib1.bibx50" id="altparen.9"/> for a review and summary of progress), these constructs
are also limited by our current understanding of the drivers of ice sheet
evolution.</p>
      <p id="d1e278">With the aim of facilitating large-scale development and execution of ISM and
coupled ESM-ISM experiments, and determining the degree to which they
sufficiently represent aspects of the actual Earth system, we present the
software and data package LEX <xref ref-type="bibr" rid="bib1.bibx22" id="paren.10"/>, a validation extension to
the Land Ice Verification and Validation toolkit
<xref ref-type="bibr" rid="bib1.bibx21" id="paren.11"><named-content content-type="pre">LIVVkit;</named-content></xref>, which provides a basic but extensible
capability to assess ice sheet models within, and independent of, coupled ESM
configurations (hereafter, LIVVkit and LEX will collectively be referred to
as simply LIVVkit). The philosophy of verification and validation (V&amp;V),
using terminology and standards from <xref ref-type="bibr" rid="bib1.bibx40" id="text.12"/>, and its adoption
by the LIVVkit to verify ice sheet model simulations is presented and
discussed in <xref ref-type="bibr" rid="bib1.bibx20" id="text.13"/>. Efforts to validate both ISM and ISM-ESM
behavior, including a new capability to compare ESM-derived surface mass
balance against recently available observations, are detailed here.</p>
</sec>
<sec id="Ch1.S2">
  <title>Target simulations and comparison data</title>
<sec id="Ch1.S2.SS1">
  <title>Target simulations for analysis</title>
      <p id="d1e306">In order to demonstrate the validation features of LIVVkit, we analyze output
from two Greenland ice sheet (GrIS) simulations from (1) a high-resolution
ISM and (2) a global, fully coupled ESM from which ISM forcing is derived.
Both have been presented in the literature and made available to us, which
allows us to verify the software for use by others with confidence and
complement existing community validation efforts.</p>
      <p id="d1e309">For the high-resolution Greenland ISM simulation (1), data were generated
from the Community Ice Sheet Model, version 2 (CISM2; <xref ref-type="bibr" rid="bib1.bibx46" id="altparen.14"/>),
coupled to the Albany/FELIX velocity solver <xref ref-type="bibr" rid="bib1.bibx54 bib1.bibx55" id="paren.15"/>,
hereafter referred to as CISM-A. These simulations are described in detail
by <xref ref-type="bibr" rid="bib1.bibx47" id="text.16"/>. This configuration is selected to highlight how LIVVkit could
be used to validate a stand-alone simulation that can then be used as an
initial condition for follow-on simulations. The simulation used here
includes a dynamic ice sheet component forced by a time-varying surface mass
balance (SMB) field. It spans the years 1991–2013, although these dates should be
considered a generic present-day period because the data assimilation
techniques used for the initialization used multiple datasets from the last
20 years. The initial state was generated through a multi-step procedure to
produce balanced internal temperature and velocity fields, which was then
forced by surface mass balance anomalies from the Regional Area Climate Model
(RACMO, version 2; <xref ref-type="bibr" rid="bib1.bibx56" id="altparen.17"/>). The goal in creating these simulations
was to illustrate the use of the Cryospheric Model Comparison Tool
(CmCt), an ice sheet model validation tool that focuses primarily on the
preprocessing necessary to facilitate the comparison of satellite data to ISM
output <xref ref-type="bibr" rid="bib1.bibx39" id="paren.18"/>. That effort is complementary to the validation
software presented here, which focuses on comparisons to in situ and
remotely sensed data from other sources.</p>
      <p id="d1e327">For the coupled ESM (2), we analyze output from the atmosphere <xref ref-type="bibr" rid="bib1.bibx36" id="paren.19"/>
and land surface <xref ref-type="bibr" rid="bib1.bibx25" id="paren.20"/> components within a global, fully coupled
simulation from the Community Earth System Model (CESM version 1.0.6;
<xref ref-type="bibr" rid="bib1.bibx6" id="altparen.21"/>). For this model,
the ice sheet surface mass balance (accumulation of less runoff<?pagebreak page1069?> and
sublimation) is calculated within the snowpack model of the land surface
component and then downscaled to the relatively higher-resolution ice sheet
grid in order to provide SMB forcing for the ISM component <xref ref-type="bibr" rid="bib1.bibx49" id="paren.22"/>,
as described in <xref ref-type="bibr" rid="bib1.bibx28" id="text.23"/>. Details about the simulation and the SMB are
presented in <xref ref-type="bibr" rid="bib1.bibx61" id="text.24"/> (hereafter V13). Here, we focus on a historical,
transient simulation spanning 1850–2005, although we restrict our analysis
to 1960–2005 except where noted to avoid issues related to model spin-up.
Hereafter, we refer to this simulation as CESM.</p>
</sec>
<sec id="Ch1.S2.SS2">
  <title>Comparison data specific for ISM</title>
      <p id="d1e355">ISMs that use a data assimilation approach to most closely reproduce
present-day conditions for their initial state and forcing (as compared to those that
are spun up from pre-industrial or earlier states) currently use much of the
most informative observational data for model initialization. As an example
to move the community towards robust present-day validation, we apply LIVVkit
to generate and present model–data comparisons using as many available
datasets as possible and including those that are used for model
initialization.</p>
      <p id="d1e358">For validation of surface velocity and ice thickness, the data available for
comparison are initialization data. These were obtained using a
partial differential equation (PDE)-constrained optimization procedure <xref ref-type="bibr" rid="bib1.bibx44" id="paren.25"/>. We include these in
LIVVkit with the expectation that independent data will replace these data
within the same workflow going forward. LIVVkit makes use of a GitHub
repository of scripts and procedures <xref ref-type="bibr" rid="bib1.bibx19" id="paren.26"/> that procures the
surface velocity and thickness datasets from a host of publicly available
sources. The workflow processes this dataset to create a number of fields of
variables in an expected format, with all the masking and projections necessary for postprocessing in LIVVkit (explained in Sect. <xref ref-type="sec" rid="Ch1.S3"/>). The velocity fields used for comparison originate from
the NASA Making Earth System Data Records for Use in Research
Environments (MEaSUREs) program, which provides annual ice-sheet-wide
velocity maps for Greenland, derived using Interferometric Synthetic Aperture
Radar (InSAR) data from the RADARSAT-1 satellite
<xref ref-type="bibr" rid="bib1.bibx16 bib1.bibx17" id="paren.27"/>. The dataset currently contains ice velocity
data for the winters of 2000–2001 and 2005–2006, 2006–2007, and 2007–2008
acquired from RADARSAT-1 InSAR data from the Alaska Satellite Facility (ASF),
and a 2008–2009 mosaic derived from the Advanced Land Observation Satellite
(ALOS) and TerraSAR-X data. For bed topography and ice thickness, we use the
Greenland Ice Mapping Project digital elevation model <xref ref-type="bibr" rid="bib1.bibx15" id="paren.28"><named-content content-type="pre">GIMP
DEM;</named-content></xref> for topography of the ice-free areas, and the
<xref ref-type="bibr" rid="bib1.bibx34" id="text.29"/> bed topography and ice thickness estimates, which are derived
from ice surface elevation data, airborne radar soundings from Operation
IceBridge, and the GIMP DEM (as a reference surface). It is straightforward
to update and/or augment these same data with new years and locations as they
become available <xref ref-type="bibr" rid="bib1.bibx35" id="paren.30"><named-content content-type="pre">e.g.,</named-content></xref>.</p>
</sec>
<sec id="Ch1.S2.SS3">
  <title>Comparison data specific for ESM</title>
      <p id="d1e392">In the case of coupled ESM validation for ISM development, modelers will
benefit from more focused and quantitative evaluation in the vicinity of the
GrIS, as compared to the global and regional model validation typically
provided with the release of components that comprise ESM. Therefore, LIVVkit
provides validation of the atmosphere and land surface components in ESMs
specifically over the GrIS region for key variables that affect it.
Validation of the atmosphere and land surface is still limited by the
availability of observed data over the GrIS (and Antarctic ice sheet),
