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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-12-2211-2018</article-id><title-group><article-title>Greenland Ice Mapping Project: ice flow velocity variation at sub-monthly to
decadal timescales</article-title><alt-title>Greenland Ice Mapping Project</alt-title>
      </title-group><?xmltex \runningtitle{Greenland Ice Mapping Project}?><?xmltex \runningauthor{I. Joughin et al.}?>
      <contrib-group>
        <contrib contrib-type="author" corresp="yes" rid="aff1">
          <name><surname>Joughin</surname><given-names>Ian</given-names></name>
          <email>ian@apl.washington.edu</email>
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Smith</surname><given-names>Ben E.</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-1118-7865</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2">
          <name><surname>Howat</surname><given-names>Ian</given-names></name>
          
        </contrib>
        <aff id="aff1"><label>1</label><institution>Polar Science Center, Applied Physics Lab, University of Washington,
1013 NE 40th St., Seattle, WA 98105-6698, USA</institution>
        </aff>
        <aff id="aff2"><label>2</label><institution>Byrd Polar and Climate Research Center, Ohio State University, 1090
Carmack Road, Columbus, OH 43210, USA</institution>
        </aff>
      </contrib-group>
      <author-notes><corresp id="corr1">Ian Joughin (ian@apl.washington.edu)</corresp></author-notes><pub-date><day>11</day><month>July</month><year>2018</year></pub-date>
      
      <volume>12</volume>
      <issue>7</issue>
      <fpage>2211</fpage><lpage>2227</lpage>
      <history>
        <date date-type="received"><day>15</day><month>February</month><year>2018</year></date>
           <date date-type="rev-request"><day>27</day><month>February</month><year>2018</year></date>
           <date date-type="rev-recd"><day>19</day><month>June</month><year>2018</year></date>
           <date date-type="accepted"><day>20</day><month>June</month><year>2018</year></date>
      </history>
      <permissions>
        
        
      <license license-type="open-access"><license-p>This work is licensed under the Creative Commons Attribution 4.0 International License. To view a copy of this licence, visit <ext-link ext-link-type="uri" xlink:href="https://creativecommons.org/licenses/by/4.0/">https://creativecommons.org/licenses/by/4.0/</ext-link></license-p></license></permissions><self-uri xlink:href="https://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>
    <p id="d1e104">We describe several new ice velocity maps produced by the
Greenland Ice Mapping Project (GIMP) using Landsat 8 and Copernicus Sentinel
1A/B data. We then focus on several sites where we analyse these data in
conjunction with earlier data from this project, which extend back to the
year 2000. At Jakobshavn Isbræ and Køge Bugt, we find good agreement when
comparing results from different sensors. In a change from recent behaviour,
Jakobshavn Isbræ began slowing substantially in 2017, with a midsummer
peak that was even slower than some previous winter minima. Over the last
decade, we identify two major slowdown events at Køge Bugt that coincide
with short-term advances of the terminus. We also examined populations of
glaciers in north-west and south-west Greenland to produce a record of speed-up
since 2000. Collectively these glaciers continue to speed up, but there are
regional differences in the timing of periods of peak speed-up. In addition,
we computed trends in winter flow speed for much of the south-west margin of
the ice sheet and find little in the way of statistically significant changes
over the period covered by our data. Finally, although the consistency of the
data is generally good over time and across sensors, our analysis
indicates that substantial differences can arise in regions with high strain
rates (e.g. shear margins) where sensor resolution can become a factor. For
applications such as constraining model inversions, users should factor in
the impact that the data's resolution has on their results.</p>
  </abstract>
    </article-meta>
  </front>
<body>
      

