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  <front>
    <journal-meta><journal-id journal-id-type="publisher">TC</journal-id><journal-title-group>
    <journal-title>The Cryosphere</journal-title>
    <abbrev-journal-title abbrev-type="publisher">TC</abbrev-journal-title><abbrev-journal-title abbrev-type="nlm-ta">The Cryosphere</abbrev-journal-title>
  </journal-title-group><issn pub-type="epub">1994-0424</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/tc-14-2869-2020</article-id><title-group><article-title>New gravity-derived bathymetry for the Thwaites, Crosson, and Dotson ice
shelves revealing two ice shelf populations</article-title><alt-title>Gravity-derived bathymetry adjacent to the Thwaites Glacier system</alt-title>
      </title-group><?xmltex \runningtitle{Gravity-derived bathymetry adjacent to the Thwaites Glacier system}?><?xmltex \runningauthor{T. A. Jordan et al.}?>
      <contrib-group>
        <contrib contrib-type="author" corresp="yes" rid="aff1">
          <name><surname>Jordan</surname><given-names>Tom A.</given-names></name>
          <email>tomj@bas.ac.uk</email>
        <ext-link>https://orcid.org/0000-0003-2780-1986</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2">
          <name><surname>Porter</surname><given-names>David</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2">
          <name><surname>Tinto</surname><given-names>Kirsty</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff3">
          <name><surname>Millan</surname><given-names>Romain</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff4">
          <name><surname>Muto</surname><given-names>Atsuhiro</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Hogan</surname><given-names>Kelly</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-1256-8010</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Larter</surname><given-names>Robert D.</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-8414-7389</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff5">
          <name><surname>Graham</surname><given-names>Alastair G. C.</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff6">
          <name><surname>Paden</surname><given-names>John D.</given-names></name>
          
        <ext-link>https://orcid.org/0000-0003-0775-6284</ext-link></contrib>
        <aff id="aff1"><label>1</label><institution>British Antarctic Survey, High Cross, Madingley Road, Cambridge, CB3 0ET, UK</institution>
        </aff>
        <aff id="aff2"><label>2</label><institution>Lamont-Doherty Earth Observatory, Columbia University, Palisades, NY, 10964-8000, USA</institution>
        </aff>
        <aff id="aff3"><label>3</label><institution>Institut des Géosciences de l'Environnement, Université
Grenoble Alpes, CNRS, 38000 Grenoble, France</institution>
        </aff>
        <aff id="aff4"><label>4</label><institution>Dept. of Earth and Environmental Science, Temple University,
Philadelphia, PA 19122, USA</institution>
        </aff>
        <aff id="aff5"><label>5</label><institution>College of Marine Science, University of South Florida, St
Petersburg, FL 33701, USA</institution>
        </aff>
        <aff id="aff6"><label>6</label><institution>Center for Remote Sensing of Ice Sheets (CReSIS), The University of
Kansas, KS 66045, USA</institution>
        </aff>
      </contrib-group>
      <author-notes><corresp id="corr1">Tom A. Jordan (tomj@bas.ac.uk)</corresp></author-notes><pub-date><day>9</day><month>September</month><year>2020</year></pub-date>
      
      <volume>14</volume>
      <issue>9</issue>
      <fpage>2869</fpage><lpage>2882</lpage>
      <history>
        <date date-type="received"><day>29</day><month>November</month><year>2019</year></date>
           <date date-type="rev-request"><day>10</day><month>January</month><year>2020</year></date>
           <date date-type="rev-recd"><day>1</day><month>June</month><year>2020</year></date>
           <date date-type="accepted"><day>17</day><month>June</month><year>2020</year></date>
      </history>
      <permissions>
        <copyright-statement>Copyright: © 2020 </copyright-statement>
        <copyright-year>2020</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://tc.copernicus.org/articles/.html">This article is available from https://tc.copernicus.org/articles/.html</self-uri><self-uri xlink:href="https://tc.copernicus.org/articles/.pdf">The full text article is available as a PDF file from https://tc.copernicus.org/articles/.pdf</self-uri>
      <abstract><title>Abstract</title>
    <p id="d1e188">Ice shelves play a critical role in the long-term
stability of ice sheets through their buttressing effect. The underlying
bathymetry and cavity thickness are key inputs for modelling future ice
sheet evolution. However, direct observation of sub-ice-shelf bathymetry is
time-consuming, logistically risky, and in some areas simply not possible.
Here we use new compilations of airborne and marine gravity, radar depth
sounding, and swath bathymetry to provide new estimates of sub-ice-shelf
bathymetry outboard of the rapidly changing West Antarctic Thwaites Glacier
and beneath the adjacent Dotson and Crosson ice shelves. This region is of
special interest, as the low-lying inland reverse slope of the Thwaites
Glacier system makes it vulnerable to marine ice sheet instability, with
rapid grounding line retreat observed since 1993 suggesting this process may
be underway. Our results confirm a major marine channel <inline-formula><mml:math id="M1" display="inline"><mml:mrow><mml:mo>&gt;</mml:mo><mml:mn mathvariant="normal">800</mml:mn></mml:mrow></mml:math></inline-formula> m
deep extends tens of kilometres to the front of Thwaites Glacier, while the
adjacent ice shelves are underlain by more complex bathymetry. Comparison of
our new bathymetry with ice shelf draft reveals that ice shelves formed
since 1993 comprise a distinct population where the draft conforms closely
to the underlying bathymetry, unlike the older ice shelves, which show a more
uniform depth of the ice base. This indicates that despite rapid basal
melting in some areas, these recently floated parts of the ice shelf are not
yet in dynamic equilibrium with their retreated grounding line positions and
the underlying ocean system, a factor which must be included in future
models of this region's evolution.</p>
  </abstract>
    </article-meta>
  </front>
<body>
      

<sec id="Ch1.S1" sec-type="intro">
  <label>1</label><title>Introduction</title>
      <p id="d1e210">The Thwaites Glacier system is a globally important region of change in the
cryosphere system (Fig. 1a)
(Scambos et al., 2017). In
this region the marine based West Antarctic Ice Sheet comes into direct
contact with upwelling modified Circumpolar Deep Water (mCDW), which is warm
relative to the typical cool dense shelf water on Antarctic continental
shelves (Jenkins et al., 2018). This warm water can both erode the
buttressing ice shelves and directly melt the grounded ice, both factors
driving dynamic thinning and retreat of glaciers and contributing to rising
global sea level (Pritchard et al., 2012). The inland reverse slope of the
bed beneath Thwaites Glacier and some of the adjacent glaciers means that
marine ice sheet instability may occur  (Schoof, 2007; Weertman,
1974). In this case a feedback is setup where grounding line retreat exposes
a progressively larger cross-sectional area of ice; hence, more ice fluxes
into the ocean leading to further glacial retreat. Satellite observations
revealing an increase in the velocity of <inline-formula><mml:math id="M2" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">100</mml:mn></mml:mrow></mml:math></inline-formula> ma<inline-formula><mml:math id="M3" 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>
extending <inline-formula><mml:math id="M4" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">100</mml:mn></mml:mrow></mml:math></inline-formula> km inland from the Thwaites grounding line and a
surface draw down of over 1 ma<inline-formula><mml:math id="M5" 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> indicate that this region is changing
now (Gardner et al., 2018; Milillo et al., 2019).<?pagebreak page2870?> It has been argued that
the dramatic retreat of the grounding lines of Thwaites, Pope, Smith, and Kohler
glaciers of between 10 and 30 km since 1993 (Fig. 1a) means that ice sheet
collapse due to marine ice sheet instability may have begun (Rignot et
al., 2014; Milillo et al., 2019; Joughin et al., 2014).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F1" specific-use="star"><?xmltex \currentcnt{1}?><label>Figure 1</label><caption><p id="d1e259">Regional setting and input data. <bold>(a)</bold> Ice velocity
(Rignot et al., 2017) with grounding lines from interferometric synthetic aperture radar (InSAR) shown in colour
(Rignot et al., 2014; Milillo et al., 2019); grey lines represent rock exposure. TGT and EIS denote the Thwaites Glacier tongue and Eastern Ice Shelf, respectively. <bold>(b)</bold> Line gravity data
coverage, with regions of known topography and an inset showing Antarctic context.
ASE is Amundsen Sea Embayment, and WAIS is the West Antarctic Ice Sheet. <bold>(c)</bold> Integrated
free air gravity anomaly grid. <bold>(d)</bold> Topographic constraints, with direct observations shown in strong colors. Onshore these were taken from airborne radar including Operation Ice Bridge (OIB) (Paden et al., 2010, updated 2018) and the ITGC airborne survey. Offshore bathymetric data was taken from ship-borne swath coverage (Hogan et al., 2020). Pale colours show BEDMAP2 DEM (Fretwell et
al., 2013). Yellow areas highlight post-1993 ice shelves. Red boxes show the locations of
Figs. 4 and 6.</p></caption>
        <?xmltex \igopts{width=355.659449pt}?><graphic xlink:href="https://tc.copernicus.org/articles/14/2869/2020/tc-14-2869-2020-f01.png"/>