whether it is used directly or within reanalysis products. As with the ice
sheet data, additional regional in situ and remotely sensed data will improve
LIVVkit and are a target for further development.</p>
      <p id="d1e395">From LIVVkit, the examples presented in Sect. <xref ref-type="sec" rid="Ch1.S4.SS2"/> include
cloud fractions from an ESM, which are compared to the International
Satellite Cloud Climatology Project (ISCCP) <xref ref-type="bibr" rid="bib1.bibx48" id="paren.31"/> and the combined
CloudSat radar and Cloud-Aerosol Lidar with Orthogonal Polarization (CALIOP) lidar datasets (hereafter CLOUDSAT) <xref ref-type="bibr" rid="bib1.bibx18" id="paren.32"/>
reanalysis products. ISCCP resolves the diurnal cycle, within which monthly
averages are created, and provides the longest available time record.
CLOUDSAT covers only a short time record; however, the detection techniques
are considered superior for the Arctic. The interested reader is referred to
the Climate Data Guide <xref ref-type="bibr" rid="bib1.bibx45" id="paren.33"/> for more details about the attributes and
limitations of these datasets.</p>
</sec>
<sec id="Ch1.S2.SS4">
  <title>Surface mass balance comparison data</title>
      <p id="d1e415">Given the dependence of ice sheet evolution on surface mass balance, LIVVkit
tracks SMB for both coupled ESM and stand-alone ISM, even if it is provided
as a forcing for a simulation for the ISM. For an ice-sheet-wide view of SMB
behavior, LIVVkit presents metrics relative to the most recently available
version of RACMO, version 2.3 (RACMO2.3), the characteristics of which are
summarized in <xref ref-type="bibr" rid="bib1.bibx37" id="text.34"/>. The configuration of RACMO2.3 has been
specifically designed and validated for its fidelity in capturing the
extended Greenland region. As with initialization data, model-to-model
comparisons of SMB data do not provide independent validation. This is
especially true when applied to a stand-alone ISM that has been forced with
model SMB, as is the case for CISM-A, which has been forced with RACMO2.0
(presented in Sect. <xref ref-type="sec" rid="Ch1.S4.SS1"/>). We include these comparisons within
LIVVkit because it is useful (1) when presented against ESM SMB and (2) to
have available when monitoring other aspects of ice sheet evolution to
attribute sources of bias. RACMO2.3 data are provided at<?pagebreak page1070?> approximately 11 km
horizontal resolution with 40 vertical layers and include the GrIS and
other nearby areas. LIVVkit is currently configured to compare years
1980–1999 of the RACMO2.3 simulation because it was forced with the more
recent ERA-Interim reanalysis data <xref ref-type="bibr" rid="bib1.bibx51 bib1.bibx10" id="paren.35"/> from 1979 to 2014, and
many of the model development runs for Earth system models cover the period
spanning 1979–2000 as part of the Atmospheric Model Intercomparison Protocol
(AMIP-II) <xref ref-type="bibr" rid="bib1.bibx12" id="paren.36"/>.</p>
      <p id="d1e429">To provide independent validation of an ESM SMB field, LIVVkit compares in
situ SMB values using 623 core/pit/stake measurements from a diversity of
sources. Many of these were included in <xref ref-type="bibr" rid="bib1.bibx61" id="text.37"><named-content content-type="post">Fig. 6</named-content></xref> but have been
updated in LIVVkit with new data and selection criteria. For a station to be
included, it must contain a record of location, elevation, and observation
start/end dates. Here, we use 387 locations out of a possible 450 from a
collection of accumulation-zone (net specific SMB <inline-formula><mml:math id="M1" display="inline"><mml:mrow><mml:mo>&gt;</mml:mo><mml:mn mathvariant="normal">0</mml:mn></mml:mrow></mml:math></inline-formula>) estimates compiled
by <xref ref-type="bibr" rid="bib1.bibx9" id="text.38"/> using data from <xref ref-type="bibr" rid="bib1.bibx41" id="text.39"/>, <xref ref-type="bibr" rid="bib1.bibx42" id="text.40"/>, and
<xref ref-type="bibr" rid="bib1.bibx2" id="text.41"/>. In addition to the stations included from <xref ref-type="bibr" rid="bib1.bibx2" id="text.42"/>,
38 additional ice cores from the Program for Arctic Regional Climate Assessment (PARCA) <xref ref-type="bibr" rid="bib1.bibx3" id="paren.43"/> have been added, with six of
those as replacements to the earlier 2001 study. The PARCA compilation also
includes reanalyses of time series from 20 coastal weather stations to
estimate SMB; however, only estimates from ice cores and snow pits are
currently included in LIVVkit. We also include data from the Programme for Monitoring of the Greenland Ice Sheet  (PROMICE), a
compilation of glacier explorations and in situ measurements taken since the
1960s from the GrIS ablation zone (SMB <inline-formula><mml:math id="M2" display="inline"><mml:mrow><mml:mo>&lt;</mml:mo><mml:mn mathvariant="normal">0</mml:mn></mml:mrow></mml:math></inline-formula>) <xref ref-type="bibr" rid="bib1.bibx31" id="paren.44"/>. From 790
original locations, all but 198 stations were excluded based on the following
criteria:
<list list-type="bullet"><list-item>
      <p id="d1e481">unknown elevation or start or end date of observation period;</p></list-item><list-item>
      <p id="d1e485">observation period was less than 95 % of a year (i.e., seasonal
data);</p></list-item><list-item>
      <p id="d1e489">accumulation data were derived using a methodology other than pit/core measurements (e.g., weather
stations or surface lowering relative to ramp road).</p></list-item></list>
For all stations, temporal data were aggregated and treated as typical
climatology, regardless of the record length. If annual SMB estimates were
supplied for multiple years, LIVVkit averages over all years to provide a
single annual value for each location. Because station selection is subject
to various adjustments based on the type of validation to be performed, we
choose these selection criteria to facilitate a general starting-point
comparison.</p>
      <p id="d1e493">Model results are also compared to accumulation estimates derived from 25
NASA Operation IceBridge radar airborne flights from the 2013 and 2014
seasons as detailed in <xref ref-type="bibr" rid="bib1.bibx27" id="text.45"/> and the associated supplementary
data. The measurements capture internal reflecting horizons in the top few
hundred meters of the ice sheet, which can be used to estimate the historical
SMB record spanning the past three centuries. The IceBridge data from
<xref ref-type="bibr" rid="bib1.bibx27" id="text.46"/> are provided as raw estimates seasonally for a given
lat/long coordinate. Because the temporal record varies for each site, LIVVkit
calculates annually averaged SMB at each location.</p>
      <p id="d1e502">In order to provide basin-scale estimates of SMB, we use the <xref ref-type="bibr" rid="bib1.bibx64" id="text.47"/>
drainage basin delineations as visualized by color in Fig. <xref ref-type="fig" rid="Ch1.F1"/>
(colors) and with numbering conventions preserved. This figure also
illustrates the location and extent of basin-wide SMB data, including
pit/core locations (filled shapes) and IceBridge altimetry transects (white
lines). Accumulation-zone SMB estimates from <xref ref-type="bibr" rid="bib1.bibx9" id="text.48"/> and
<xref ref-type="bibr" rid="bib1.bibx3" id="text.49"/> PARCA cores are shown as blue circles, while ablation-zone
PROMICE data <xref ref-type="bibr" rid="bib1.bibx31" id="paren.50"/> are shown as yellow triangles. The data
points are sized by the length of their temporal record, with larger markers
indicating that estimates were averaged from a greater number of annual SMB
values.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F1" specific-use="star"><label>Figure 1</label><caption><p id="d1e522">Greenland ice sheet drainage basin
delineations (colored and numbered regions) as in <xref ref-type="bibr" rid="bib1.bibx64" id="text.51"/>, the location
and temporal extent of the pit/core locations (filled circles and triangles),
and the altimetry transects (white lines) used in LIVVkit SMB analyses. The
basin numbers follow Zwally's designation and the colors correspond to those
used in histograms and scatter plots throughout. Pit/core data points are
sized by the length of their temporal record, with larger points indicating
annual estimates were taken from a greater number of yearly SMB
values.</p></caption>
          <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://gmd.copernicus.org/articles/12/1067/2019/gmd-12-1067-2019-f01.png"/>