      <?xmltex \hack{\newpage}?>
<sec id="Ch1.S1" sec-type="intro">
  <title>Introduction</title>
      <p id="d1e116">As recently as the 1990s (Paterson, 1994), it was assumed that the Greenland
Ice Sheet and its outlet glaciers would respond slowly to climate change.
Since the satellite record began, largely since the 1990s, it has proved
these early assumptions false. In particular, many glaciers in Greenland
have sped up substantially over the last two decades (e.g. Joughin et al.,
2010; Moon et al., 2012; Rignot and Kanagaratnam, 2006), including several
of Greenland's largest glaciers (Howat et al., 2005; Joughin et al., 2004;
Luckman et al., 2006). In addition to the ice sheet's outlet glaciers,
slow-flowing areas near its margin speed up and slow down seasonally (e.g.
Joughin et al., 2008a; van de Wal et al., 2008; Zwally et al., 2002) in
response to surface meltwater making its way to the bed through moulins,
which can penetrate ice more than 1 km thick (Das et al., 2008).</p>
      <p id="d1e119">Several groups have produced estimates of velocity for Greenland using
synthetic aperture radar (SAR) and optical images (Mouginot et al., 2017;
Nagler et al., 2015; Rosenau et al., 2015). As part of the work described
here, several maps from 2000 onwards have been produced by the Greenland Ice
Mapping Project (GIMP) (Joughin et al., 2010, 2017; Moon et al., 2012). The
GIMP maps have made extensive use of SAR data from the European Space
Agency's (ESA) ERS 1&amp;2, the Canadian Space Agency's (CSA) RADARSAT 1, the
Japanese Space Agency's (JAXA) ALOS-PALSAR, and the German Space Agency's
(DLR) TerraSAR-X and TanDEM-X missions.</p>
      <p id="d1e122">In late 2014 the European Union's Copernicus programme began providing
Sentinel 1A SAR data at 12-day intervals suitable for ice-sheet mapping
(Mouginot et al., 2017; Nagler et al., 2015). With the addition of Sentinel
1B to the<?pagebreak page2212?> Copernicus constellation in late 2016, ESA began processing
and distributing regular 6-day coverage of Greenland's coastal regions.
These coastal data are complemented by several cycles of coverage over the
interior each winter to provide annual coverage of the entire ice sheet.
These data are routinely ingested into the NASA MEaSUREs programme's GIMP
velocity products, which are freely distributed through the National Snow
and Ice Data Center (NSIDC, 2018). In addition to radar data, the maps from
2014 onwards also include Landsat 8 data.</p>
      <p id="d1e125">Here we describe the production of new GIMP velocity maps that incorporate
the Sentinel 1A/B and Landsat 8 data along with data from other sources.
Although we emphasize the new products, we examine these products in the
context of the entire GIMP 17-year time series to estimate seasonal- to
decadal-scale variability in Greenland. We analyse the continuity of the
data set and evaluate the magnitudes of any systematic differences between
data sets produced using different sensors. Finally, we examine changes in
ice flow at several locations in Greenland to demonstrate the utility of the
time series for understanding processes related to ice-sheet and
outlet glacier dynamics.</p>
</sec>
<sec id="Ch1.S2">
  <title>Methods</title>
      <p id="d1e134">The GIMP velocity products are derived using
speckle-tracking/feature-tracking cross-correlation algorithms applied to
pairs of SAR or Landsat 8 images. In cases where the interferometric phase
is available, it is also included in the solution since it improves the
resolution and provides greater accuracy for the component of motion
directed in the satellite look direction (Joughin et al., 2010). The GIMP
velocity products described here are processed using the same core set of
algorithms, which have been described extensively elsewhere (Joughin, 2002;
Joughin et al., 2010, 2017). As a result, here we focus only on the details
of the processing relevant to Sentinel 1A/B data.</p>
      <p id="d1e137">Unlike traditional stripmap SAR data used in earlier GIMP products, which
are distributed as spatially continuous images, the data from the
Interferometric Wide (IW) swath mode of the Sentinel 1 Terrain Observation with
Progressive Scans SAR (TOPSAR) are distributed as series of overlapping
<inline-formula><mml:math id="M1" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 82 by 20 km discrete bursts, acquired along three adjacent
sub-swaths. Since the bursts are small relative to the scale of the ice
sheet, the first step in our processing is to use the GAMMA Interferometric
SAR (ISP) package to assemble each set of bursts into a continuous
single-look complex (SLC) image with a width of <inline-formula><mml:math id="M2" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 250 km and a
length of several hundred kilometres. Once the SLCs are assembled, we
process them in the same way that we would normal stripmap (i.e.
non-bursted) SAR images, using our in-house speckle-tracking algorithms.
Although some data acquisitions traverse the full length of Greenland, we
typically break these data acquisitions up in to individual pieces of more
manageable size (<inline-formula><mml:math id="M3" display="inline"><mml:mo lspace="0mm">&lt;</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M4" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 1200 km).</p>
      <p id="d1e168">For many early SAR missions, the accuracy of the orbital state vectors was
not sufficient to determine the geometric baseline (difference in position)
between the satellite(s) on successive passes. As a result, ground control
points of known elevation and speed often are used to solve for the
geometric baseline parameters to produce calibrated velocity measurements
(Joughin et al., 1996). In principal, the Sentinel 1A/B orbital state
vectors are sufficiently accurate to calculate the baseline and other
geometric parameters with little or no ground control (Nagler et al., 2015).
Since our workflow is adapted to use ground control points, however, we use
these points with Sentinel 1 data to maintain consistency with earlier GIMP
products. For the regular 6- and 12-day Sentinel coastal acquisitions, our
baseline solutions are largely constrained by bedrock points, where we know
that the velocity should be zero. For the winter campaigns, however, some
swaths are positioned well away from the coasts. In these cases, we use our
existing control-point database, which includes balance velocities and GPS
measurements from areas where little change in flow speed is expected
(Joughin et al., 2017). We augment these control points by extracting
SAR-derived point velocity estimates from areas where there is overlap with
well-constrained coastal data takes acquired at similar times.</p>
      <p id="d1e171">An advantage of using control points is that they offer the potential to
improve the baseline solution, although this improvement has declined over
time as orbit reconstructions improve with each new sensor. A second
advantage is that the control-points may, at least partially, mitigate
other, non-positional, sources of error. For example, the baseline solution
can partially compensate for ionospheric path delays, particularly at L-band
for which such delays are larger. The potential downside to using control
points is that velocity errors at the control points can bias the solution.
Our baseline solutions, however, use 100s to 1000s of points to solve for at
most six parameters, providing a relatively robust solution. Furthermore, we
have carefully culled the control points to avoid introducing biases
(Joughin et al., 2017).</p>
      <p id="d1e175">The Landsat 8 panchromatic (band 8) 15 m data are high-pass filtered and
then processed using a cross-correlation-based feature-tracking algorithm
similar to that used by others (Fahnestock et al., 2016; Jeong et al.,
2017). The images are delivered in UTM format, so we first project them to
the polar stereographic projection (EPSG:3413) that we use for all of the
GIMP products. Although the Landsat-8 offsets are produced in map-projected
coordinates, we use a control-point procedure to fit a simple plane to each
velocity component in each image pair to compensate for geolocation errors
(Joughin et al., 2017). In the final stage of calculation, corrections are
made for the projection-dependent-scale distortion.</p>
      <p id="d1e178">Once the SAR and Landsat 8 data have been calibrated using control points,
all of the data are combined and mosaicked to the final output grid using
our<?pagebreak page2213?> velocity-determination algorithms (Joughin, 2002; Joughin et al., 2010,
2017). At each point in the output, the result represents an
inverse-error-weighted (i.e. <inline-formula><mml:math id="M5" display="inline"><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:mo>/</mml:mo><mml:msup><mml:mi mathvariant="italic">σ</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>) average of all viable
estimates. As described below, besides the inverse-error weighting,
additional weighting is applied to the data as needed. As part of the
velocity estimation procedure, a formal error estimate is produced for each
point in the output grid. In general, these errors agree well (within about
a factor of 2) with independent estimates of error (Joughin et al., 2017).
Although the error estimates are given as 1<inline-formula><mml:math id="M6" display="inline"><mml:mi mathvariant="italic">σ</mml:mi></mml:math></inline-formula> values, the actual
distribution likely has a heavier tail than that of a Gaussian distribution
but with the same standard deviation. Care should be taken, therefore, in
applying standard tests of statistical significance due to the potential for
large outliers.</p>
      <p id="d1e203">Most prior SAR missions have provided coverage exclusively along ascending
or descending orbits. With the Sentinel 1A/B mission, however, the
measurements often cover an area from both ascending and descending orbits,
particularly during the winter mapping campaigns. In such cases, we apply a
surface-parallel flow assumption to determine the velocity solely from
ascending and descending range offsets (Joughin et al., 1998). The advantage
of this approach is that it avoids using the noisier, along-track azimuth
offsets. A disadvantage is that range-offset errors tend to be amplified by
about a factor of 3 in the north–south direction. Nonetheless, such
solutions are generally far less noisy than pure range-azimuth offset
estimates, particularly at times when the ionosphere introduces errors in
the azimuth component of the speckle-tracked velocity estimates (Gray et
al., 2000). In our final solutions, we include both types of estimates,
weighted by their respective inverse-error estimates.</p>
      <p id="d1e206">The GIMP project produces two types of velocity products. The first type
provides “snapshot” velocities calculated from the displacements in a
single image pair. The second type provides aggregated estimates, which
represent a single time period but are formed by averaging multiple
individual estimates. In the latter case, the individual constituent
estimates may not uniformly sample the output interval. In these cases,
there are various trade-offs that must be considered to produce accurate
results without sacrificing too much temporal resolution or introducing too
large deviations from the nominal time stamp (temporal skew).</p>
      <p id="d1e209">Through GIMP, we produce annual (12-monthly), winter (up to 9-monthly),
quarterly (3-monthly), and monthly aggregate products. As an example of the
temporal-resolution issues that arise in producing such data sets, consider
the case of monthly sampling, with time intervals corresponding to each
calendar month. If our only source data are 12-day Sentinel 1A pairs, then
some pairs will straddle the beginning and end of each month. In this case,
we weight each pair by its duration of overlap with the month. In the absence of other
weighting, this operation is equivalent to linearly interpolating the 12-day
time series to each day of the month and then averaging the result. This
operation necessarily degrades the temporal resolution of the product, since
interpolation can be represented as the convolution of a low-pass filter
with the data. In this example, degradation would be relatively small.</p>
      <p id="d1e212">Another problem with temporal sampling is what to do with data with
coarser temporal resolution than the sampling interval. In areas where
data are plentiful, coarsely-sampled data may be discarded. There are cases,
however, where these data may be the only available or their inclusion might
significantly improve accuracy. As a result, we do include some data with
coarser temporal resolution than the nominal sampling interval. In
particular, we allow the inclusion of data collected over a time span up to
<inline-formula><mml:math id="M7" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 60 % greater than the sampling interval. Weighting is
applied to these data (e.g. for a 30-day interval; a 48-day Landsat 8 would
be weighted by a factor of 30/48) so they mainly contribute to the solution
in cases where there is insufficient finer-resolution data. Thus, in some
areas the temporal resolution of the GIMP products is coarser than the
posted sampling interval, with the degree of resolution degradation
depending on the spatially varying mix of data used to compute the velocity.</p>
      <p id="d1e223">Both the weighting to accommodate temporal sampling and the inverse-error
weighting can skew the nominal centre data for each aggregated product. For
example, if a subset of the data is much less noisy, it will contribute more
heavily to the average and skew the effective data toward the time covered
by the less noisy result. Similarly, missing data can skew the effective
time away from the nominal sampling time. To indicate where a large temporal
skew may have occurred, we apply the data weights to compute the average of
the deviation of the data for each pair from the nominal centre date. Since
this scalar variable represents a complicated average of many data, it is
best used to diagnose cases where temporal skew could be an issue rather
than to serve as a correction. All data plotted here are shown for their
nominal time stamp.</p>
      <p id="d1e226">While our goal is to produce uniform sampling, some degree of temporal skew
and loss of resolution as described above is inevitable. Our approach
attempts to optimally balance the level of noise with the size of data gaps
for the anticipated common applications of the data set, as illustrated in
the examples below. The individual estimates, however, remain available for
cases where more precise timing is needed and a higher noise level can be
tolerated (e.g. to compare speed-up with terminus retreat events).</p>
</sec>
<sec id="Ch1.S3">
  <title>Results</title>