      </fig>

      <p id="d1e280">Understanding the bathymetry beneath the ice shelves separating the open
marine realm of the Amundsen Sea Embayment and the grounded ice of the
Thwaites Glacier system is of particular importance for the evolution of
this region (Fig. 1a). The bathymetry beneath ice shelves is a fundamental
control on the ice sheet stability, as the shape of the water cavity is a
first-order control on sub-ice-shelf currents, including the flux of warm,
deep-ocean water to the ice shelf bases and the grounding line beyond
(Jacobs et al., 2011). Melting, thinning, and ultimately
disintegration of ice shelves will trigger faster glacial flow, forcing
glacial retreat, leading to global mean sea level rise (Scambos et al.,
2004; Rignot et al., 2014). Cavity shape is also likely an important factor
controlling the rate of melting close to the grounding line
(Milillo et al., 2019; Schoof, 2007). Direct
measurement of sub-ice-shelf bathymetry by seismic sounding is slow and
often impractical due to the extremely crevassed environment (Brisbourne
et al., 2014; Rosier et al., 2018). Exploration of sub-ice-shelf cavities
using autonomous underwater vehicles can also be risky and time-consuming to
attain regional coverage (Jenkins et al., 2010; Davies et al., 2017). An
alternative technique to provide a first-order estimate of the bathymetry is
the inversion of airborne gravity anomaly data, which can be collected
quickly and efficiently over large areas.</p>
      <p id="d1e284">Recovery of bathymetry from gravity data relies on the fundamental fact that
the density contrast at the seabed gives rise to significant and measurable
gravity anomalies. A variety of techniques have been employed to invert
gravity data for bathymetry. In the simplest case, the free-air anomaly is
transformed directly to an equivalent surface assumed to reflect the
bathymetry. This can be done in 3D using a fast Fourier transform approach
such as the Parker–Oldenburg iterative method
(Gómez-Ortiz and Agarwal, 2005), as has been applied to the Larsen
Ice Shelf (Cochran and Bell, 2012). Although the broad pattern of
the bathymetry is resolved, transformation of gravity signals directly into
equivalent topography can give rise to significant errors, attributed in the
case of the Larsen Ice Shelf to geological factors such as crustal thickness
and sedimentary basins distorting the gravity field
(Brisbourne et al., 2014). An alternative technique
models the bathymetry using gravity data along multiple 2D profiles, for
example across the Abbot Ice Shelf (Cochran et al., 2014)
and outboard of Thwaites Glacier (Tinto and Bell,
2011; Tinto et al., 2011). Such models are constrained to match known
topography, and inferences about the underlying geology provide additional
constraints. The 3D bathymetry beneath the Pine Island Glacier ice shelf was
inverted from gravity data using a 3D prism model and a simulated annealing
technique solving for bathymetry and a sedimentary layer
(Muto et al., 2016). Although this technique returns a
bathymetry model constrained by observations, it is not clear whether
signatures due to sediments and bathymetry can be reliably separated without
a priori constraints such as seismic observations (Roy et al., 2005).
More recently, a 3D model constrained by regional bathymetry and subglacial
topography was used to model bathymetry offshore of Pine Island and Thwaites
glaciers, and beneath the Crosson and Dotson ice shelves (Millan
et al., 2017). This model showed a complex topography with deep channels
extending to the margin of the ice sheet, particularly in the Dotson–Crosson
area where previously unknown deep (<inline-formula><mml:math id="M6" display="inline"><mml:mrow><mml:mo>&gt;</mml:mo><mml:mn mathvariant="normal">1200</mml:mn></mml:mrow></mml:math></inline-formula> m) channels were
identified.</p>
      <p id="d1e297">In this paper we re-evaluate the sub-ice-shelf bathymetry offshore from
Thwaites Glacier and beneath the Crosson and Dotson ice shelves (Fig. 1a)
through the integration of new airborne gravity data collected during the
2018/2019 field season as part of the NERC/NSF International Thwaites Glacier
Collaboration (ITGC), Operation IceBridge (OIB) (Cochran and Bell,
2010, updated 2018), and new marine gravity data from the R/V <italic>Nathaniel B. Palmer</italic> collected during the cruise NBP19-02 (Fig. 1b). To recover bathymetry
from gravity beneath the ice shelves, we employ an algorithm-based approach
similar to that used for the Brunt Ice Shelf
(Hodgson et al., 2019). This approach constrains
the recovered topography to match all direct topographic observations. This
constraint helps account for geological factors, such as variations in
crustal thickness, sedimentary basins, or intrusions. We acknowledge that
away from direct topographic observations the uncertainties in the
bathymetric estimate due to geological factors increase. However, we suggest
that using a well-constructed gravity-derived bathymetry is preferable to
unconstrained interpolation across sub-ice-shelf bathymetric data gaps many
tens of kilometres wide. Such use of gravity data is routine for predicting
topography in unsurveyed parts of the ocean using satellite data
(Smith and Sandwell, 1994) and is being used in the Arctic where
higher-resolution airborne data are included (Abulaitijiang et al.,
2019).</p>
      <p id="d1e303">Our results confirm the shape and position of the previously identified
troughs (Millan et al., 2017). Differences in the inversion
results beneath the inboard parts of some of the ice shelves are identified,
reflecting the higher resolution of the new gravity data set and differences
in the methods used. Our improved topographic estimate reveals variations in
sub-ice-shelf cavity thickness, which have implications for the rate at
which the warm ocean water can access the present-day grounding lines and
the mechanism of grounding line retreat in these and other areas.</p>
</sec>
<?pagebreak page2871?><sec id="Ch1.S2">
  <label>2</label><title>Methods</title>
<sec id="Ch1.S2.SS1">
  <label>2.1</label><title>The integrated gravity and topographic data sets</title>
      <?pagebreak page2872?><p id="d1e321">We utilise airborne gravity data from OIB and the ITGC campaign, together
with marine gravity data from cruise NBP19-02 (Fig. 1b and c). The OIB
free-air gravity data were collected from a DC-8 aircraft travelling at
<inline-formula><mml:math id="M7" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">120</mml:mn></mml:mrow></mml:math></inline-formula> m s<inline-formula><mml:math id="M8" 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> at an altitude of <inline-formula><mml:math id="M9" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">450</mml:mn></mml:mrow></mml:math></inline-formula> m above
the ice surface, using the Sander Geophysics AirGrav system
(Studinger et al., 2008). These data have an error of <inline-formula><mml:math id="M10" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">1.67</mml:mn></mml:mrow></mml:math></inline-formula> mGal in this region and resolve anomalies with a <inline-formula><mml:math id="M11" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">10</mml:mn></mml:mrow></mml:math></inline-formula> km
full wavelength (Cochran and Bell, 2010, updated 2018; Tinto
and Bell, 2011). The ITGC campaign utilised a Twin Otter aircraft, flying at
<inline-formula><mml:math id="M12" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">60</mml:mn></mml:mrow></mml:math></inline-formula> m s<inline-formula><mml:math id="M13" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>, on average 340 m above the ice, and a
different “strapdown” gravity approach based around an iMAR Inertial
Navigation System (INS) (Becker et al., 2015; Wei and
Schwarz, 1998). The resulting data have an internal error from crossover
analysis of 1.56 mGal and resolve wavelengths down to <inline-formula><mml:math id="M14" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">5</mml:mn></mml:mrow></mml:math></inline-formula> km
(Jordan et al., 2020c) (see Supplement Sect. S2 for
details).</p>
      <p id="d1e409">Airborne gravity data were restricted to lines flown at <inline-formula><mml:math id="M15" display="inline"><mml:mrow><mml:mo>&lt;</mml:mo><mml:mn mathvariant="normal">1500</mml:mn></mml:mrow></mml:math></inline-formula> m
above the surface. Of this subset over 95 % of the data were collected at
<inline-formula><mml:math id="M16" display="inline"><mml:mrow><mml:mn mathvariant="normal">450</mml:mn><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mrow class="unit"><mml:mi mathvariant="normal">m</mml:mi></mml:mrow><mml:mo>±</mml:mo><mml:mn mathvariant="normal">200</mml:mn><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mrow class="unit"><mml:mi mathvariant="normal">m</mml:mi></mml:mrow></mml:mrow></mml:math></inline-formula>  above the surface. Upward and downward continuation of