        </fig>

      <p id="d1e534">Processing the IceBridge data from <xref ref-type="bibr" rid="bib1.bibx27" id="text.52"/>, which are provided as
raw estimates seasonally for a given latitude/longitude coordinate, is a
two-step process in LIVVkit. Each model cell is assigned to a Z12 basin.
LIVVkit does this by converting the Z12 drainage basin outlines into
polygons, and then decides which polygon contains which model cell centers.
If a model cell center is not within any of the basin polygons, it is
assigned basin “0”. Correspondingly, each IceBridge measurement at a
lat/long location is averaged over seasons to obtain an annual SMB value. Some
locations have older SMB records so the average annual SMB value used for
comparison to the model is the mean over all available temporal records.
Then, a kd-tree/nearest-neighbor method is used to find the model cell closest to
the observed lat/long measurement. Thus, the Z12 basin at that location will
be the same one as the corresponding model cell, found in the first step.</p>
      <p id="d1e540">The present strategy to include both observational and model comparison data
was chosen to maximize (1) clarity (the scientist understands the limitations
of the information); (2) reproducibility (automation within LIVVkit); and
(3) extensibility (users can add additional data for their own comparisons
with minimal local adaption of the code). For provenance, changes to
LIVVkit's inclusion of new data are controlled through releases so users can
be certain of the data they are comparing for a given tag of the data
repository. LIVVkit can be altered at will once the code is forked or
downloaded locally to suit the user's needs. The step to process comparison
data is a separate step explained in Sect. <xref ref-type="sec" rid="Ch1.S3"/>, but it is
automated and fully documented. A discussion about potential new candidate
data to add to the current collection is provided in Sect. <xref ref-type="sec" rid="Ch1.S5"/>.
Additional details and references to the comparison data can be found on the
GitHub site <xref ref-type="bibr" rid="bib1.bibx21" id="paren.53"/>.</p>
</sec>
</sec>
<?pagebreak page1071?><sec id="Ch1.S3">
  <title>Software infrastructure for validation</title>
      <p id="d1e557">LIVVkit is a Python-based, open-source software package designed for
verification and validation of ice sheet and Earth system models. LIVVkit
operates on model output, viewing the model as a black box. This strategy
provides flexibility in analyzing many different models, assuming some basic
conventions are followed. LIVVkit is installable through Anaconda/Miniconda,
PiPy, or GitHub, and provides the <monospace>livv</monospace> command line interface (CLI),
which is used to execute the analyses and output the results to a portable
website on the user's local machine. The details of the design<?pagebreak page1072?> philosophy,
construction, and verification components of LIVVkit are described in detail
along with an example of validation to show the structure of the overall
toolkit in <xref ref-type="bibr" rid="bib1.bibx20" id="text.54"/>. A robust validation capability for ESM and ISM,
which includes modules for postprocessing and organization of model and
observational data and the creation of plots, tables, and metrics, is
presented here.</p>
      <p id="d1e566">There are three major steps to validate a model simulation (or set of
simulations): (1) gathering the required observational and model output data,
(2) postprocessing the observational and raw model output data to make
comparable data products, and (3) running the analyses and creating
visualizations of the prepared data products. On the observational side,
steps (1) and (2) require a significant amount of time investment <xref ref-type="bibr" rid="bib1.bibx53" id="paren.55"><named-content content-type="pre">up
to 70 % of the time spent on analytics projects;</named-content></xref>
due to the disparate nature of observational data reporting, the large variety of
formats involved, and the expertise often needed to correctly manipulate
observing data. Similarly, for both modeling and observational data, a
significantly large, and ever-increasing, amount of data needs to be moved
from raw data storage locations to the analysis machine. For example, NASA's
Earth observing data are expected to grow to 50 PB by 2020 <xref ref-type="bibr" rid="bib1.bibx29" id="paren.56"/>. Similarly, even the
ice-sheet-only CISM-A simulation data described above constitute well over
200 GB of data.</p>
      <p id="d1e577">To deal with the challenges surrounding steps (1) and (2), either the
observing data are brought to an analysis machine co-located with the model
data or the model data are brought to an analysis machine co-located with the
observations (and observational specialists). Due to the sophistication
required for analysis of GRACE data, <xref ref-type="bibr" rid="bib1.bibx47" id="text.57"/> and <xref ref-type="bibr" rid="bib1.bibx39" id="text.58"/> have
taken the latter approach. However, workflow is hard to integrate into a
model development cycle, especially one using automated testing, and so
moving processed observational data to analysis machines at modeling centers is
the preferred approach by Earth system models <xref ref-type="bibr" rid="bib1.bibx59" id="paren.59"><named-content content-type="pre">e.g.,
CESM;</named-content></xref>. In either approach, the data being moved are
processed into a comparable product before the movement happens in order to
reduce the amount of data transferred. Even so, the data repository for CESM
is well over 1 TB in size <xref ref-type="bibr" rid="bib1.bibx59" id="paren.60"/>.</p>
      <p id="d1e594">LIVVkit has taken a hybrid approach of the two strategies by developing a
LIVVkit Extensions (LEX) package <xref ref-type="bibr" rid="bib1.bibx22" id="paren.61"/>, which is available via
GitLab repository, under a modified BSD open-source license, hosted at Oak
Ridge National Laboratory <xref ref-type="bibr" rid="bib1.bibx22" id="paren.62"><named-content content-type="pre">ORNL;</named-content></xref>. The repository holds a
collection of validation analysis extension to LIVVkit, as well as
observational and model data by utilizing git large file support
(<monospace>git-lfs</monospace>). Each analysis in LEX is required to provide at minimum
the required processed observational data; a <monospace>README</monospace> describing the
original data, how to acquire them, and any rehosting/licensing issues
associated with the data; a BibTeX file containing any relevant citations;
postprocessing scripts used to generate the processed data; and a minimal set
of model data such that an example analysis can be run. The LEX repository is
already sizable, as it contains some large (gigabyte-scale) observations
datasets, and is expected to grow to unwieldy proportions as more
observational data are included and older datasets are updated. In order to
handle the projected size of this repository, LIVVkit details the commands
necessary to only clone the analysis files without the data files (e.g., the
description, configuration, and BibTeX files) in order to see which analyses
are available, and then pull down just the latest version of the required
data to run the analyses. This allows both observationalists and modelers to
co-develop the analyses available by always having a minimal working example
available. Further facilitating this co-development is the GitHub-like
interface provided by the GitLab instance which allows code and datasets to
be commented on, issues to be raised, and development goals and tasks to be
outlined.</p>
      <p id="d1e612">For the model and observation data discussed here, LEX provides a set of
single-execution, task-parallel postprocessing (bash) scripts designed for
automated postprocessing of output at LCFs, so that the data are prepared for
scientific analysis through (and outside of) LIVVkit. These scripts can be
adapted for other systems, although smaller computing systems may limit the
user to lower-resolution data as a target. Earth system models are comprised
of multiple component models (e.g., land, ocean, atmosphere, sea ice, land
ice) that may either be active or provided as a data model, depending on the
configuration selected. LIVVkit currently targets the atmosphere, land
surface, and ice sheets if they are active, creating a new directory set by
the user that contains subdirectories for each component and all their final
data products, including their incumbent metadata and associated masking and
mapping files. This enables full reproducibility and structure for additional
analysis within or independent of LIVVkit.</p>
      <p id="d1e615">The postprocessing scripts use a combination of Python and NetCDF operators
(NCOs) <xref ref-type="bibr" rid="bib1.bibx62" id="paren.63"/>, an open-source collection of programs that operate on a
diversity of scientific data. They use <monospace>ncclimo</monospace> commands within
versions NCO/4.6.9 and later to facilitate the extraction of monthly,
seasonal, and annual means (and optionally, to regrid the data) as well as
its baseline commands to average, sum, produce weighted and masked data, and
other operations typically used in geoscientific analyses. NCO addresses
provenance and transparency by appending the specific details of operations
within the metadata of datasets it processes and it performs task parallelism
where applicable.</p>
      <p id="d1e624">For stand-alone ice sheet model output (i.e., where climate forcing fields
such as surface temperature and surface mass balance are not
provided from coupling to a climate model), LIVVkit processes the SMB data
used to force the model, thickness, three-dimensional temperature and
horizontal velocity, and surface elevation, and it assumes that the data are
located within a single file. From the velocity components, it will create
the velocity norms. When complete, the postprocessed data directory contains
<list list-type="bullet"><list-item>
      <p id="d1e629">multi-year monthly, seasonal, and annual climatologies (time averages)
over the selected period for all
variables;</p></list-item><list-item>
      <p id="d1e633">time series of all variables and their annually and area-weighted averages
over the length of output for
selected variables; and</p></list-item><list-item>
      <p id="d1e637">annual and seasonal ice sheet mask area-weighted and GrIS-masked averages
for selected variables over the
selected period of analysis.</p></list-item></list>
For GrIS-masked data, values are averaged over a region defined by a minimum
ice thickness (0.001 m default, used for this analysis). For velocity, areal
averages are computed over the cells where they are defined.</p>
      <p id="d1e641">When processing large-scale coupled Earth system model simulations, to which
an active ice sheet may or may not be coupled, LIVVkit targets radiation,
thermodynamics, hydrological, and dynamical variables that influence ice
sheet evolution. This process is more extensible and robust than for
stand-alone ice sheet model processing, as coupled models more closely follow
metadata conventions. For the coupled model, the completed postprocessed data
directory contains
<list list-type="bullet"><list-item>
      <p id="d1e646">multi-year monthly, seasonal, and annual climatologies over the selected
period for all variables;</p></list-item><list-item>
      <p id="d1e650">time series of annually and area-weighted averages and GrIS masked for
selected variables, each in a
separate file, over the length of output;</p></list-item><list-item>
      <p id="d1e654">annual and seasonal area-weighted and GrIS-masked averages for selected
variables over the selected period of analysis; and</p></list-item><list-item>
      <p id="d1e658">annualized daily averages for selected variables over the full length of
the simulation</p></list-item></list>
within subdirectories for each component. Processing these high-resolution
data requires computing nodes with high memory. These “fat” nodes can be
accessed using batch nodes at LCFs, and LIVVkit's processing scripts handle
the batch queue submission.</p>
      <p id="d1e662">It is important to acknowledge that there are numerous intellectual property
concerns with hosting and redistributing datasets. To partially satisfy these
concerns, LIVVkit uses the data description to provide some context to the
analysis and requests that the original data authors are cited in any
publication which utilizes the analyses for testing, development, or
scientific analysis. The appropriate citations, detailed in the provided
BibTeX file, are listed on the output website. Additionally, LEX maintains a
public–private development cycle where analyses are developed in a private
git repository (also hosted at ORNL) and only released to the public
repository once dataset author/maintainer permission is provided (LIVVkit
itself is publicly developed). For analyses that rely on datasets where
permission cannot be granted, LIVVkit will provide a description of how to
acquire the data and scripts to process the data for analysis.</p>
      <p id="d1e665">Currently, the LIVVkit development team is pursuing partnerships with data
providers like NASA and NSIDC to reduce or eliminate the time to get new
analyses into the public LEX repository. We note that the lack of
standards/adoption and/or metadata conventions, e.g., CF conventions, has
been the biggest challenge for the rapid inclusion of a dataset in LEX,
rather than intellectual property concerns.</p>
      <p id="d1e669">Once the postprocessing is complete, the prepared model and
observational/comparison data are analyzed over a suite of time and space
slices and are provided to the users in a combination of easily digestible
text, tables, and figures. A validation analysis is initiated by pointing the
LIVVkit execute command, <monospace>livv</monospace>, to a JSON<fn id="Ch1.Footn1"><p id="d1e675">JavaScript Object
Notation is a lightweight, language-independent tool that both machines and
humans can parse.</p></fn> configuration file that specifies the analysis details:<?xmltex \hack{\newline}?><?xmltex \hack{\newline}?><?xmltex \hack{\noindent}?><?xmltex \igopts{height=8.535827pt}?><inline-graphic xlink:href="https://gmd.copernicus.org/articles/12/1067/2019/gmd-12-1067-2019-g01.png"/></p>
      <p id="d1e686">Within the JSON configuration file, the user provides the type of model run
and the location of the output and comparison data. The user may also specify
the location where the output data and website will be placed when complete
(via the –<monospace>out-dir</monospace> or <monospace>-o</monospace> option) and launch a simple HTTP
server to host the website (via the –<monospace>serve</monospace> or <monospace>-s</monospace> option).
When the HTTP server is launched, a direct hyperlink is printed on the
command line to either the analyses that were just executed or a previous
analysis selected via the CLI. For example, all the figures and analyses
presented here can be reproduced by executing the following command from the
top directory of LEX.<?xmltex \hack{\newline}?><?xmltex \hack{\newline}?><?xmltex \hack{\noindent}?><?xmltex \igopts{width=213.395669pt}?><inline-graphic xlink:href="https://gmd.copernicus.org/articles/12/1067/2019/gmd-12-1067-2019-g02.png"/></p>
      <?pagebreak page1074?><p id="d1e709">While any particular analysis performed by LIVVkit can be quite
sophisticated, creating a new analysis in LIVVkit/LEX is intended to be
straightforward for the user. The processes of building an extension is
detailed in the LIVVkit documentation. A template validation analysis is
provided within the software that details the minimal Python code needed to
run an analysis script, along with a minimal template JSON configuration
file. A user can place any external information needed by their analysis in
the configuration file (e.g., paths to data, years to analyze, method
switches). For sophisticated analyses, LIVVkit is also able to import
analysis packages developed with a standard Python package structure as long
as a configuration file and a LIVVkit entry point are provided. The LEX
repository also functions as a set of examples and contains both the basic
script and package style analyses.</p>
</sec>
<sec id="Ch1.S4">
  <title>Presentation and visualization</title>
      <p id="d1e719">Targeting stand-alone ice sheet and coupled Earth system model output within
LIVVkit provides two common use cases of model evaluation of ice sheet
behavior and drivers. A subset of these analyses is presented below, with a
special focus on a basin-wide analysis of the surface mass balance using more
recent observational data presented in Sect. <xref ref-type="sec" rid="Ch1.S2"/>.</p>
<sec id="Ch1.S4.SS1">
  <title>Stand-alone land ice model analysis</title>
      <p id="d1e729">Using GrIS simulation data, processed as described in Sect. <xref ref-type="sec" rid="Ch1.S3"/>,
LIVVkit produces a website with metrics and plots for
validation. As an overall check of model behavior and to identify potential
large-scales biases, there is a table of annualized and areal average values
over the selected time record for relevant variables, which includes the
SMB forcing, dimensional velocity (e.g., zonal (<inline-formula><mml:math id="M3" display="inline"><mml:mi>U</mml:mi></mml:math></inline-formula>)
and meridional (<inline-formula><mml:math id="M4" display="inline"><mml:mi>V</mml:mi></mml:math></inline-formula>) velocity components, respectively), and velocity norm.
Table <xref ref-type="table" rid="Ch1.T1"/> displays a similar version of the table produced by
LIVVkit as applied to the CISM-A simulation described in
Sect. <xref ref-type="sec" rid="Ch1.S2"/>.</p>