<?xmltex \floatpos{p}?><table-wrap id="Ch1.T1" orientation="landscape"><caption><p id="d1e238">Summary of GIMP velocity data sets and current archival status.</p></caption><oasis:table frame="topbot"><oasis:tgroup cols="4">
     <oasis:colspec colnum="1" colname="col1" align="justify" colwidth="142.26378pt"/>
     <oasis:colspec colnum="2" colname="col2" align="left"/>
     <oasis:colspec colnum="3" colname="col3" align="justify" colwidth="56.905512pt"/>
     <oasis:colspec colnum="4" colname="col4" align="justify" colwidth="150.799606pt"/>
     <oasis:thead>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1">Product</oasis:entry>
         <oasis:entry colname="col2">DOI</oasis:entry>
         <oasis:entry colname="col3">Date range</oasis:entry>
         <oasis:entry colname="col4">Sensors</oasis:entry>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1">Individual glacier velocities</oasis:entry>
         <oasis:entry colname="col2"><ext-link xlink:href="https://doi.org/10.5067/MEASURES/CRYOSPHERE/nsidc-0481.001" ext-link-type="DOI">10.5067/MEASURES/CRYOSPHERE/nsidc-0481.001</ext-link></oasis:entry>
         <oasis:entry colname="col3">2009–present</oasis:entry>
         <oasis:entry colname="col4">TerraSAR-X and TanDEM-X</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1">Winter velocity maps (September–May)</oasis:entry>
         <oasis:entry colname="col2"><ext-link xlink:href="https://doi.org/10.5067/OC7B04ZM9G6Q" ext-link-type="DOI">10.5067/OC7B04ZM9G6Q</ext-link></oasis:entry>
         <oasis:entry colname="col3">2000–2001, 2005–2010, 2012–2013, 2014–present</oasis:entry>
         <oasis:entry colname="col4">RADARSAT 1, ALOS PALSAR, TerraSAR-X, TanDEM-X, and Sentinel 1A/B</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1">Annual velocity</oasis:entry>
         <oasis:entry colname="col2"><ext-link xlink:href="https://doi.org/10.5067/OBXCG75U7540" ext-link-type="DOI">10.5067/OBXCG75U7540</ext-link></oasis:entry>
         <oasis:entry colname="col3">Late 2014-present</oasis:entry>
         <oasis:entry colname="col4">TerraSAR-X, TanDEM-X, Sentinel 1A/B, Landsat 8</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1">Quarterly velocity (November–February, March–May, June–August, September–November)</oasis:entry>
         <oasis:entry colname="col2"><ext-link xlink:href="https://doi.org/10.5067/1Q1AM4U8Y892" ext-link-type="DOI">10.5067/1Q1AM4U8Y892</ext-link></oasis:entry>
         <oasis:entry colname="col3">Late 2014–present</oasis:entry>
         <oasis:entry colname="col4">TerraSAR-X, TanDEM-X, Sentinel 1A/B, Landsat 8</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1">Monthly velocity (by calendar month)</oasis:entry>
         <oasis:entry colname="col2"><ext-link xlink:href="https://doi.org/10.5067/OPFQ9QDEUFFY" ext-link-type="DOI">10.5067/OPFQ9QDEUFFY</ext-link></oasis:entry>
         <oasis:entry colname="col3">Late 2014–present</oasis:entry>
         <oasis:entry colname="col4">TerraSAR-X, TanDEM-X, Sentinel 1A/B, Landsat 8</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Individual Landsat-8 and Sentinel 1A/B</oasis:entry>
         <oasis:entry colname="col2">Delivery to archive scheduled for autumn 2018</oasis:entry>
         <oasis:entry colname="col3">Late 2014–present</oasis:entry>
         <oasis:entry colname="col4">Sentinel 1A/B and Landsat 8</oasis:entry>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup></oasis:table></table-wrap>