the gravity data to a common altitude was neglected as continuation by
<inline-formula><mml:math id="M17" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">200</mml:mn></mml:mrow></mml:math></inline-formula> m will have little impact on the amplitude of the
gravity anomalies (<inline-formula><mml:math id="M18" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:math></inline-formula> mGal) given the <inline-formula><mml:math id="M19" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">1000</mml:mn></mml:mrow></mml:math></inline-formula> m
range to the key bathymetric sources. Downward continuation can also
introduce unnecessary artefacts, and neglecting upward continuation preserves
short wavelength gravity information. The data collected <inline-formula><mml:math id="M20" display="inline"><mml:mrow><mml:mo>&gt;</mml:mo><mml:mn mathvariant="normal">650</mml:mn></mml:mrow></mml:math></inline-formula> m
from the ice surface may give rise to an artificially smooth bathymetry but
are spatially restricted (Fig. S1 in the Supplement) and do not appear to give rise to any
anomalous signals in the integrated free-air gravity dataset (Fig. 1c).</p>
      <p id="d1e483">Marine gravity data from cruise NBP19-02 matched the pattern of the airborne
anomalies but were offset by <inline-formula><mml:math id="M21" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">7.14</mml:mn></mml:mrow></mml:math></inline-formula> mGal above the level of
the airborne data. The majority of this offset is due to the difference
between geoid (marine) and ellipsoid (airborne) references used for the
different systems. In the area of overlap the geoid–ellipsoid difference
results in a <inline-formula><mml:math id="M22" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">9</mml:mn></mml:mrow></mml:math></inline-formula> mGal discrepancy, based on the GOCO3s
satellite gravity model  (Pail et al., 2010). The residual
<inline-formula><mml:math id="M23" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:math></inline-formula> mGal difference may reflect drift in the marine system,
and potential discrepancies in base station ties between the different
surveys. Alternatively, unconsidered shorter wavelength variability in the
gravity field not resolved by the GOCO3s model (<inline-formula><mml:math id="M24" display="inline"><mml:mrow><mml:mo>&lt;</mml:mo><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">160</mml:mn></mml:mrow></mml:math></inline-formula> km) or temporal changes in the geoid associated with glacio-isostatic
adjustment and mass loss may account for the residual shift. Such features
do not impact the locally recovered bathymetry and are beyond the scope of
this paper. The average measured shift of 7.14 mGal was therefore subtracted
from the marine line data as a single offset value. All line data were then
merged into a single database, interpolated onto a 1 km mesh raster, and
filtered with a 5 km low-pass filter removing residual line-to-line noise.
This filter wavelength is justified, as anomalies with wavelengths <inline-formula><mml:math id="M25" display="inline"><mml:mrow><mml:mo>&lt;</mml:mo><mml:mn mathvariant="normal">5</mml:mn></mml:mrow></mml:math></inline-formula> km are not resolved by the airborne gravity systems used. The final,
integrated free-air gravity map (Fig. 1c) shows a clear pattern of high and
low anomalies, which first-order match the main 5–10 km wavelength
features visible in the available onshore subglacial topography and offshore
bathymetry (Fig. 1d).</p>
      <p id="d1e538">The topographic observations onshore were taken from OIB line radar data
(Paden et al., 2010, updated 2018), augmented with new depth
sounding radar collected along with the gravity data during the ITGC
campaign (Fig. 1d). These new bed elevation data were collected using a
600–900 MHz accumulation radar provided by the Center for Remote Sensing of
Ice Sheets (CReSIS). Bed elevations were picked from synthetic aperture radar (SAR)-processed
radargrams in a semi-automated fashion. Although the primary target of this
radar system was shallow ice sheet structures, bed elevation was resolved
through ice up to <inline-formula><mml:math id="M26" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">1900</mml:mn></mml:mrow></mml:math></inline-formula> m thick. Visual inspection revealed a
few incorrect onshore bed picks in the OIB dataset on Bear Island, which
gave bed elevations above the highly accurate Reference Elevation Model of Antarctica (REMA) surface digital elevation
model (DEM) (Howat et al., 2019). These points were
deleted from the integrated line bed elevation dataset. The line bed
elevation data were corrected to the GL04c Geoid
(Forste et al., 2008), and the data were then interpolated onto a
1 km mesh raster. This gridded dataset was carefully masked to remove
regions that are now covered by the floating ice shelf based on the most up-to-date grounding lines (Rignot et al., 2014; Milillo et al., 2019). Bed
elevation values over local sub-shelf pinning points were also excluded.
This masking mitigates the risk of the base of a floating ice shelf being
misidentified as a bed elevation point and biasing the inversion. Beyond the
ice shelves we took the values constrained by a new compilation of shipborne
multibeam swath bathymetric data
(Hogan et al., 2020), which was
downsampled to a 1 km mesh raster for this study (Fig. 1d).</p>
</sec>
<sec id="Ch1.S2.SS2">
  <label>2.2</label><title>Recovering sub-ice-shelf bathymetry</title>
      <p id="d1e559">To recover a gravity-enhanced bathymetry we follow an algorithmic approach,
rather than a pure inversion  (Hodgson et al.,
2019). We refer to this as the topographic shift method, as an initial topographic estimate
derived from the gravity data is shifted to match observed topographic tie
points. Summarising the method, the initial 3D topographic estimate (Fig. S2a) was calculated from the free-air anomaly (Fig. 1c) using an iterative
forward modelling method (von Frese et al., 1981).
Differences between the initial topographic estimate (Fig. S2b) and
the observed bathymetry and onshore topography were calculated (Fig. 1d) and
interpolated using a tensioned spline (Smith and Wessel, 1990). This
difference grid was then subtracted from the initial topographic estimate to
provide the final bathymetric estimate (Fig. 2a). For the full details of the
method, see Sect. S1 in the Supplement. The topographic shift method
is conceptually similar to the gravity shift method developed and applied along the
Greenland coast, where the initial free-air gravity data were shifted to
match the variable gravity field from models of known topography prior to
inversion for bathymetry (An et al., 2019). This gravity shift
method was subsequently employed to fill the sub-ice shelf bathymetry in the
Thwaites Glacier region of the recent BedMachine Antarctica compilation
(Fig. S5c in the Supplement) (Morlighem et al., 2020). The advantage of both the topographic
and gravity shift techniques is that features in the gravity field due to
variations in crustal thickness, sedimentary basins, or intrusions are
implicitly taken into account, as long as they overlap with the topographic
control points. This assumption is most robust<?pagebreak page2873?> for long wavelength features,
such as variations in crustal thickness or regional sedimentary basins,
where the associated errors will impact multiple topographic control points,
allowing good control of the resulting error field. The impact of more
localised geological features that only partially overlap constraining
topographic data will be less well defined, and we make the assumption that
such errors fall off smoothly away from the affected control points.
Geological features that have no overlap with constraining topographic
observations can still introduce artefacts, distorting the recovered
bathymetry in proportion to their size and density contrast.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F2" specific-use="star"><?xmltex \currentcnt{2}?><label>Figure 2</label><caption><p id="d1e564">New bathymetry and cavity maps. <bold>(a)</bold> Final topography from terrain
shift method. White lines A–D mark profiles in Fig. 3. The yellow outline
encloses the region constrained by gravity data. The pink line shows the <inline-formula><mml:math id="M27" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">800</mml:mn></mml:mrow></mml:math></inline-formula> m depth
contour. Light grey lines mark grounding lines and the ice shelf edge. <bold>(b)</bold> Sub-ice-shelf water column thickness based on the new gravity-derived bathymetry and the REMA DEM with an assumption
of hydrostatic equilibrium. Regions where the ice sheet is predicted to be
grounded show negative cavity thickness.</p></caption>
          <?xmltex \igopts{width=355.659449pt}?><graphic xlink:href="https://tc.copernicus.org/articles/14/2869/2020/tc-14-2869-2020-f02.png"/>