<?xmltex \floatpos{t}?><table-wrap id="Ch1.T1"><label>Table 1</label><caption><p id="d1e755">Area-weighted and GrIS-masked annual averages for variables from
CISM-A model output. “Input areal average” refers to the processed
datasets from observations as described in Sect. <xref ref-type="sec" rid="Ch1.S2"/> that are used
for the initial state of the model before spin-up.</p></caption><oasis:table frame="topbot"><oasis:tgroup cols="4">
     <oasis:colspec colnum="1" colname="col1" align="left"/>
     <oasis:colspec colnum="2" colname="col2" align="left"/>
     <oasis:colspec colnum="3" colname="col3" align="right"/>
     <oasis:colspec colnum="4" colname="col4" align="right"/>
     <oasis:thead>
       <oasis:row>
         <oasis:entry colname="col1">Variable</oasis:entry>
         <oasis:entry colname="col2">Units</oasis:entry>
         <oasis:entry colname="col3">Model</oasis:entry>
         <oasis:entry colname="col4">Input</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2"/>
         <oasis:entry colname="col3">areal</oasis:entry>
         <oasis:entry colname="col4">areal</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2"/>
         <oasis:entry colname="col3">average</oasis:entry>
         <oasis:entry colname="col4">average</oasis:entry>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row>
         <oasis:entry colname="col1">SMB</oasis:entry>
         <oasis:entry colname="col2">kg m<inline-formula><mml:math id="M5" 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> a<inline-formula><mml:math id="M6" 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></oasis:entry>
         <oasis:entry colname="col3">259.0</oasis:entry>
         <oasis:entry colname="col4">255.9</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Top layer temperature</oasis:entry>
         <oasis:entry colname="col2"><inline-formula><mml:math id="M7" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C</oasis:entry>
         <oasis:entry colname="col3"><inline-formula><mml:math id="M8" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2.3</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col4">NA</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1"><inline-formula><mml:math id="M9" display="inline"><mml:mi>U</mml:mi></mml:math></inline-formula> velocity</oasis:entry>
         <oasis:entry colname="col2">m a<inline-formula><mml:math id="M10" 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></oasis:entry>
         <oasis:entry colname="col3"><inline-formula><mml:math id="M11" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">8.3</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col4"><inline-formula><mml:math id="M12" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">14.5</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1"><inline-formula><mml:math id="M13" display="inline"><mml:mi>V</mml:mi></mml:math></inline-formula> velocity</oasis:entry>
         <oasis:entry colname="col2">m a<inline-formula><mml:math id="M14" 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></oasis:entry>
         <oasis:entry colname="col3"><inline-formula><mml:math id="M15" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">3.1</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col4"><inline-formula><mml:math id="M16" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">0.8</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Velocity norm</oasis:entry>
         <oasis:entry colname="col2">m a<inline-formula><mml:math id="M17" 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></oasis:entry>
         <oasis:entry colname="col3">54.3</oasis:entry>
         <oasis:entry colname="col4">62.7</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Ice thickness</oasis:entry>
         <oasis:entry colname="col2">m</oasis:entry>
         <oasis:entry colname="col3">2179</oasis:entry>
         <oasis:entry colname="col4">1781</oasis:entry>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup></oasis:table><table-wrap-foot><p id="d1e760">NA: not available.</p></table-wrap-foot></table-wrap>