      <p id="d1e372">Table 1 summarizes only the GIMP velocity products discussed here. For
simplicity it excludes the multi-year average product (Joughin et al., 2017)
and optical-only (Howat, 2017) GIMP products. Of the products in Table 1,
the winter velocities and the individual glacier velocities have been
described earlier (Joughin et al., 2010; Moon et al., 2012). Here we
describe updates to these products and provide details related to several
new products.</p>
<?pagebreak page2214?><sec id="Ch1.S3.SS1">
  <title>GIMP products</title>
      <p id="d1e380">The oldest set of GIMP products presented here is a series of winter
velocity maps, which extend back to the winter of 2000–2001 and are derived
entirely from SAR data (Joughin, 2017b). For these maps, we define winter to
be the period with little or no melt, extending from 1 September to 31 May.
Many of these earlier GIMP winter velocity maps use campaign-mode data and
are hence derived from acquisitions spanning only a few months. The first
winter map to include Sentinel 1A data, available from late 2014,
was produced largely from data collected toward the latter half of the
2014–2015 winter. The 2015–2016 and 2016–2017 winter maps include data from
the full 9-month period along the coasts, with campaign coverage in the
interior.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F1"><caption><p id="d1e385">Annual velocity map for 2016 plotted over a SAR image mosaic. Arrows
indicate glaciers plotted in subsequent figures. The white outline shows the
area shown in Fig. 7. Red boxes show the locations of TerraSAR-X and
TanDEM-X scenes used in GIMP velocity maps.</p></caption>
          <?xmltex \igopts{width=199.169291pt}?><graphic xlink:href="https://tc.copernicus.org/articles/12/2211/2018/tc-12-2211-2018-f01.png"/>

        </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F2" specific-use="star"><caption><p id="d1e396"><bold>(a)</bold> Number of valid Sentinel 1A/B estimates made using data
collected over the period from January 2015 to September 2017. Standard
deviations <bold>(b)</bold> <inline-formula><mml:math id="M8" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mrow><mml:msub><mml:mi mathvariant="normal">v</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> and <bold>(c)</bold> <inline-formula><mml:math id="M9" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mrow><mml:msub><mml:mi mathvariant="normal">v</mml:mi><mml:mi>y</mml:mi></mml:msub></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> of velocity estimates collected
over the same period.</p></caption>
          <?xmltex \igopts{width=384.112205pt}?><graphic xlink:href="https://tc.copernicus.org/articles/12/2211/2018/tc-12-2211-2018-f02.png"/>