        </fig>

</sec>
<sec id="Ch1.S2.SS3">
  <label>2.3</label><title>Ice shelf draft and cavity thickness</title>
      <p id="d1e597">The depth of the ice shelf base and the thickness of the sub-ice-shelf
water-filled cavity (Fig. 2b) were calculated assuming the ice shelf is in
hydrostatic balance  (Griggs and Bamber, 2011). Hydrostatically
defined draft is typically a good approximation to radar-measured ice
thickness (Griggs and Bamber, 2011) and provides seamless coverage of our
study area. The input surface elevation data were taken from the REMA
digital elevation model (DEM) (Howat et al., 2019),
corrected to the GL04c Geoid (Forste et al., 2008), and
re-sampled onto a 500 m grid cell size raster. In the study area the REMA
DEM is based on satellite observations between 2014 and 2016 and therefore
reflects the surface elevation after widespread ungrounding between 1993
and 2014 (Rignot et al., 2014). Ice and water densities were
assumed to be 917 and 1027 kg m<inline-formula><mml:math id="M28" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>, respectively, and a 16 m firn
correction was applied  (Griggs and Bamber, 2011). Uncertainties
in these assumed values may have an impact on the precise values of ice
shelf draft but are unlikely to significantly distort the calculated
pattern of water cavity thickness. Comparison between ice shelf base
calculated from the higher resolution DEM and the longer wavelength
bathymetry resolved by the gravity (<inline-formula><mml:math id="M29" display="inline"><mml:mrow><mml:mo>&gt;</mml:mo><mml:mn mathvariant="normal">5</mml:mn></mml:mrow></mml:math></inline-formula> km) will introduce high-frequency features into the estimated cavity depth, and unresolved
bathymetric features will generate errors in cavity thickness. However, the
regional trends in cavity thickness will not be affected and can be
discussed. Errors in ice shelf draft of up to 80 m in the 10–25 km most
proximal to the grounding line may occur due to the rigidity of the ice
shelf (Rignot et al., 2011), but in Thwaites glacier this
“bending zone” appears to be narrow (<inline-formula><mml:math id="M30" display="inline"><mml:mrow><mml:mo>&lt;</mml:mo><mml:mn mathvariant="normal">5</mml:mn></mml:mrow></mml:math></inline-formula> km)
(Milillo et al., 2019), which we attribute to the highly
fractured nature of the ice shelf in this region.</p>
</sec>
</sec>
<sec id="Ch1.S3">
  <label>3</label><title>Results</title>
      <p id="d1e641">Our modelled sub-ice-shelf bathymetry (Fig. 2a) reveals a complex offshore
topography from <inline-formula><mml:math id="M31" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">250</mml:mn></mml:mrow></mml:math></inline-formula> to <inline-formula><mml:math id="M32" display="inline"><mml:mrow><mml:mo>&gt;</mml:mo><mml:mn mathvariant="normal">1000</mml:mn></mml:mrow></mml:math></inline-formula> m deep, with a
pattern of ridges and troughs of a size and scale consistent with the
terrain mapped onshore with radar, and offshore with multi-beam swath
bathymetry. All the key bathymetric features we observe are imaged as
anomalies in the free-air gravity data and are therefore not artefacts of
the inversion technique. Many of the isolated pinning points seaward of
Thwaites Glacier and beneath the Crosson Ice Shelf shown by InSAR-derived
grounding lines (Rignot et al., 2014) are revealed by our study
as being situated on broader bathymetric highs. In these areas our recovered
topography predicts that the ice shelf is grounded, or within 100 m of
grounding (i.e. the water column is calculated to be less than 100 m thick;
Fig. 2b). As our inversion did not use any additional data (swath, seismic,
or radar) to constrain the elevation at these isolated pinning points within
the ice shelves, the fact that many appear to be within error of their
grounding level provides qualitative support for the reliability of our
inversion.</p>
      <p id="d1e664">The revealed sub-ice-shelf cavity is <inline-formula><mml:math id="M33" display="inline"><mml:mrow><mml:mo>&gt;</mml:mo><mml:mn mathvariant="normal">500</mml:mn></mml:mrow></mml:math></inline-formula> m thick in many areas.
Adjacent to parts of Thwaites Glacier this deep cavity reaches to within
0–10 km of the grounding line. In contrast, the inboard parts of the Dotson
and Crosson ice shelves formed since 1993 overlie a cavity typically
<inline-formula><mml:math id="M34" display="inline"><mml:mrow><mml:mo>&lt;</mml:mo><mml:mn mathvariant="normal">150</mml:mn></mml:mrow></mml:math></inline-formula> m thick (Fig. 2b), and the thick (<inline-formula><mml:math id="M35" display="inline"><mml:mrow><mml:mo>&gt;</mml:mo><mml:mn mathvariant="normal">450</mml:mn></mml:mrow></mml:math></inline-formula> m) cavity
lies more than 10–30 km from the current grounding line.</p>
      <p id="d1e697">Profiles of the bathymetry beneath the ice shelves confirm the complex
sub-ice-shelf pattern (Fig. 3). Our results show that the tips of both the
Eastern Ice Shelf and Thwaites Glacier tongue are grounded at their seaward
ends on a linear but dissected ridge, while a <inline-formula><mml:math id="M36" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">1000</mml:mn></mml:mrow></mml:math></inline-formula> m deep
sub-ice-shelf cavity is apparent behind the pinning ridge (Fig. 3a and b).
Where the grounding line of the Thwaites Glacier tongue has retreated since
1993, the estimated ice shelf base closely follows the modelled bathymetry
(Fig. 3b). Along the narrow channel close to Bear Island a cavity
<inline-formula><mml:math id="M37" display="inline"><mml:mrow><mml:mo>&gt;</mml:mo><mml:mn mathvariant="normal">500</mml:mn></mml:mrow></mml:math></inline-formula> m thick is apparent beneath the Crosson Ice Shelf, but this
does not extend into the region where the grounding line has retreated most
significantly in recent decades (Khazendar et al., 2016)
(Fig. 3c). Profiles across the Dotson Ice shelf towards Kohler Glacier
indicate the grounding line is separated from the main sub-ice-shelf cavity
by a sill, which appears to reach within <inline-formula><mml:math id="M38" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">200</mml:mn></mml:mrow></mml:math></inline-formula> m of the base
of the ice shelf (Figs. 2b and 3d).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F3" specific-use="star"><?xmltex \currentcnt{3}?><label>Figure 3</label><caption><p id="d1e733">Profiles across ice shelves. For each panel the upper part shows the ice surface from
REMA DEM (Howat et al., 2019) and the base of ice shelf
calculated assuming hydrostatic equilibrium, together with gravity-derived
bathymetric estimates. The central part of each panel shows the input free-air gravity anomaly.
The lower part of each panel shows magnetic anomalies derived from ITGC survey data
(Jordan et al., 2020b) and ADMAP2
(Golynsky et
al., 2018). The data are taken from <bold>(a)</bold> Thwaites Eastern Ice Shelf, <bold>(b)</bold> Thwaites Glacier tongue, <bold>(c)</bold> Crosson Ice Shelf, and <bold>(d)</bold> Dotson Ice Shelf. Note the thin cavity in regions of ice
sheet grounding line retreat since 1993 (grey boxes in the upper panels). Additionally,
in <bold>(d)</bold> note the <inline-formula><mml:math id="M39" display="inline"><mml:mrow><mml:mo>&gt;</mml:mo><mml:mn mathvariant="normal">500</mml:mn></mml:mrow></mml:math></inline-formula> m bathymetric highs in BedMachine (Morlighem et al., 2020) and Millan et al.
(2017) profiles not associated with a free-air gravity anomaly, indicative
of artefacts resulting from the inversion process.</p></caption>
        <?xmltex \igopts{width=469.470472pt}?><graphic xlink:href="https://tc.copernicus.org/articles/14/2869/2020/tc-14-2869-2020-f03.png"/>