      <p id="d1e1031">LIVVkit displays a suite of two-dimensional contour plots of climatological
averages over the selected time record. Figure <xref ref-type="fig" rid="Ch1.F2"/> presents
the surface mass balance from CISM-A, RACMO2.3, and their difference. Because
the CISM-A simulation was forced with RACMO2.0 and not RACMO2.3 data, there
are differences between CISM-A and RACMO2.3 that mirror the differences
between the RACMO versions, in particular the southwestern and northern melt
regions and over strong accumulation regions <xref ref-type="bibr" rid="bib1.bibx37" id="paren.64"/>. Although for
this example of SMB within CISM-A, the comparison is somewhat contrived to
illustrate capability, SMB forcings can be monitored along with output
variables to track their impact on the simulation.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F2" specific-use="star"><label>Figure 2</label><caption><p id="d1e1042">Surface mass balance contours for <bold>(a)</bold> CISM-A forced with
RACMO2.0, <bold>(b)</bold> RACMO2.3, and <bold>(c)</bold> CISM-A minus RACMO2.3, with
CISM-A interpolated to the coarser RACMO2.3 grid.</p></caption>
          <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://gmd.copernicus.org/articles/12/1067/2019/gmd-12-1067-2019-f02.png"/>

        </fig>

      <p id="d1e1060">Scatter plots comparing the same data are also displayed, whereby areas with
close correspondence between the two datasets are clustered along the red
identity line. As applied to CISM-A vs. RACMO2.3 for the SMB
(Fig. <xref ref-type="fig" rid="Ch1.F3"/>), generally the differences between the
model and RACMO2.3 surface mass balance values are small (as expected given
the origin of the SMB forcing data).</p>

      <?xmltex \floatpos{p}?><fig id="Ch1.F3"><label>Figure 3</label><caption><p id="d1e1067">Scatter plot of all grid points of SMB for RACMO2.3 vs. CISM-A
interpolated to the RACMO2.3 grid.</p></caption>
          <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://gmd.copernicus.org/articles/12/1067/2019/gmd-12-1067-2019-f03.png"/>

        </fig>

      <p id="d1e1076">LIVVkit also presents contour figures for the GrIS climatology of top-level
temperature (without comparison data; not shown), and velocity <inline-formula><mml:math id="M18" display="inline"><mml:mrow><mml:msup><mml:mi>L</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula> norm for
a stand-alone model. The norms are created for the entire GrIS and several
regions of interest, which are those that highlight the Jakobshavn,
Zachariae, and Petermann glaciers. Figure <xref ref-type="fig" rid="Ch1.F4"/> is focused
around drainage basins 7 and 8 (see Fig. <xref ref-type="fig" rid="Ch1.F1"/> for reference) to
include the Jakobshavn glacier.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F4" specific-use="star"><label>Figure 4</label><caption><p id="d1e1096">The norm of the surface velocity field (m s<inline-formula><mml:math id="M19" 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>, given by the
color bars) from initialization <xref ref-type="bibr" rid="bib1.bibx16 bib1.bibx17" id="paren.65"/> <bold>(a)</bold>,
CISM-A <bold>(b)</bold>, and the difference <bold>(c)</bold> over drainage basins 7 and 8 as indicated by
Fig. <xref ref-type="fig" rid="Ch1.F1"/>.</p></caption>
          <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://gmd.copernicus.org/articles/12/1067/2019/gmd-12-1067-2019-f04.png"/>

        </fig>

</sec>
<sec id="Ch1.S4.SS2">
  <title>Coupled-model analysis</title>
      <p id="d1e1138">Land ice behavior is critically dependent on various forcings from the
atmosphere and land surface, so analyses of these fields within a coupled
model comprise a significant portion of LIVVkit validation. LIVVkit also
targets the land ice component within a coupled simulation using the same
analysis procedures described in Sect. <xref ref-type="sec" rid="Ch1.S4.SS1"/> for a stand-alone
land ice model, if that component is active. As with the stand-alone
analysis, LIVVkit presents area-averaged climatological fields in tabular
form for a “quick look” overview applied to the CESM simulation and
RACMO2.3 comparison data, as shown in Table <xref ref-type="table" rid="Ch1.T2"/>. When applying
the GrIS mask for averaging, the variables are multiplied by the percent of
grid cell that is land ice, which is constant for the CESM simulation. Within
the land model component, the downwelling and net shortwave (SW<inline-formula><mml:math id="M20" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">d</mml:mi></mml:msub></mml:math></inline-formula>
and SW<inline-formula><mml:math id="M21" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">net</mml:mi></mml:msub></mml:math></inline-formula>) and longwave (LW<inline-formula><mml:math id="M22" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">d</mml:mi></mml:msub></mml:math></inline-formula> and LW<inline-formula><mml:math id="M23" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">net</mml:mi></mml:msub></mml:math></inline-formula>) radiation,
respectively, the net surface radiation, <inline-formula><mml:math id="M24" display="inline"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">net</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, the turbulent
sensible and latent heat fluxes (SHFs and LHFs), and the SMB are all
summarized. From the atmosphere component, the 2 m air temperature (T2m) is
presented. Here, LIVVkit produces identical results for CESM output as in V13
except for the SMB, because LIVVkit uses monthly averaged values of the ice
growth/melt (QICE) field.</p>

<?xmltex \floatpos{t}?><table-wrap id="Ch1.T2"><label>Table 2</label><caption><p id="d1e1196">Area-weighted and GrIS-masked climatologies for a host of key land
surface variables from CESM's land surface and atmosphere components for
summer (JJA), except SMB, which is an annual climatology, compared to
RACMO2.3 values. All variables are in W m<inline-formula><mml:math id="M25" 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> except SMB
(kg m<inline-formula><mml:math id="M26" 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> a<inline-formula><mml:math id="M27" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>) and T2m (<inline-formula><mml:math id="M28" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C).</p></caption><oasis:table frame="topbot"><oasis:tgroup cols="3">
     <oasis:colspec colnum="1" colname="col1" align="left"/>
     <oasis:colspec colnum="2" colname="col2" align="right"/>
     <oasis:colspec colnum="3" colname="col3" align="right"/>
     <oasis:thead>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1">Data</oasis:entry>
         <oasis:entry colname="col2">CESM</oasis:entry>
         <oasis:entry colname="col3">RACMO2.3</oasis:entry>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row>
         <oasis:entry colname="col1">SW<inline-formula><mml:math id="M29" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">d</mml:mi></mml:msub></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col2">268</oasis:entry>
         <oasis:entry colname="col3">301</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">SW<inline-formula><mml:math id="M30" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">net</mml:mi></mml:msub></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col2">61</oasis:entry>
         <oasis:entry colname="col3">58</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">LW<inline-formula><mml:math id="M31" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">d</mml:mi></mml:msub></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col2">235</oasis:entry>
         <oasis:entry colname="col3">224</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">LW<inline-formula><mml:math id="M32" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">net</mml:mi></mml:msub></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col2"><inline-formula><mml:math id="M33" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">46</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3"><inline-formula><mml:math id="M34" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">52</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1"><inline-formula><mml:math id="M35" display="inline"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">net</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col2">15</oasis:entry>
         <oasis:entry colname="col3">5.5</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">SHF</oasis:entry>
         <oasis:entry colname="col2">7</oasis:entry>
         <oasis:entry colname="col3">8</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">LHF</oasis:entry>
         <oasis:entry colname="col2"><inline-formula><mml:math id="M36" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">8</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3"><inline-formula><mml:math id="M37" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">6</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">SMB</oasis:entry>
         <oasis:entry colname="col2">209</oasis:entry>
         <oasis:entry colname="col3">238</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">T2m</oasis:entry>
         <oasis:entry colname="col2"><inline-formula><mml:math id="M38" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">20.6</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3"><inline-formula><mml:math id="M39" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">21.9</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup></oasis:table></table-wrap>

      <p id="d1e1471">The variables summarized in Table <xref ref-type="table" rid="Ch1.T2"/> are also presented as
contour plots over GrIS to highlight regional differences from RACMO2.3.
Annualized and/or seasonal fields (as appropriate) from land surface and
atmosphere are provided for the model, RACMO2.3, and the difference, where
RACMO2.3 is interpolated to the CESM grid. The summer LW<inline-formula><mml:math id="M40" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">net</mml:mi></mml:msub></mml:math></inline-formula> in
CESM is presented in Fig. <xref ref-type="fig" rid="Ch1.F5"/> as an example and shows that
although the model is able to capture the general spatial variation and
minimum values near the NE coast, there are overly large values (less heat
loss) near the center of the land ice.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F5" specific-use="star"><label>Figure 5</label><caption><p id="d1e1490">Summer net longwave radiation (W m<inline-formula><mml:math id="M41" 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>) for CESM <bold>(a)</bold>,
RACMO2.3 <bold>(b)</bold>, and the difference <bold>(c)</bold>. The black solid lines
denote elevation at 0, 1000, 2000, and 3000 km levels in each grid. The CESM
elevation <bold>(b, c)</bold> uses the 5 km downscaled
values.</p></caption>
          <?xmltex \igopts{width=369.885827pt}?><graphic xlink:href="https://gmd.copernicus.org/articles/12/1067/2019/gmd-12-1067-2019-f05.png"/>