        </fig>

      <?pagebreak page2215?><p id="d1e444">Our individual glacier estimates (see red boxes in Fig. 1 for locations)
provide 11-, 22-, and 33-day “snapshot” estimates for many of Greenland's
fastest outlets, derived using data from DLR's TerraSAR-X and TandDEM-X
missions (Joughin et al., 2016a). At present these estimates cover the
period from 2009 to 2017, with future coverage dependent on data
availability. The high (1–3 m) single-look resolution of these X-band
instruments is such that of all of the GIMP products, these products have
the best resolution and short-term accuracy.</p>
      <p id="d1e447">Regular Sentinel-1A/B and Landsat 8 coverage now allows GIMP to produce
annually averaged velocity maps from 2015 onwards (Joughin, 2017a). To
temporally align these products with other GIMP products, each year extends
from December to November (e.g. the 2015 product extends from 1 December 2014 to 30 November 2015). Figure 1 shows the 2016 annual velocity map.
These annual products tend to have the best coverage because Landsat 8
data are often able to fill in those areas, primarily in the
high-accumulation areas of the south-east, where SAR methods consistently
produce gaps on some glaciers.</p>
      <p id="d1e450">The GIMP project also produces a routine set of monthly and quarterly
velocity maps as detailed in Table 1. This time series begins in December 2014 and includes Copernicus Sentinel 1A/B, TerraSAR-X/TanDEM-X, and
Landsat 8 data. For periods with daylight, the Landsat 8 data contribute
heavily to the results. By contrast, in winter some products are entirely
radar derived. For the spring and autumn quarterly products in particular, the
Landsat 8 data can contribute to the temporal skew because daylight
collection is skewed toward the early (autumn) or late (spring) part of the
period.</p>
</sec>
<sec id="Ch1.S3.SS2">
  <title>Sentinel 1 coverage and individual estimates</title>
      <p id="d1e459">The Copernicus Sentinel 1A/B satellites now provide routine coastal
sampling, with less frequent sampling in the interior during each winter.
Together, these satellites have mapped the velocity of many coastal areas
more than 100 times since late 2014 (Fig. 2a), exceeding the collective
coastal coverage of all prior SAR missions. A further advantage of the
Sentinel instruments is the fine (2.3 m) slant-range sampling of the
single-look data, which is second only to the TerraSAR-X/TanDEM-X
instruments. The azimuth sampling (13.9 m) of the Sentinel IW TOPS mode is
<inline-formula><mml:math id="M10" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 7 times coarser, however, than that of TerraSAR-X/TanDEM-X
and <inline-formula><mml:math id="M11" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 2.7 times coarser than that of RADARSAT 1. Resolution
has a direct effect on accuracy; hence the error in the azimuth (parallel to
the satellite track) component of motion typically is about a factor of 3.5
times worse than that in the range (cross-track) direction (see also
Mouginot et al., 2017). In many cases, the azimuth offset accuracy is
further degraded by ionospheric effects (Gray et al., 2000).</p>
      <p id="d1e476">Successful velocity estimation with speckle-tracking relies on maintaining
a strong interferometric correlation between images, which declines with the
time between image acquisitions due to processes such as melt and firn
compaction. As a consequence, the Sentinel 1A/B 6- and 12-day repeat
intervals greatly improve the ability to detect displacement relative to the
24-day repeat period of RADARSAT and the 35-day repeat periods of ENVISAT
and ERS-1/2 (when not in tandem or ice modes). This improvement is
particularly<?pagebreak page2216?> evident for high-accumulation coastal areas in the south-east
(Fig. 2a), where Sentinel 1 provides <inline-formula><mml:math id="M12" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 20 or more
measurements for regions in which all RADARSAT 1 data, collected over a
13-year period, provided few or no viable estimates (Joughin et al., 2017).</p>
      <p id="d1e486">Since displacement data are scaled by the observation interval used to
derive velocity, individual Sentinel 1A/B velocities derived using 6- and
12-day image pairs are relatively sensitive to errors that are uncorrelated
in time, such as those caused by the ionosphere. These errors, however, are
reduced when stacking (averaging) multiple estimates. To help assess the
errors of individual Sentinel 1A/B pairs, Fig. 2b and c shows the standard
deviations (<inline-formula><mml:math id="M13" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mrow><mml:msub><mml:mi mathvariant="normal">v</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:msub><mml:mo>,</mml:mo><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mrow><mml:msub><mml:mi mathvariant="normal">v</mml:mi><mml:mi>y</mml:mi></mml:msub></mml:mrow></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> of the individual
estimates collected from January 2015 and extending to
September 2017. For the interior of the ice sheet, where there is little or
no melt and speeds do not vary significantly, the means of the individual
standard deviations are <inline-formula><mml:math id="M14" display="inline"><mml:mrow><mml:msub><mml:mover accent="true"><mml:mi mathvariant="italic">σ</mml:mi><mml:mo mathvariant="normal">¯</mml:mo></mml:mover><mml:mrow><mml:msub><mml:mi mathvariant="normal">v</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:msub><mml:mo>=</mml:mo><mml:mn mathvariant="normal">6</mml:mn></mml:mrow></mml:math></inline-formula>.2 and <inline-formula><mml:math id="M15" display="inline"><mml:mrow><mml:msub><mml:mover accent="true"><mml:mi mathvariant="italic">σ</mml:mi><mml:mo mathvariant="normal">¯</mml:mo></mml:mover><mml:mrow><mml:msub><mml:mi mathvariant="normal">v</mml:mi><mml:mi>y</mml:mi></mml:msub></mml:mrow></mml:msub><mml:mo>=</mml:mo><mml:mn mathvariant="normal">17</mml:mn></mml:mrow></mml:math></inline-formula>.5 m yr<inline-formula><mml:math id="M16" 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>. The large difference between the <inline-formula><mml:math id="M17" display="inline"><mml:mi>x</mml:mi></mml:math></inline-formula> (east-west) and
<inline-formula><mml:math id="M18" display="inline"><mml:mi>y</mml:mi></mml:math></inline-formula> (north–south) components indicates the dominance of the azimuth errors,
which are more closely aligned with the north–south direction. These values
provide estimates of uncertainty for the individual velocity estimates under
relatively stable conditions, as is evident over the ice-free areas in
Fig. 2b. The data in Fig. 2b represent a mix of 6- (<inline-formula><mml:math id="M19" display="inline"><mml:mo lspace="0mm">∼</mml:mo></mml:math></inline-formula> 60 %), 12- (37 %) and 24-day (3 %) pairs. As a result, these values
should underestimate the uncertainty for 6-day pairs and overestimate it for
12-day or longer pairs.</p>
      <p id="d1e596">The causes of the large standard deviations in velocity for coastal areas
(reddish areas in Fig. 2b and c) are more complicated because some of the
variability indicates actual variations in speed, such as seasonal
variability and marine-terminating glacier dynamics. Close inspection of the
data, however, reveals that much of the variability, especially on slow-moving
coastal areas, is due to noise. In these areas, surface melting and
other changes (e.g. high firn compaction rates) lead to weaker intra-pair
correlation and, thus, noisier estimates.</p>
      <p id="d1e600">Although the results shown in Fig. 2b and c are representative of mean
performance, there is substantial variability in data quality, with some
estimates being much better than others. For this reason, we expect the
temporally aggregated, error-weighted averages described above to yield much
lower errors in aggregated velocity maps relative to unweighted averaging.
In areas where there is both ascending and descending coverage, we reduce
errors further by including offsets derived entirely from crossing
range-offset data as described above.</p>
</sec>
<sec id="Ch1.S3.SS3">
  <title>Resolution and systematic differences</title>