      </fig>

</sec>
<sec id="Ch1.S4">
  <label>4</label><title>Discussion</title>
<sec id="Ch1.S4.SS1">
  <label>4.1</label><title>Quantification of errors</title>
      <p id="d1e783">Quantification of the errors associated with gravity inversions is
challenging, as a combination of intrinsic but quantifiable uncertainties in
the gravity data, the inversion assumptions, and the poorly understood
variability of sub-surface geology all contribute to the error budget.
Errors in the gravity field of <inline-formula><mml:math id="M40" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">1.56</mml:mn></mml:mrow></mml:math></inline-formula> mGal defined from
crossover analysis directly contribute to <inline-formula><mml:math id="M41" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">23</mml:mn></mml:mrow></mml:math></inline-formula> m uncertainty
in the recovered bathymetry. The modelled rock density of 2670 kg m<inline-formula><mml:math id="M42" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>
assumes no sediments are present at the sea floor. This is reasonable given
the generally rugged morphology observed<?pagebreak page2874?> across many parts of the Amundsen
Sea inner shelf (Nitsche et al., 2013; Graham et al., 2009; Larter et al.,
2009). However, assuming all bathymetry was carved into lithified sediment,
the total amplitude of the sub-ice-shelf topography could be underestimated
by <inline-formula><mml:math id="M43" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">11</mml:mn></mml:mrow></mml:math></inline-formula> % (<inline-formula><mml:math id="M44" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">130</mml:mn></mml:mrow></mml:math></inline-formula> m), assuming a typical
sediment density of 2500 kg m<inline-formula><mml:math id="M45" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> (Telford et al., 1990). Lower-density unlithified sediment could lead to even larger underestimates of
topographic amplitude, but such material would not be expected to form all
of the <inline-formula><mml:math id="M46" display="inline"><mml:mrow><mml:mo>&gt;</mml:mo><mml:mn mathvariant="normal">1000</mml:mn></mml:mrow></mml:math></inline-formula> m high ridges recovered by our inversion and imaged
by recent swath data (Hogan et al.,
2020). Other geological factors, such as dense gabbroic intrusions, or local
sedimentary basins could further distort the recovered bathymetry if they
are away from the direct bathymetric observations, which would mitigate the
impact of such features on the final bathymetric model. Underlying
geological factors can, in some cases, be revealed by coincident
aeromagnetic data, as in the case of the Brunt Ice Shelf (Jordan and
Becker, 2018; Hodgson et al., 2019) and Ross Ice Shelf
(Tinto et al., 2019).
In our study, tight correlation between high-amplitude magnetic
(Jordan et al., 2020b) and gravity anomalies is only seen beneath
the grounded part of Thwaites Glacier (Fig. 3b). Such tight correlation is
indicative of a significant geological feature distorting the gravity
signature (Jordan and Becker, 2018) but is not seen on
profiles across the offshore regions (Fig. 3). This favours a model where
underlying geological factors do not dominate the inversion results.</p>
      <p id="d1e861">In addition to quantifying the errors, it is important to note that the
resolution of the bathymetry recovered from gravity data is limited by the
wavelengths resolved by the gravity systems and the survey line spacing. For
this study, the gravity systems resolved minimum wavelengths of 5 to 10 km,
and a minimum line spacing of <inline-formula><mml:math id="M47" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">5</mml:mn></mml:mrow></mml:math></inline-formula> km is achieved outboard of
Thwaites Glacier, while a minimum line spacing of <inline-formula><mml:math id="M48" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">7.5</mml:mn></mml:mrow></mml:math></inline-formula> km was
achieved over the Dotson and Crosson ice shelves. This study therefore only
recovers bathymetric features with a wavelength of <inline-formula><mml:math id="M49" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">5</mml:mn></mml:mrow></mml:math></inline-formula> km and
upwards.</p>
      <p id="d1e894">To best quantify the uncertainty in the sub-ice-shelf bathymetric estimate
in our study region we utilised the new shipborne multibeam bathymetric data
collected predominantly by a recent ITGC cruise, NBP19-02 (Fig. 1a)
(Hogan et al., 2020). The
topographic shift method was rerun with these multibeam data excluded from
the constraining bathymetric dataset (Fig. 4a). The difference between the
results with and without this test dataset (Fig. 4a and b) provides a
snapshot of the errors associated with our recovered bathymetry (Fig. 4c).
In this region the mean error is <inline-formula><mml:math id="M50" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">40</mml:mn></mml:mrow></mml:math></inline-formula> m, with a standard deviation of 100 m.
We take this standard deviation to be representative of the expected error
in our modelled bathymetry. This error is within the typical range for that
quoted for gravity-derived bathymetry, for example error estimates of
<inline-formula><mml:math id="M51" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">60</mml:mn></mml:mrow></mml:math></inline-formula> m have been suggested in Greenland (An et
al., 2019), while errors of up to <inline-formula><mml:math id="M52" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">160</mml:mn></mml:mrow></mml:math></inline-formula> m are suggested for
the Larsen Ice Shelf where, unlike our study, no account had been made for
the underlying geology (Brisbourne et<?pagebreak page2875?> al., 2014; Cochran and Bell, 2012).
The mean error we find indicates that the bathymetry constrained by the
swath data is deeper than predicted by the gravity inversion alone, and
hence that there are geological features in this region distorting the
recovered bathymetry. It is apparent that the largest errors are associated
with higher-frequency topography revealed by the new multibeam data. Such
errors resulting from comparison of datasets with fundamentally different
resolutions is to be expected, highlighting the need for multibeam
bathymetry in regions where sub-kilometre-scale resolution of bathymetry is
required. This is particularly relevant in areas where the seabed topography
includes high-amplitude variations at short wavelengths. In addition, this
pattern of errors means that single seismic observations of cavity depth may
not be ideal tie points for gravity inversions in rugged regions such as
near Thwaites Glacier. A single such seismic measurement typically relies on
a receiver array <inline-formula><mml:math id="M53" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">250</mml:mn></mml:mrow></mml:math></inline-formula> m long (Brisbourne
et al., 2014) and hence could image a local high or low, biasing the wider
gravity inversion.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F4" specific-use="star"><?xmltex \currentcnt{4}?><label>Figure 4</label><caption><p id="d1e940">Error estimates. <bold>(a)</bold> Bathymetric estimate excluding bathymetric
data from cruises NBP19-02 and JR294 (yellow outlines). <bold>(b)</bold> Bathymetry
including new multibeam data (as in Fig. 2a). <bold>(c)</bold> Discrepancy in areas of
additional data. <bold>(d)</bold> Histogram of errors in areas of new multibeam
constraint.</p></caption>
          <?xmltex \igopts{width=355.659449pt}?><graphic xlink:href="https://tc.copernicus.org/articles/14/2869/2020/tc-14-2869-2020-f04.png"/>