        </fig>

      <p id="d1e1523">Contour and scatter plots of climatological atmospheric 2 m height
temperature are also provided for polar summer<?pagebreak page1075?> (JJA) and winter (DJF) in
LIVVkit; a contour plot for JJA is shown in Fig. <xref ref-type="fig" rid="Ch1.F6"/>. The
near-surface temperature is critical to track in a coupled model because it drives
the processes of surface melt and refreezing.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F6" specific-use="star"><label>Figure 6</label><caption><p id="d1e1530">Averages for the JJA season of surface temperature over the GrIS for
CESM <bold>(a)</bold>, RACMO2.3 <bold>(b)</bold>, and CESM-RACMO2.3 <bold>(c)</bold>.
Elevation contours are as in Fig. <xref ref-type="fig" rid="Ch1.F5"/>.</p></caption>
          <?xmltex \igopts{width=369.885827pt}?><graphic xlink:href="https://gmd.copernicus.org/articles/12/1067/2019/gmd-12-1067-2019-f06.png"/>

        </fig>

      <p id="d1e1550">The representation of clouds over GrIS in the coupled model is also evaluated
in LIVVkit because they contribute to the surface energy budget and related
processes such as surface melting and refreezing <xref ref-type="bibr" rid="bib1.bibx58" id="paren.66"/>. The
comparisons provided by LIVVkit include the annual cycle of monthly averaged
low, high, and total clouds for both the model and ISCCP and CLOUDSAT
observationally derived datasets and contour plots of annual and seasonal
averages of low, high, and total cloud amount. For the annual cycles, the data
are area averaged over the GrIS region for each month of the climatology.
Several examples of the cloud analysis as applied to CESM are displayed in
Figs. <xref ref-type="fig" rid="Ch1.F7"/> and <xref ref-type="fig" rid="Ch1.F8"/>. The ISCCP and CLOUDSAT
monthly averages over GrIS in Fig. <xref ref-type="fig" rid="Ch1.F7"/> exhibit a seasonal
cycle, which is consistent with findings over the entire Arctic<?pagebreak page1077?> <xref ref-type="bibr" rid="bib1.bibx7" id="paren.67"/>.
However, the CESM produces total clouds that are considerably too few and
capture no summer minimum, also consistent with noted CESM biases observed
for the whole Arctic region <xref ref-type="bibr" rid="bib1.bibx5" id="paren.68"/>. This bias is not universal for
all cloud levels; Fig. <xref ref-type="fig" rid="Ch1.F8"/> shows that the annual values of
low clouds more closely match CLOUDSAT than ISCCP (although the seasonal
cycle is opposite that from observations, with a summer maximum; not shown). These
plots indicate the need for a deeper investigation. Recent efforts to
understand the limitations of both models and observed and reanalysis
datasets in representing clouds over the Arctic (e.g., <xref ref-type="bibr" rid="bib1.bibx7 bib1.bibx26" id="altparen.69"/>),
and focused over Greenland <xref ref-type="bibr" rid="bib1.bibx14" id="paren.70"/>, provide a good starting point.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F7"><label>Figure 7</label><caption><p id="d1e1579">Climatological monthly averages of total clouds over the GrIS region
for CESM (red), ISCCP <xref ref-type="bibr" rid="bib1.bibx48" id="paren.71"/> (green), and CLOUDSAT <xref ref-type="bibr" rid="bib1.bibx18" id="paren.72"/>
(cyan).</p></caption>
          <?xmltex \igopts{width=213.395669pt}?><graphic xlink:href="https://gmd.copernicus.org/articles/12/1067/2019/gmd-12-1067-2019-f07.png"/>

        </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F8" specific-use="star"><label>Figure 8</label><caption><p id="d1e1597">Climatological annual average of low clouds (%) over the GrIS for
CESM <bold>(a)</bold>, ISCCP <xref ref-type="bibr" rid="bib1.bibx48" id="paren.73"/> <bold>(b)</bold>, and CLOUDSAT
<xref ref-type="bibr" rid="bib1.bibx18" id="paren.74"/> <bold>(c)</bold>. The downscaled CESM values are used for all
elevation contours.</p></caption>
          <?xmltex \igopts{width=369.885827pt}?><graphic xlink:href="https://gmd.copernicus.org/articles/12/1067/2019/gmd-12-1067-2019-f08.png"/>

        </fig>

      <p id="d1e1621">Similar to Fig. <xref ref-type="fig" rid="Ch1.F2"/> for CISM-A, LIVVkit produces a contour
plot of ice-sheet-wide SMB compared to RACMO2.3 (not shown). For the coupled
simulation, a times series for the area-averaged values over GrIS covering
the entire range of a simulation is provided by LIVVkit, as in
Fig. <xref ref-type="fig" rid="Ch1.F9"/> for CESM. The values are calculated with
the same methodology as with the SMB in Table <xref ref-type="table" rid="Ch1.T2"/>, except for
the time averaging.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F9"><label>Figure 9</label><caption><p id="d1e1632">Times series of the (blue) CESM surface mass balance for the entire
simulation, 1851–2006, compared to the (orange) RACMO 2.3 surface mass
balance.</p></caption>
          <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://gmd.copernicus.org/articles/12/1067/2019/gmd-12-1067-2019-f09.png"/>

        </fig>

      <p id="d1e1641">To break down climatological behavior of the time series and quantify the
variability, a box plot of the SMB time series is provided, as shown in
Fig. <xref ref-type="fig" rid="Ch1.F10"/> for CESM and RACMO2.3. In this plot, the
rectangle spans the 25 % quartile to the 75 % quartile (the
interquartile range, or IQR) of the time series with the median shown as the
red line in the rectangle. The two whiskers represent <inline-formula><mml:math id="M42" display="inline"><mml:mrow><mml:mn mathvariant="normal">1.5</mml:mn><mml:mo>×</mml:mo></mml:mrow></mml:math></inline-formula> IQR above
the 75 % quartile and below the 25 % quartile, respectively. The
diamonds outside the whiskers are suspected outliers. In
Fig. <xref ref-type="fig" rid="Ch1.F9"/>, the extent of the whiskers is similar
for CESM and RACMO23, so the model data have similar variability compared to
RACMO2.3. However, the slightly smaller and lower IQR box for the RACMO2.3
data indicates that its data are slightly less variable and skewed low. Given
the smaller dataset size of RACMO2.3, this result is not surprising.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F10"><label>Figure 10</label><caption><p id="d1e1660">Box plot of <bold>(a)</bold> CESM annual surface mass balance for the
entire simulation, 1851–2006, compared to the <bold>(b)</bold> RACMO 2.3 annual
surface mass balance for 1961–2013. The diamonds represent extreme values
within the series as explained in the text.</p></caption>
          <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://gmd.copernicus.org/articles/12/1067/2019/gmd-12-1067-2019-f10.png"/>

        </fig>

</sec>
<sec id="Ch1.S4.SS3">
  <title>Basin scale SMB analysis</title>
      <?pagebreak page1078?><p id="d1e1681">The increasing availability of SMB observational data outlined in
Sect. <xref ref-type="sec" rid="Ch1.S2"/> presents an opportunity to delve into the quality of
simulated SMB. With this in mind, LIVVkit provides analyses of the SMB by
basin and elevation using these data, applied here to the CESM SMB values
that have been downscaled to 5 km within the land ice component. A LIVVkit
contour plot of the CESM SMB, overlain by circles representing the observed
data locations (as in Fig. <xref ref-type="fig" rid="Ch1.F1"/>), is shown in Fig. <xref ref-type="fig" rid="Ch1.F11"/>.
This figure is similar to Fig. 7 of V13 but includes
more recently available data. The colors within the circles represent SMB
estimates based on snow pit and/or firn/ice core studies.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F11"><label>Figure 11</label><caption><p id="d1e1692">Filled contours of the annual SMB of the Greenland land ice as
modeled by CESM, with pit/core field estimates overlaid as filled circles.
Data were compiled as detailed in Sect. <xref ref-type="sec" rid="Ch1.S2"/> from both ablation and
accumulation zones.</p></caption>
          <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://gmd.copernicus.org/articles/12/1067/2019/gmd-12-1067-2019-f11.png"/>