      <?xmltex \floatpos{t}?><fig id="Ch1.F3" specific-use="star"><caption><p id="d1e612">Profiles of speed from Sverdrup Glacier (see Fig. 1 for
location) along the <bold>(a)</bold> transverse (A-A<inline-formula><mml:math id="M20" display="inline"><mml:msup><mml:mi/><mml:mo>′</mml:mo></mml:msup></mml:math></inline-formula>) and <bold>(b)</bold> longitudinal (B-B<inline-formula><mml:math id="M21" display="inline"><mml:msup><mml:mi/><mml:mo>′</mml:mo></mml:msup></mml:math></inline-formula>)
profiles shown in the inset. The speeds were calculated using individual
TerraSAR-X (TSX) and Sentinel 1A/B (S1) pairs collected in early summer
2017.</p></caption>
          <?xmltex \igopts{width=355.659449pt}?><graphic xlink:href="https://tc.copernicus.org/articles/12/2211/2018/tc-12-2211-2018-f03.png"/>

        </fig>

      <p id="d1e645">Figure 3 shows a comparison of individual Sentinel 1A/B and TerraSAR-X
velocity estimates for transverse and longitudinal profiles (see inset) from
Sverdrup Glacier (see Fig. 1 for location) in north-west Greenland. All of
these data were collected over a <inline-formula><mml:math id="M22" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 3-week period in the summer
of 2017. The transverse-profile data (Fig. 3a) indicate summer speed-up of
about 100 to 200 m yr<inline-formula><mml:math id="M23" 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> over the period covered by the data. For estimates
that are nearly coincident in time, there is agreement between the
TerraSAR-X and Sentinel 1A/B data toward the centre of fast flow and in the
adjacent, slow-moving areas. Along the shear margins, however, there are
systematic differences of up to <inline-formula><mml:math id="M24" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 700 m yr<inline-formula><mml:math id="M25" 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>. For the most part,
these differences can largely be attributed to differences in the sensor
resolution. With an adequate cross-correlation window size and further
smoothing to improve accuracy, the effective azimuth-direction resolution is
<inline-formula><mml:math id="M26" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 1.5 km for Sentinel 1 A/B and 460 m for TerraSAR-X. As a
result, the TerraSAR-X data track the sharp gradients at the shear margins,
while Sentinel 1A/B tends to smooth over them.</p>
      <p id="d1e693">Figure 3b plots data for a longitudinal profile down Sverdrup Glacier. Over
most of the profile, the data agree to within roughly the level of
uncertainty indicated by the error bars and any seasonal variation. The
error bars represent the random errors for individual estimates, which are
uncorrelated from one estimate to the next. Examination of the data,
however, indicates that some of the differences between the profiles is
sensor-specific rather than random. Some of these differences are
attributable to the different resolutions as just described. Other sources
of systematic error, however, may be present. For example, the DEM used for
the surface parallel flow correction can introduce slope-dependent errors
that depend on the imaging geometry (i.e. results from the same sensor with
the same viewing geometry have a common error). For past products, we have
assumed a worst-case error of about 3 % or <inline-formula><mml:math id="M27" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 30 to 90 m yr<inline-formula><mml:math id="M28" 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>
for the speeds shown in Fig. 3, which is of similar magnitude to the
observed differences. For these products, however, we expect improved
performance based on the quality of the latest GIMP DEM (Howat, 2017).
Because these errors are mixed in with the resolution errors, it is
difficult to isolate and quantify each source of error.</p>
      <p id="d1e715">We also note that the accuracy of the DEM determines the geolocation
accuracy of the final results (<inline-formula><mml:math id="M29" display="inline"><mml:mo lspace="0mm">∼</mml:mo></mml:math></inline-formula> 1.25 m horizontal location
error for each 1 m of elevation error). For areas similar to the Sverdrup
Glacier example, where thinning rates are small, geolocation errors have a
negligible impact on the results. In areas of rapid thinning and strong
velocity gradients, such as Jakobshavn Isbræ, the surface height at the
time of data acquisition may substantially differ from that of the DEM,
resulting in significant geolocation errors. Since the tens of metres per
year variability of Jakobshavn Isbræ make it an extreme case, we have
mitigated the resulting errors in TerraSAR-X products using annually updated
DEMs for this glacier.</p>
</sec>
<sec id="Ch1.S3.SS4">
  <?xmltex \opttitle{Outlet glaciers: Jakobshavn Isbr{\ae} and K{\o}ge Bugt}?><title>Outlet glaciers: Jakobshavn Isbræ and Køge Bugt</title>
      <p id="d1e732">As indicated in Table 1, GIMP provides several data sets at a variety of
spatial and temporal resolutions generated from multiple sensors, covering
overlapping periods. To better<?pagebreak page2217?> understand the temporal consistency of these
data sets for outlet glacier studies, here we examine the speeds over a
9-year period, during which there is substantial overlap of the various data
sets. In particular, we focus on Jakobshavn Isbræ and Køge Bugt. Although
some intercomparison for a more limited set of the Jakobshavn Isbræ data
has been presented elsewhere (Joughin et al., 2012; Lemos et al., 2018), we
present a more comprehensive intercomparison here. Køge Bugt is estimated
to be the glacier with the third greatest imbalance in Greenland for the
period 2000 to 2012 (Enderlin et al., 2014), making its record of flow
variability of interest for understanding ice loss. Finally, with high
strain rates and as two of the fastest glaciers in Greenland, they represent
some of the most difficult areas to map, providing a robust demonstration of
GIMP's measurement capabilities.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F4" specific-use="star"><caption><p id="d1e737">Speeds for Jakobshavn Isbræ at the points M6, M13, and M20 shown in
the inset over the periods from <bold>(a)</bold> 2007 to 2017 and <bold>(b)</bold> January 2015 to
December 2017. Results show individual TerraSAR-X/TanDEM-X (triangles) and
Sentinel 1A/B estimates (circles). Also shown are the aggregate monthly
(squares) and winter (diamonds) products, which take advantage of all
available data. For clarity we omitted the annual and quarterly products
listed in Table 1. Error bars also are omitted because they are small
relative to the plot marker size.</p></caption>
          <?xmltex \igopts{width=355.659449pt}?><graphic xlink:href="https://tc.copernicus.org/articles/12/2211/2018/tc-12-2211-2018-f04.png"/>