        </fig>

</sec>
<sec id="Ch1.S4.SS2">
  <label>4.2</label><title>Previous bathymetric estimates</title>
      <?pagebreak page2876?><p id="d1e969">Comparison between our topographic shift method and previous gravity
inversions in this region show the broad sub-ice-shelf features are resolved
by all methods, but differences in the detailed results are clear (Fig. S5).
The OIB Level 3 data product (Tinto et al., 2011; Tinto
and Bell, 2011) shows the largest discrepancies (Figs. S5a, d and
3a, b), with our new inversion showing bathymetry 200 to 300 m shallower at
the grounding line. This in part reflects the fact that the OIB bathymetric
estimate was limited to using gravity data from 2011 and earlier. In addition this
bathymetric model relied on integrating the results of a series of 2D
forward gravity models, incorporating observed bathymetry and radar-derived
topography beneath the grounded ice. These gravity models did not factor in
any regional trends in the gravity field but rather corrected for a single
DC shift at the outboard end of each profile and modified the upper crustal
density at the inland end of the profile to achieve a good fit. Unmodelled
regional trends could therefore be a factor distorting the recovered
bathymetry.
<?xmltex \hack{\newpage}?>
The Millan et al. (2017) inversion of bathymetry from gravity data shows the
same general pattern of sub-ice-shelf bathymetry as our topographic shift
method (Fig. S5b). However, differences are observed, most clearly beneath
the inboard parts of the Dotson Ice Shelf (Fig. S3e). In addition
significant undulation in the recovered bathymetry that is not associated with any
gravity signal is seen, for example, from 100 to 120 km in Fig. 3d. Such
variability is indicative of artefacts due to the inversion approach. As our
topographic shift method is different, and we incorporate additional new
gravity, bathymetric, and radar data, it is not immediately clear what the
source of these discrepancies are. To independently assess the results of
Millan et al. (2017) we compare their results with BedMachine Antarctica
(Morlighem et al., 2020) (Fig. S4c), which used the same input data as
Millan et al. (2017), and the gravity shift method previously applied to the
Greenland margin (An et al., 2019). The key difference between
the An et al. (2019) and Millan et al. (2017) methods is that the newer
approach applies a variable rather than single DC shift to the gravity prior
to inverting for the bathymetry. The residuals between the Millan et al. (2017) result and BedMachine Antarctica (the gravity shift method) (Fig. S4f)
show a similar pattern to the residuals between the Millan et al. (2017)
result and our topographic shift method (Fig. S4e). This indicates that the
use of a single DC shift was a significant issue in the older inversion
(Millan et al., 2017), which may have led to an overestimate of
the depth of some near-shore features.</p>
      <p id="d1e974">Comparing BedMachine Antarctica and our topographic shift results reveals
that differences of over 250 m are still present (Fig. S5g). We suggest that
these remaining differences reflect the additional multibeam bathymetric,
ITGC radar, and gravity data used in our topographic shift result. In
addition, the different bed topography onshore (OIB and ITGC line radar data
here vs. mass conservation in BedMachine Antarctica; Morlighem et al.,
2020) and exclusion of<?pagebreak page2877?> sub-ice-shelf pinning points from our topographic
shift result also likely contributed to the differences. For example,
topography with no associated gravity signal is seen in the BedMachine
profile in Fig. 3d, indicating the method and tie points used introduced
some artefacts. This highlights the need for caution when using
gravity-derived bathymetry and the value of high-resolution gravity data
with tight line spacing, such as the integrated OIB/ITGC dataset, together
with additional well-constrained and well-distributed observational tie
points beneath the ice shelves and around their margins.</p>
</sec>
<sec id="Ch1.S4.SS3">
  <label>4.3</label><title>Implications for the Amundsen Sea ice shelves</title>
<sec id="Ch1.S4.SS3.SSS1">
  <label>4.3.1</label><title>Pathways for water</title>
      <p id="d1e992">The results of our new bathymetric estimates have significant implications
for how we understand the pattern of cryospheric changes occurring in the
Thwaites, Dotson, and Crosson areas. Our primary observation confirms that
the ice front in the centre of Thwaites Glacier is directly and easily
accessible to mCDW through a channel over 800 m deep beneath the Thwaites
Eastern Ice Shelf and Thwaites Glacier tongue (Millan et al., 2017; Tinto
and Bell, 2011) (Fig. 2a). This trough is separated from an adjacent
<inline-formula><mml:math id="M54" display="inline"><mml:mrow><mml:mo>&gt;</mml:mo><mml:mn mathvariant="normal">1000</mml:mn></mml:mrow></mml:math></inline-formula> m deep trough by a ridge that is in places <inline-formula><mml:math id="M55" display="inline"><mml:mrow><mml:mo>&lt;</mml:mo><mml:mn mathvariant="normal">150</mml:mn></mml:mrow></mml:math></inline-formula> m
deep where the Eastern Ice Shelf and Thwaites Glacier tongue were pinned.
However, 700 to 800 m deep channels cut the ridge, linking the two troughs
and potentially facilitating lateral circulation beneath the ice shelves.
Warm mCDW is dense and could be filling the bathymetric depressions and
troughs on the continental shelf we observe, transporting heat from the
global ocean to interact with ice shelves, and contributing to ice sheet
grounding line melting (Jenkins et al., 2010).</p>
      <p id="d1e1015">The Crosson Ice Shelf is underlain by bathymetry 300 to 500 m deep,
shallower than the typical core of the mCDW (Assmann et
al., 2013). A 700–1000 m deep channel is present flanking Bear Island
(Figs. 2b and 3c), but its width of just 10 km suggests that the flux of
mCDW may be lower via this route. However, in some years the upper boundary
of the mCDW can sit around 400–600 m deep (Dutrieux et al., 2014; Jenkins
et al., 2018), shallower than much of the bathymetry beneath the Crosson Ice
Shelf, meaning mCDW could still access the inner Crosson cavity. The final
<inline-formula><mml:math id="M56" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">30</mml:mn></mml:mrow></mml:math></inline-formula> km to the most recent grounding line of Smith Glacier is
characterised by a cavity typically 100–200 m thick. As models indicate that
reduced cavity thickness can suppress strong oceanic circulation
(Seroussi et al., 2017), this could limit the supply of mCDW
water to the grounding line. The Dotson Ice Shelf is underlain by a broad
cavity <inline-formula><mml:math id="M57" display="inline"><mml:mrow><mml:mo>&gt;</mml:mo><mml:mn mathvariant="normal">800</mml:mn></mml:mrow></mml:math></inline-formula> m deep and is separated from the currently
rapidly changing grounding line of the western branch of the Kohler Glacier
by a sill 700–800 m deep (Fig. 3d). This sill may partially shield this
grounding line from oceanographically driven change, as the bulk of the
inflowing mCDW is mapped at a depth of <inline-formula><mml:math id="M58" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">800</mml:mn></mml:mrow></mml:math></inline-formula> m at the Dotson
ice shelf margin (Miles et al., 2016).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F5" specific-use="star"><?xmltex \currentcnt{5}?><label>Figure 5</label><caption><p id="d1e1050">Data density plot of hydrostatic ice shelf draft against sub-shelf
bathymetry. Trend lines show the best linear fit through a data point cloud. <bold>(a)</bold> Plot for ice shelves outboard of the 1993 grounding line. <bold>(b)</bold> Plot for ice
shelves formed by grounding line retreat since 1993, with the inset showing
histogram of cavity thickness beneath the areas of newly developed ice
shelf. Note that data where ice shelf depth is <inline-formula><mml:math id="M59" display="inline"><mml:mrow><mml:mo>&gt;</mml:mo><mml:mn mathvariant="normal">0</mml:mn></mml:mrow></mml:math></inline-formula> m result from
regions where the ice shelf surface elevation is less than the firn
correction. Points which plot below the <inline-formula><mml:math id="M60" display="inline"><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:mo>:</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:math></inline-formula> line are theoretically grounded.
However, errors in the gravity-derived topography with a standard deviation
of <inline-formula><mml:math id="M61" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">100</mml:mn></mml:mrow></mml:math></inline-formula> m are noted (Fig. 4d); hence, some areas which appear
shallowly grounded may in fact be floating. In addition, uncertainties in
grounding line position and real pinning points within the areas designated
as ice shelves contribute to the observed scatter of anomalous points.</p></caption>
            <?xmltex \igopts{width=412.564961pt}?><graphic xlink:href="https://tc.copernicus.org/articles/14/2869/2020/tc-14-2869-2020-f05.png"/>