        </fig>

      <?pagebreak page1079?><p id="d1e1703">To provide more quantitative comparisons, these data are also presented as a
histogram of differences between modeled and observed annual surface mass
balance values at pit/core locations where data exist. It is shown for the
entire GrIS in Fig. <xref ref-type="fig" rid="Ch1.F12"/> and for each of the eight basins
delineated in Figs. <xref ref-type="fig" rid="Ch1.F1"/> and <xref ref-type="fig" rid="Ch1.F13"/>. Observational
data for Figs. <xref ref-type="fig" rid="Ch1.F12"/> and <xref ref-type="fig" rid="Ch1.F13"/> were compiled and
processed by LIVVkit from the pit/core data as described in
Sect. <xref ref-type="sec" rid="Ch1.S2"/>. The vertical light blue line denotes the 0 difference
line for model vs. observed data; values above (below) this line indicate
that the model overestimates (underestimates) SMB in comparison to altimetry
observations. High frequencies near zero imply greater model agreement. Note
that because this plot compares nearest-neighbor values without any spatial
interpolation, one coarse model cell may be compared to multiple (if not
many) observed SMB estimates, because the data collection sites are often
located in clusters. The correspondence of model to observational data varies
significantly by basin and shows better agreement in the central latitude
regions as compared to the southern and northern regions. V13 showed lower
values of SMB over region 4 for CESM relative to RACMO2.0, but in fact CESM
is rather close to observations in this region. Consistent with this, RACMO
version 2.3 exhibits a significant decrease in precipitation <xref ref-type="bibr" rid="bib1.bibx37" id="paren.75"/>,
apparently bringing its SMB closer to observations. LIVVkit also provides
plots similar to those in Figs. <xref ref-type="fig" rid="Ch1.F12"/> and <xref ref-type="fig" rid="Ch1.F13"/>
but with comparison to the IceBridge data.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F12"><label>Figure 12</label><caption><p id="d1e1729">Histogram of differences between modeled and observed annual SMB, at
all collected pit/core locations as detailed in Sect. <xref ref-type="sec" rid="Ch1.S2"/> from
ablation and accumulation zones. The light blue line highlights 0 difference
between model and observed; values above (below) this line indicate that the
model overestimates (underestimates) SMB in comparison to the
observations.</p></caption>
          <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://gmd.copernicus.org/articles/12/1067/2019/gmd-12-1067-2019-f12.png"/>

        </fig>

      <?xmltex \floatpos{p}?><fig id="Ch1.F13" specific-use="star"><label>Figure 13</label><caption><p id="d1e1742">As in Fig. <xref ref-type="fig" rid="Ch1.F12"/> but broken down into basins as marked
in Fig. <xref ref-type="fig" rid="Ch1.F1"/>. Axes have been normalized for the eight drainage
histograms to highlight differences between the number of comparison points
per basin.</p></caption>
          <?xmltex \igopts{width=284.527559pt}?><graphic xlink:href="https://gmd.copernicus.org/articles/12/1067/2019/gmd-12-1067-2019-f13.png"/>

        </fig>

      <p id="d1e1755">Scatter plots comparing CESM to the SMB estimates from pit/core data and
IceBridge areal estimates, separating accumulation and ablation zones and
colored by basin, are also provided by LIVVkit.
Figure <xref ref-type="fig" rid="Ch1.F14"/>, which shows pit/core data, demonstrates that
CESM is currently not able to capture the SMB well in the ablation areas of
basin 6 (gray, the southwest GrIS). Figure <xref ref-type="fig" rid="Ch1.F13"/> shows this
bias as well. Separating ablation from accumulation provides the source of
bias: the overly positive SMB in region 6, and overall, is due to too little
ablation relative to observations, not too much accumulation.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F14" specific-use="star"><label>Figure 14</label><caption><p id="d1e1764">CESM annual SMB vs. observed estimates at locations taken from
accumulation <bold>(a)</bold> and ablation zones <bold>(b)</bold>. Observational data
were compiled as detailed in Sect. <xref ref-type="sec" rid="Ch1.S2"/>. In both figures, colors
correspond to the eight major drainage basins, as shown in
Fig. <xref ref-type="fig" rid="Ch1.F1"/>, and the <inline-formula><mml:math id="M43" display="inline"><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mo>:</mml:mo><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:math></inline-formula> line is drawn in
blue.</p></caption>
          <?xmltex \igopts{width=384.112205pt}?><graphic xlink:href="https://gmd.copernicus.org/articles/12/1067/2019/gmd-12-1067-2019-f14.png"/>

        </fig>

      <p id="d1e1797">While SMB comparisons by basin are helpful, model biases in elevation can
provide clues as to the source. Figure <xref ref-type="fig" rid="Ch1.F15"/> presents CESM
and observed SMB over accumulation and ablation regions vs. their elevation,
and colored by basin, so that model developers are able to identify areas
where there is an elevation mismatch. Because the model and observed data are
not co-located, their horizontal locations are different. The observed data
show a strong positive linear relationship between SMB and elevation up to
about 1500 m, above which almost all points (except several in basin 1) have
a positive SMB. The model is also able to capture this characteristic;
however, the linear relationship is more diffuse, and the linear increase in
ablation with decreasing elevation is too weak in CESM in basin 6 of the
GrIS. Referring back to Fig. <xref ref-type="fig" rid="Ch1.F6"/>, the temperature gradient from
the higher central part of GrIS to the edges is slightly weaker in CESM than
RACMO2.3 in summer (and even more so in winter; not shown), with colder
temperatures at the edges, which is consistent with the slope of elevation
vs. SMB shown in Fig. <xref ref-type="fig" rid="Ch1.F15"/>.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F15" specific-use="star"><label>Figure 15</label><caption><p id="d1e1809">Field estimates of annual SMB as a function of observed
elevation <bold>(a)</bold> and CESM annual SMB as a function of model
elevation <bold>(b)</bold> from both accumulation and ablation zones. For the
observed data, the size of the point represents the number of years in the
field record, with larger points containing comparatively more temporal
information than smaller points, and each point represents an annual surface
mass balance estimate averaged across at least 1 year of data. For the
modeled data, each point represents a model cell containing an available
field estimate location. In both figures, colors correspond to the drainage
basins as shown in Fig. <xref ref-type="fig" rid="Ch1.F1"/>.</p></caption>
          <?xmltex \igopts{width=369.885827pt}?><graphic xlink:href="https://gmd.copernicus.org/articles/12/1067/2019/gmd-12-1067-2019-f15.png"/>

        </fig>

      <?pagebreak page1081?><p id="d1e1826">LIVVkit breaks down the model vs. elevation data comparison along several key
transects in the ablation zone, and Fig. <xref ref-type="fig" rid="Ch1.F16"/> shows that
for CESM, all four transects contain some mismatch, but the Qammanarssup Sermia
and Kangerlussuaq (K) transects (basin 6) echo the overly weak modeled slope
of elevation vs. SMB ablation as seen in Fig. <xref ref-type="fig" rid="Ch1.F15"/>. As for
the accumulation zone, LIVVkit's processed IceBridge transect data are
presented as contours by location in the GrIS along with model vs. observed
data in Fig. <xref ref-type="fig" rid="Ch1.F17"/>. The CESM bias has a latitudinal
gradient; SMB is overestimated (e.g., basin 2) compared to annual IceBridge
estimates in the northern half of the GrIS and the bias decreases going
south, becoming too low relative to the observed data in the southern half.
The source of this bias could be analyzed within the context of temperature,
cloud cover, precipitation, and latent and sensible heat fluxes using figures
such as Figs. <xref ref-type="fig" rid="Ch1.F8"/> and <xref ref-type="fig" rid="Ch1.F5"/>, but covering the
relevant seasons, but that is beyond the scope of this survey.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F16" specific-use="star"><label>Figure 16</label><caption><p id="d1e1841">Annual surface mass balance as a function of observed elevation at
four different areas in the ablation zone of GrIS. Red dots are modeled SMB
and elevation, while blue dots are observed SMB and elevation from pit/core
field estimates. Observational data were compiled from the PROMICE database
<xref ref-type="bibr" rid="bib1.bibx31" id="paren.76"/>.</p></caption>
          <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://gmd.copernicus.org/articles/12/1067/2019/gmd-12-1067-2019-f16.png"/>

        </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F17" specific-use="star"><label>Figure 17</label><caption><p id="d1e1855">Observed annual surface mass balance of GrIS along IceBridge
altimetry transects <bold>(a)</bold> and the differences between the observations
and model along the transects <bold>(b)</bold>.</p></caption>
          <?xmltex \igopts{width=369.885827pt}?><graphic xlink:href="https://gmd.copernicus.org/articles/12/1067/2019/gmd-12-1067-2019-f17.png"/>