        </fig>

      <p id="d1e752">Figure 4a shows the Jakobshavn Isbræ time series for the last decade
plotted using many of the GIMP products listed in Table 1. The labels of the
points on the main trunk (see M6, M13, and M20 in inset) give their
approximate distance in kilometres from the 2004 terminus, which we use for
consistency with earlier work (Joughin et al., 2012, 2008b, 2014). As
previously noted, there is a strong annual cycle of speed-up, coinciding with
summer retreats of the terminus, followed by slowdown during the winter
re-advances. A new finding is that the summertime (maximum) speeds have
declined since 2012, and the summer 2017 peak is the slowest for the period
shown in Fig. 4. Moreover, this peak was actually slower than the winter
2016 minimum and just slightly faster than 2015 winter minimum.</p>
      <p id="d1e756">To facilitate a more detailed comparison of the data, Fig. 4b shows the
period from January 2015 to December 2017. The good agreement in this figure
between the monthly and 11-day TerraSAR-X/TanDEM-X data largely reflects the
dominant contribution of the X-band data to the monthly time series. For the
two fastest points (M6 and M13), Sentinel 1A provides no valid measurements
in the early part of the time series. Once Sentinel 1B acquisitions
commenced in October 2016, however, the 6-day sampling began providing
estimates for the faster-flowing ice. At all three points, the Sentinel data
provide close agreement with the TerraSAR-X/TanDEM-X data consistently with
other independent Sentinel 1A/B estimates (Lemos et al., 2018).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F5" specific-use="star"><caption><p id="d1e761">Speeds for the glacier discharging ice through to Køge Bugt at the
points M6, M13, and M20 shown in the inset over the periods from <bold>(a)</bold> 2007 to
2017 and <bold>(b)</bold> January 2015 to December 2017. Results show individual
TerraSAR-X/TanDEM-X (triangles) and Sentinel 1A/B estimates (circles). Also
shown are the aggregate monthly (squares) and winter (diamonds) products,
which take advantage of all available data. For clarity we omitted the
annual and quarterly products listed in Table 1. Error bars also are omitted
because they are small relative to the plot marker size.</p></caption>
          <?xmltex \igopts{width=355.659449pt}?><graphic xlink:href="https://tc.copernicus.org/articles/12/2211/2018/tc-12-2211-2018-f05.png"/>

        </fig>

      <p id="d1e776">Figure 5a shows the variation in speed at approximately 3, 6, and 9 km (see
KB3, KB6, and KB9 in the inset) from the 2017 terminus position of a large
unnamed glacier that discharges ice through Køge Bugt (bay). In contrast to
Jakobshavn Isbræ, there is no clear seasonal signal, although the speed
changes substantially on timescales of a few years. From 2007 to 2009, KB3
sped up from just over 6 to nearly 10 km yr<inline-formula><mml:math id="M30" 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>. For the next few years
the speed at KB3 remained relatively constant before peaking briefly at 11 km yr<inline-formula><mml:math id="M31" 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> in 2012,
after which it slowed to <inline-formula><mml:math id="M32" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 7.4 km yr<inline-formula><mml:math id="M33" 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> by May 2013. This decline was followed by another speed-up to <inline-formula><mml:math id="M34" display="inline"><mml:mo>&gt;</mml:mo></mml:math></inline-formula> 10 km yr<inline-formula><mml:math id="M35" 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>
by spring 2015. Speeds then dipped to <inline-formula><mml:math id="M36" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 6.8 km yr<inline-formula><mml:math id="M37" 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> in autumn 2016
but picked up again soon after. The prominent signal at KB3 is far more
muted at points inland, with speeds 6 km upstream at KB9, staying within the
range of 3 to 4 km yr<inline-formula><mml:math id="M38" 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>.</p>
      <?pagebreak page2218?><p id="d1e873">Figure 5b shows the same Køge Bugt data over the period from 2015 to 2017.
Relative to Jakobshavn Isbræ, the Køge Bugt glacier was sampled far less
frequently with TerraSAR-X, so there are several gaps in this time series,
especially during the non-summer months. As with Jakobshavn Isbræ, the
12-day Sentinel 1A sampling prior to October 2016 did not yield valid
measurements for the two fastest points (KB3 and KB6). Farther inland at
KB9, the 12-day Sentinel data worked well, with almost every possible pair
yielding velocity estimates. The missing points in 2015 at KB9 are largely
due to the Sentinel 1A acquisition schedule.</p>
      <p id="d1e876">In general, the points from the different sensors agree well, although close
inspection does indicate that there are some small biases. For example, the
summer 2017 speeds at KB9 measured with TerraSAR-X (red triangles) are
consistently about 200 m yr<inline-formula><mml:math id="M39" 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> slower than those measured with Sentinel 1
(green circles). Although small, this bias is larger than the expected level
of error (<inline-formula><mml:math id="M40" display="inline"><mml:mo lspace="0mm">&lt;</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M41" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 100 m yr<inline-formula><mml:math id="M42" 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>). Differences of similar
magnitude occur at M13 on Jakobshavn Isbræ. In both cases, these
differences likely result from differing sensor resolution, as described
above.</p>
</sec>
<sec id="Ch1.S3.SS5">
  <title>North-west and south-east</title>
      <p id="d1e923">Numerous glaciers have sped up in Greenland (Joughin et al., 2010; Moon et
al., 2012; Rignot and Kanagaratnam, 2006), which is well documented by the
GIMP data set. Many of these speed-ups have been concentrated in north-west
and south-east Greenland. To demonstrate the collective behaviour of
north-west glaciers, Fig. 6a shows a stack (summed speeds) plot for the 43 glaciers (excluding Jakobshavn Isbræ), for which there is good temporal
coverage over the 16-year period. Figure 6b shows a similar plot for 29
glaciers in south-east Greenland. For each glacier, we sampled the centre of
the main trunk at a point a few kilometres up stream of its terminus. We
did not use a fixed distance because the position of many the termini
vary secularly or seasonally by up to several kilometres over the period
covered by the data set.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F6" specific-use="star"><caption><p id="d1e928">Summed speeds for collections of glaciers in <bold>(a)</bold> north-west and <bold>(b)</bold> south-east
Greenland. For these plots the bottom curve represents the speed
of the first glacier (58 for the north-west). The next curve from the bottom
is the sum of the first glacier and the second (58<inline-formula><mml:math id="M43" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula>56 for the north-west).
Each successive curve is then the sum of the next glacier added to the
cumulative sum of the previous glaciers. The legend identifies individual
glaciers using the glacier IDs (numbers) used for the GIMP terminus position
data set (Moon and Joughin, 2008; Moon et al., 2015). Figure S1 in the Supplement shows the
location of each numbered glacier. Because Jakobshavn represents such a
large signal (Fig. 3), we did not include it the north-west data. For a few
glaciers, data are missing for some of the years plotted. In these cases, the
stack is arranged with missing points on top so that data on either side
bridge the gap.</p></caption>
          <?xmltex \igopts{width=412.564961pt}?><graphic xlink:href="https://tc.copernicus.org/articles/12/2211/2018/tc-12-2211-2018-f06.png"/>