          </fig>

</sec>
<sec id="Ch1.S4.SS3.SSS2">
  <label>4.3.2</label><title>Two ice shelf populations</title>
      <p id="d1e1105">A second key observation is that the ice shelves in areas that have ungrounded
since measurement of the 1993 grounding line are all underlain by relatively
thin cavities (Fig. 2b). Such thin cavity geometry in newly ungrounded
regions is predicted by some fully coupled, ice–ocean numerical models of
ice sheet retreat (Seroussi et al., 2017). These newly
formed regions of floating ice (Fig. 1d) appear to be distinct from the
wider, more established, ice shelf system, which is underlain by both thick
and thin cavities. This pattern is not simply a result of distance and
hence time since crossing the grounding line, as in places where the ice
shelf has not advanced inland thick cavities are seen at the grounding line,
for example, west of Thwaites Glacier tongue and east of Pope Glacier (Fig. 2b). To consider the different ice shelf systems in more detail we plotted
hydrostatic ice shelf draft against our recovered bathymetry (Fig. 5). This
comparison utilised the 500 m resolution model of ice sheet draft derived
from the REMA DEM (Sect. 2.3). Although the calculated ice shelf draft has
higher resolution than the gravity-derived bathymetry, the sampled
bathymetry was interpolated smoothly between grid nodes, providing a good
estimate of how bathymetry changes at longer wavelengths across the region.
Progressive downsampling of the model of ice shelf draft did not change the
trend of the observed correlation but reduced the number of points defining
the trend (Fig. S6).</p>
      <p id="d1e1108">The older ice shelves, outboard from the 1993 grounding line, show limited
correlation with the underlying bathymetry (Fig. 5a). This is expected given
the shelves float passively over the underlying topography. Regionally, the
main control on the draft of these ice shelves is likely the depth of top of
the mCDW, which drives enhanced basal melt. The fact that few of the older
ice shelves have depths greater than 500 m is consistent with this
hypothesis, as mCDW at depths of 400 to 800 m is observed in oceanographic
transects at the ice shelf edge (Miles et al., 2016; Dutrieux et al.,
2014; Jenkins et al., 2018; Jacobs et al., 1996).</p>
      <p id="d1e1111">The draft in newly established ice shelf areas shows an almost <inline-formula><mml:math id="M62" display="inline"><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:mo>:</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:math></inline-formula>
relationship with the underlying bathymetry (Fig. 5b). The difference
between the bed elevation and ice shelf draft suggests that these newly
formed cavities are on average 112 m thick, with <inline-formula><mml:math id="M63" display="inline"><mml:mrow><mml:mo>&gt;</mml:mo><mml:mn mathvariant="normal">95</mml:mn></mml:mrow></mml:math></inline-formula> % being
<inline-formula><mml:math id="M64" display="inline"><mml:mrow><mml:mo>&lt;</mml:mo><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">400</mml:mn></mml:mrow></mml:math></inline-formula> m thick. The rapid grounding line retreat
that led to the formation of the post-1993 ice shelf sectors has been
regarded as a harbinger of catastrophic collapse of the Amundsen Sea sector
of the West Antarctic Ice Sheet through geometric marine ice sheet
instability, unconstrained by inland pinning points (Rignot et
al., 2014). It has been suggested that basal melting driven by ingress of
warmer mCDW could be a key factor<?pagebreak page2878?> facilitating this process (Milillo et
al., 2019; Pritchard et al., 2012). Enhanced basal melting of up to 200 m a<inline-formula><mml:math id="M65" 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>  has been calculated from satellite observations and OIB radar profiles
over the new Thwaites Glacier ice shelves  (Milillo et al.,
2019), and rates of 50–70 m a<inline-formula><mml:math id="M66" 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> have been observed close to the
grounding line of Smith Glacier (Khazendar et al., 2016).
However, our data indicate that the highest of these melt rates must be
restricted to the grounding line, as the newly formed cavity thickness
typically does not exceed <inline-formula><mml:math id="M67" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">400</mml:mn></mml:mrow></mml:math></inline-formula> m, i.e. approximately 2 years of the most elevated melt rates and 8 years at the lower end of the
enhanced melt rates. We propose that the fast-flowing ice is advected across
the region of most enhanced melting, limiting subsequent thinning of the
cavity. This is in line with the suggestion of previous authors that where
grounding line retreat is driven by melting, very high melt rates are likely
focused at the grounding line (Lilien et al., 2019).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F6"><?xmltex \currentcnt{6}?><label>Figure 6</label><caption><p id="d1e1186">Rate of Crosson Ice Shelf thinning determined by direct radio echo
sounding measurements from 2009, 2010, and 2016 OIB  (Paden et
al., 2010, updated 2018) and the 2005 AGASEA survey (Khazendar et al.,
2016; Holt et al., 2006; Blankenship et al., 2012). Coloured contours show
the expected depth of the base of the floating ice shelf. White lines show InSAR-derived
grounding lines marking the front and back edges of the “new” ice shelf
(Rignot et al., 2014). For the regional setting, see Fig. 1d.</p></caption>
            <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://tc.copernicus.org/articles/14/2869/2020/tc-14-2869-2020-f06.jpg"/>