        </fig>

</sec>
</sec>
<sec id="Ch1.S5" sec-type="conclusions">
  <title>Conclusions</title>
      <p id="d1e1877">An initial capability to perform automated
validation of land ice and coupled models is presented, and we encourage the
land ice modeling and larger computational Earth sciences community to bring
additional tools and analysis to improve the software from this baseline. For
example, generalization of the software to use with other models and the
inclusion of more data are top priorities. Although LIVVkit targets some
aspects of relevant variables that affect land ice models within the coupled
Earth system model as detailed above, there are additional analyses that
could deliver useful information for both model developers and analysts. One
example is to provide seasonal and long-term SMB trends for information about
model stability and forcings. Specifically, seasonal (summer) SMB estimates
relative to the PROMICE dataset, which we currently only show as annualized
values, could be extended. Extensions to assess the Antarctic ice sheet (AIS)
are also greatly needed and are a near-term priority. The recent release of
Quantarctica, version
3<fn id="Ch1.Footn2"><p id="d1e1880"><uri>https://www.pgc.umn.edu/news/quantarctica-version-3-released/</uri>,
last access: 5 March 2019</p></fn>, provides a collection of ice cores to consider
for inclusion in LIVVkit.</p>
      <p id="d1e1886">Beyond new capabilities, additional observational data from both current and
new sources would provide more information and build model confidence, for
example, the Landsat 8 GoLIVE global ice velocity data derived from Landsat
8<fn id="Ch1.Footn3"><p id="d1e1889"><uri>https://nsidc.org/data/golive</uri>, last access: 5 March 2019</p></fn>
with 300 m spacing, error and quality parameters, and subannual, and in some
cases monthly or less, time periods. A recent synthesis of modeled and
remotely sensed inferences of the basal thermal state of GrIS
<xref ref-type="bibr" rid="bib1.bibx30" id="paren.77"/> would provide a starting point for comparison temperature
data. Additional SMB data to consider include data values from Airborne
SAR/Interferometric Radar Altimeter System (ASIRAS) airborne radar and
neutron-probe density measurements <xref ref-type="bibr" rid="bib1.bibx43" id="paren.78"/> and longer records from
specific regions to better analyze time series behavior, e.g.,
<xref ref-type="bibr" rid="bib1.bibx57" id="text.79"/>. <xref ref-type="bibr" rid="bib1.bibx31" id="text.80"/> provide a history of SMB observations
as a “state of the art” that can be used as a baseline for extension.
Another source for additional SMB data, the Surface Mass Balance and Snow on
Sea Ice Working Group <xref ref-type="bibr" rid="bib1.bibx52" id="paren.81"/>, compiles flights and ice snow
pit/ice core data that include PARCA cores which were included in LIVVkit as
mentioned above, as well as aerial flights from both Greenland and
Antarctica. The IceBridge dataset also included in LIVVkit uses the more
recent 2013–2014 flights; however, earlier flights as detailed in
<xref ref-type="bibr" rid="bib1.bibx23" id="text.82"/> would provide more comparison within the ablation zone.</p>
      <p id="d1e1914">Next steps for LIVVkit being pursued include a connection to the CmCt
validation framework that compares ice sheet models to altimetry and
gravimetry satellite observations from the Ice, Cloud, and land Elevation
Satellite (ICESat) and Gravity Recovery and Climate Experiment (GRACE)
<xref ref-type="bibr" rid="bib1.bibx47" id="paren.83"/>. The substantial postprocessing required to compare the model
with observations would complement the other metrics presented here, as an
opt-in feature. Performance validation, which would expand from an initial
computational verification capability as presented in <xref ref-type="bibr" rid="bib1.bibx20" id="text.84"/>, is
underway; the goals are to track model computational behavior on
high-performance computers. Efforts to enable LIVVkit's kernels, the Extended<?pagebreak page1083?> V&amp;V
for Earth Systems (EVE), to handle ensembles of output and provide
sensitivities of variables to perturbed initial conditions are also being
pursued, targeting verification using short ensembles of climate model
configurations (e.g., <xref ref-type="bibr" rid="bib1.bibx32" id="altparen.85"/>). Future work to develop and deploy
uncertainty quantification techniques using LIVVkit within a larger ensemble-based workflow would enable more robust uncertainty information regarding
climate projections.</p>
      <p id="d1e1926">Several challenges exist in deploying LIVVkit for large-scale multimodel
validation. There are several efforts we recommend for improved verification
and validation in general, and to make LIVVkit more robust and extensible.
Using common model projections and data conventions would allow many
different models to participate in LIVVkit postprocessing with minimal code
changes and other related information such as external mask and areal
information, etc. Some accepted protocol should be developed for LIVVkit to
postprocess the data automatically. The land ice community is a relative
newcomer within the coupled Earth system model community, so adoption of
already accepted formats in use by other components would facilitate this
transition. In any case, the breadth of ice sheet model development has
created an opportunity to provide critically important simulations to the
climate community, and this validation package is a step toward a predictive
capability for land ice models, both on their own and coupled to a global
Earth system model.</p><?xmltex \hack{\newpage}?>
</sec>

      
      </body>
    <back><notes notes-type="codedataavailability"><title>Code and data availability</title>

      <p id="d1e1934">The LIVVkit version 2.1 source code and documentation
<xref ref-type="bibr" rid="bib1.bibx21" id="paren.86"/> are available via a modified BSD license at
<uri>https://github.com/LIVVkit/LIVVkit</uri> (last access: 5 March 2019) and
<uri>https://livvkit.github.io/Docs</uri> (last access: 5 March 2019),
respectively. The reader can access all the datasets and reproduce all the
analyses presented here with LEX <xref ref-type="bibr" rid="bib1.bibx22" id="paren.87"/>, which is available via a
modified BSD license at <uri>https://code.ornl.gov/LIVVkit/lex</uri> (last access:
5 March 2019) and is documented in the LIVVkit documentation. More details
about data and code access are provided in Sects. <xref ref-type="sec" rid="Ch1.S2"/>
and <xref ref-type="sec" rid="Ch1.S3"/>, respectively.</p>
  </notes><notes notes-type="authorcontribution"><title>Author contributions</title>

      <p id="d1e1960">KJE wrote most of the paper and performed some of the
postprocessing. JHK led the software strategy and development of LIVVkit and
other related repositories, and performed some of the postprocessing and
visualization. MMF collected the SMB data and performed the basin SMB
postprocessing. DL and AB wrote some postprocessing and LIVVkit code. SP and
MH advised on the appropriate ice sheet metrics. JF, MV, and IT advised on
and provided example target model data and advised on appropriate metrics. CZ
developed NCO for LIVVkit needs and advised on postprocessing. All authors
edited the manuscript.</p>
  </notes><notes notes-type="competinginterests"><title>Competing interests</title>

      <p id="d1e1966">The authors declare that they have no conflict of
interest.</p>
  </notes><ack><title>Acknowledgements</title><?pagebreak page1084?><p id="d1e1972">Support for this work was provided through Scientific Discovery through
Advanced Computing (SciDAC) program funded by the US Department of Energy
Office of Advanced Scientific Computing Research and Office of Biological and
Environmental Research. This paper has been authored by UT-Battelle, LLC
and used resources of the National Center for Computational Sciences at Oak
Ridge National Laboratory, both of which are supported by the Office of
Science of the US Department of Energy under contract
no. DE-AC05-00OR22725. Contributions of Charles S. Zender were made possible by support from DOE
E3SM DE-SC0012998 and NASA ACCESS NNX14AH55A. Miren Vizcaíno
acknowledges support the European Research Council
ERC-StG-678145-CoupledIceClim. The United States Government retains and the
publisher, by accepting the article for publication, acknowledges that the
United States Government retains a non-exclusive, paid-up, irrevocable,
world-wide license to publish or reproduce the published form of this
paper, or allow others to do so, for United States Government
purposes.<?xmltex \hack{\newline}?><?xmltex \hack{\newline}?>
Edited by: Didier Roche <?xmltex \hack{\newline}?>
Reviewed by: two anonymous referees</p></ack><ref-list>
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    <!--<article-title-html>LIVVkit 2.1: automated and extensible ice sheet model validation</article-title-html>
<abstract-html><p>A collection of scientific analyses, metrics, and visualizations for robust
validation of ice sheet models is presented using the Land Ice Verification
and Validation toolkit (LIVVkit), version 2.1, and the LIVVkit Extensions
repository (LEX), version 0.1. This software collection targets stand-alone
ice sheet or coupled Earth system models, and handles datasets and analyses
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efficient and fully reproducible workflows for postprocessing, analysis, and
visualization of observational and model-derived datasets in a shareable
format, whereby all data, methodologies, and output are distributed to users
for evaluation. Extending from the initial LIVVkit software framework, we
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coupled Community Earth System Model (CESM) as well as an idealized
stand-alone high-resolution Community Ice Sheet Model, version 2 (CISM2),
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bias, using recently available in situ and remotely sensed data as
comparison. Related fields within atmosphere and land surface models, e.g.,
surface temperature, radiation, and cloud cover, are also diagnosed. Applied
to the CESM1.0, LIVVkit identifies a positive SMB bias that is focused
largely around Greenland's southwest region that is due to insufficient
ablation.</p></abstract-html>
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