          </fig>

      <p id="d1e1195">In the Smith Glacier region comparison of 2016 OIB radar data with earlier radar
data allows reconstruction of the spatial distribution of the most recent
ice shelf thinning (Fig. 6). These direct observations confirm, as predicted
from our cavity thickness estimate, that across much of the new ice shelf
thinning rates are relatively low; hence, a relatively thin cavity can be
maintained. However, they also reveal that the enhanced thinning rates of
50–70 m a<inline-formula><mml:math id="M68" 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> beneath the inner shelf noted for the period 2002–2009
(Khazendar et al., 2016) have continued into the period 2009–2016. These
high rates appear to be restricted to the area where the base of the ice
shelf is <inline-formula><mml:math id="M69" display="inline"><mml:mrow><mml:mo>&gt;</mml:mo><mml:mn mathvariant="normal">1200</mml:mn></mml:mrow></mml:math></inline-formula> m deep. One possibility is that mCDW is
penetrating to the grounding line and pooling at these depths. However, it
is not clear to what extent this water would have been mixed and diluted
during its passage through the <inline-formula><mml:math id="M70" display="inline"><mml:mrow><mml:mo>&lt;</mml:mo><mml:mn mathvariant="normal">400</mml:mn></mml:mrow></mml:math></inline-formula> m thick sub-ice-shelf cavity.
Additionally, ice shelf marginal weakening and consequent ice acceleration may have
also contributed to the observed fast grounding line retreat and thinning at
the grounding line without the need for such extreme basal melting
(Lilien et al., 2019).</p>
      <p id="d1e1230">The consistent presence of broad but vertically thin subglacial cavities
appears to challenge a purely melt-driven model of future ice sheet
collapse, as access by warm water to the grounding line would be hampered by
the thin cavity (Schoof, 2007). This physical limitation is
supported by models for Pine Island Glacier margin, which indicated that
cavities <inline-formula><mml:math id="M71" display="inline"><mml:mrow><mml:mo>&lt;</mml:mo><mml:mn mathvariant="normal">200</mml:mn></mml:mrow></mml:math></inline-formula> m thick slowed the ingress of warm bottom water over
topographic ridges (De Rydt et al., 2014). More complex fully
coupled ice–ocean models also show the development of thin cavities and
indicate that the associated weak circulation acts to slow grounding line
retreat relative to that predicted by an uncoupled model
(Seroussi et al., 2017).</p>
      <p id="d1e1243">The contrast in cavity geometry and relationship to the underlying
bathymetry of the pre- and post-1993 ice shelf regions suggests that the
recently ungrounded regions may not yet be in equilibrium with the wider
glaciological and oceanic system. As such, they may play a significant but
as yet poorly understood role in controlling the future evolution of the ice
sheet marginal system. The thin cavities in particular may act to slow
future changes. Firstly, they place a<?pagebreak page2879?> fundamental limit onto the amount of
warm water that can flux beneath the glacier and may also facilitate the
tidally driven turbulent flow mixing of water masses before they can reach
the grounding line (Holland, 2008). In addition, the thin cavities
that we observe are particularly sensitive to re-grounding on retrograde
slopes, a negative feedback that would act to temporally re-stabilise a
retreating ice sheet, a process that would be favoured by the observed
rapid uplift due to glacial isostatic adjustment  (Barletta et
al., 2018). The process of grounding line re-advance appears to have
occurred in the western Kohler Glacier (Fig. 1a), where the 2014 grounding
line lies downstream of the 2012 grounding line (Rignot et al.,
2014). Our observations of consistent thin cavities in newly ungrounded
regions support the results of coupled ice–ocean models, confirming the
necessity of such detailed modelling for predicting the evolution of the
Thwaites Glacier system (Seroussi et al., 2017).</p>
</sec>
</sec>
</sec>
<sec id="Ch1.S5" sec-type="conclusions">
  <label>5</label><title>Conclusions</title>
      <p id="d1e1257">Airborne gravity provides a good first-order estimate of sub-ice-shelf
bathymetry. Despite the relatively high uncertainty (<inline-formula><mml:math id="M72" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">100</mml:mn></mml:mrow></mml:math></inline-formula> m
standard deviation), comparisons with different gravity inversion techniques,
the location of ice shelf pinning points, and new observational bathymetric
data indicate that the pattern of sub-ice-shelf bathymetry is well
resolved.</p>
      <p id="d1e1270">Thwaites Glacier is connected to Pine Island Bay to its east by a major
trough that is <inline-formula><mml:math id="M73" display="inline"><mml:mrow><mml:mo>&gt;</mml:mo><mml:mn mathvariant="normal">800</mml:mn></mml:mrow></mml:math></inline-formula> m deep and 20 km wide. In contrast, the grounding
lines of the of Dotson and Crosson ice shelves are accessible through
relatively narrow channels and thin sub shelf cavities.</p>
      <p id="d1e1283">In the Thwaites, Dotson, and Crosson region, areas of ice shelf that
developed before and after 1993 form distinct populations. The most recently
ungrounded areas are underlain by thin cavities (average 112 m) where the
ice shelf base closely tracks the underlying bed topography. We propose that
these systems represent a transient phase of ice margin development that
may act to slow future changes, which is indicated by but not fully captured in
present models.</p>
</sec>

      
      </body>
    <back><notes notes-type="dataavailability"><title>Data availability</title>

      <p id="d1e1290">The new calculated bathymetry, along with input topography and gravity grids,
is available from the UK Polar Data Centre    (<ext-link xlink:href="https://doi.org/10.5285/7803DE8B-8A74-466B-888E-E8C737BF21CE" ext-link-type="DOI">10.5285/7803DE8B-8A74-466B-888E-E8C737BF21CE</ext-link>, Jordan et
al., 2020a). The associated ITGC line airborne gravity and magnetic data are
available from the same source (<ext-link xlink:href="https://doi.org/10.5285/776612D1-573C-49C4-AFF5-23B0FBA48271" ext-link-type="DOI">10.5285/776612D1-573C-49C4-AFF5-23B0FBA48271</ext-link>, Jordan et al.,
2020b; <ext-link xlink:href="https://doi.org/10.5285/B9B28A35-8620-4182-BF9C-638800B6679B" ext-link-type="DOI">10.5285/B9B28A35-8620-4182-BF9C-638800B6679B</ext-link>, Jordan et al., 2020c). Other data are from sources cited in the text.</p>
  </notes><app-group>
        <supplementary-material position="anchor"><p id="d1e1302">The supplement related to this article is available online at: <inline-supplementary-material xlink:href="https://doi.org/10.5194/tc-14-2869-2020-supplement" xlink:title="pdf">https://doi.org/10.5194/tc-14-2869-2020-supplement</inline-supplementary-material>.</p></supplementary-material>
        </app-group><notes notes-type="authorcontribution"><title>Author contributions</title>

      <p id="d1e1311">All authors contributed to the discussion and production of the final manuscript. Additional specific contributions are as follows: gravity data processing, topographic shift bathymetric inversion, and primary manuscript preparation was carried out by TAJ. Airborne gravity and magnetic data collection was led by DP. Discussion of bathymetry inversion techniques, including previous inversion methods, was aided by KT and RM. Discussion of gravity inversion and implications of ice sheet cavity findings was with the assistance of AM. Preparation of multibeam swath bathymetry compilation was carried out by KH. RDL provided ship-borne gravity and multibeam swath data. Processing and preparation of multibeam swath bathymetry data on NBP19-02 was carried out by AGCG. Airborne radar system development, data processing, and ice bottom tracking was led by JDP.</p>
  </notes><notes notes-type="competinginterests"><title>Competing interests</title>

      <p id="d1e1317">The authors declare that they have no conflict of interest.</p>
  </notes><ack><title>Acknowledgements</title><p id="d1e1323">This work is a British Antarctic Survey (BAS) National Capability
contribution to the International Thwaites Glacier Collaboration (ITGC),
with additional support from the BAS Geology and Geophysics Team (Tom A. Jordan).
Additional<?pagebreak page2880?> support for this work is from Lamont-Doherty Earth Observatory,
NSF grant no. NSF1842064 (David Porter, Kirsty Tinto) and the THOR (Kelly Hogan, Robert D. Larter, Alastair G. C. Graham, and cruise
NBP19-02), TARSAN (Atsuhiro Muto), and MELT (John D. Paden) projects, components of the
International Thwaites Glacier Collaboration (ITGC). This is paper no. ITGC:009.</p></ack><notes notes-type="financialsupport"><title>Financial support</title>

      <p id="d1e1328">This research has been supported by the UK Natural Environment Research Council (NERC) (grant nos. NE/S006664/1, NE/S006419/1) and US National Science Foundation (NSF) (grant nos. NSF1842064, NSFPLR-NERC-1738942, NSFPLR-NERC-1738992, NSFPLR-NERC-1739003).</p>
  </notes><notes notes-type="reviewstatement"><title>Review statement</title>

      <p id="d1e1334">This paper was edited by Joseph MacGregor and reviewed by two anonymous referees.</p>
  </notes><ref-list>
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<abstract-html><p>Ice shelves play a critical role in the long-term
stability of ice sheets through their buttressing effect. The underlying
bathymetry and cavity thickness are key inputs for modelling future ice
sheet evolution. However, direct observation of sub-ice-shelf bathymetry is
time-consuming, logistically risky, and in some areas simply not possible.
Here we use new compilations of airborne and marine gravity, radar depth
sounding, and swath bathymetry to provide new estimates of sub-ice-shelf
bathymetry outboard of the rapidly changing West Antarctic Thwaites Glacier
and beneath the adjacent Dotson and Crosson ice shelves. This region is of
special interest, as the low-lying inland reverse slope of the Thwaites
Glacier system makes it vulnerable to marine ice sheet instability, with
rapid grounding line retreat observed since 1993 suggesting this process may
be underway. Our results confirm a major marine channel  &gt; 800&thinsp;m
deep extends tens of kilometres to the front of Thwaites Glacier, while the
adjacent ice shelves are underlain by more complex bathymetry. Comparison of
our new bathymetry with ice shelf draft reveals that ice shelves formed
since 1993 comprise a distinct population where the draft conforms closely
to the underlying bathymetry, unlike the older ice shelves, which show a more
uniform depth of the ice base. This indicates that despite rapid basal
melting in some areas, these recently floated parts of the ice shelf are not
yet in dynamic equilibrium with their retreated grounding line positions and
the underlying ocean system, a factor which must be included in future
models of this region's evolution.</p></abstract-html>
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