        </fig>

      <p id="d1e950">As shown in Fig. 6, from 2000–2001 to 2016–2017 these glaciers collectively
sped up by 38  and 41 % for north-west and south-east Greenland. (Percentage speed-up is calculated as the change in cumulative
speed.) Although the degree of regional speed-up is similar, its timing
differs. In north-west<?pagebreak page2219?> Greenland, the speed-up was only 7 % from 2000–2001 to
2005–2006, but there was an increase of 29 % over the next 11 years. By
contrast, in south-east Greenland the majority of the speed-up occurred over
the first half of the observation interval (by 29 % from 2000–2001 to
2008–2009). Over the last 8 years, glaciers only sped up by a more modest
9 %, mostly due to increases in speed from 2015–2006 to 2016–2017.</p>
</sec>
<sec id="Ch1.S3.SS6">
  <title>Decadal-scale ice sheet trends in south-west Greenland</title>

      <?xmltex \floatpos{p}?><fig id="Ch1.F7"><caption><p id="d1e961"><bold>(a)</bold> Speed along a section of the south-west ice-sheet margin and
<bold>(b)</bold> significant (<inline-formula><mml:math id="M44" display="inline"><mml:mi>p</mml:mi></mml:math></inline-formula> <inline-formula><mml:math id="M45" display="inline"><mml:mo>&lt;</mml:mo></mml:math></inline-formula> 0.05) trends (colour) for the period from winter
2000–2001 to 2016–2017 calculated for the area enclosed by the white outline.
Within the outline, grey indicates no significant trend (<inline-formula><mml:math id="M46" display="inline"><mml:mrow><mml:mi>p</mml:mi><mml:mo>≥</mml:mo><mml:mn mathvariant="normal">0</mml:mn></mml:mrow></mml:math></inline-formula>.05). The
underlying grey-scale image is a SAR image from RADARSAT (Joughin et al.,
2016b). Bright radar returns upstream of the outline generally indicate
percolation facies, while darker tones within the outline indicate bare-ice
or wet-snow facies (Fahnestock et al., 1993). The circles (SW1-3, and NL)
indicate the locations for data plotted in Fig. 8. The black rectangle
shows the approximate area examined by Tedstone et al. (2015), which we
refer to as T2015 in the text. The 700 (magenta) and 1100 (black) elevation
contours are also shown.
</p></caption>
          <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://tc.copernicus.org/articles/12/2211/2018/tc-12-2211-2018-f07.jpg"/>

        </fig>

      <p id="d1e1001">Earlier work indicated that an area of the land-terminating margin of the
Greenland Ice Sheet is slowing down, possibly as the result of a more
efficient basal drainage network that has evolved to accommodate recent
increases in melt (Tedstone et al., 2015). The black rectangles in Fig. 7
show the location of this region, which we refer to as T2015. Although the
data from that study extend over a much longer interval than the GIMP data,
all of the significant change occurred since 2000, which closely matches
the period covered by GIMP. Thus, we use the GIMP data to explore the
hypothesis that the changes observed by the previous study were
representative of the behaviour of the south-west sector as a whole. We use
the winter data set for this analysis because it provides the longest time
span. As noted above, we employ control points in the interior of the ice
sheet where we expect the change to be small, which could bias the results. To
help avoid this problem, we restrict our analysis to slow-flowing (Fig. 7a)
areas where the elevation is less than 1400 m (see white outline
Figs. 1 and 7), which we know to be near the coast and thus well
constrained by bedrock control points. As Fig. 7 indicates, this region
roughly corresponds to the bare-ice and wet-snow zones (Fahnestock et al.,
1993), where substantial melt and lake drainage occur.</p>
      <p id="d1e1004">Figure 7b shows the spatial distribution (colour) of statistically
significant (<inline-formula><mml:math id="M47" display="inline"><mml:mrow><mml:mi>p</mml:mi><mml:mo>≤</mml:mo><mml:mn mathvariant="normal">0</mml:mn></mml:mrow></mml:math></inline-formula>.05) trends in our study area. In the southernmost
part of the region, there is a strong speed-up trend associated with the
large outlet glacier, Narsap Sermia. Similarly, there is a strong positive
trend where the top part of the region borders Jakobshavn Isbræ. In the
T2015 region (see black rectangle in Fig. 7), we find some indication of
slowdown, but the trends are less than those estimated by Tedstone et al. (2015).
One land-terminating glacier displays<?pagebreak page2220?> a pronounced slowdown (SW3 in Fig. 7),
but the slowing is confined to near the terminus. Any trends for the
rest of the region are small and scattered.</p>
      <p id="d1e1019">The results in Fig. 7 indicate where significant (<inline-formula><mml:math id="M48" display="inline"><mml:mrow><mml:mi>p</mml:mi><mml:mo>≤</mml:mo><mml:mn mathvariant="normal">0</mml:mn></mml:mrow></mml:math></inline-formula>.05) trends occur
(e.g. those that are unlikely to be false alarms). The results do not
answer the question of whether given data with a trend of <inline-formula><mml:math id="M49" display="inline"><mml:mi>X</mml:mi></mml:math></inline-formula> m yr<inline-formula><mml:math id="M50" 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> can
we reliably detect a non-zero trend of magnitude <inline-formula><mml:math id="M51" display="inline"><mml:mi>X</mml:mi></mml:math></inline-formula> above the noise (missed
detections). As an extreme example, if the trend was 0.01 m yr<inline-formula><mml:math id="M52" 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> and
the noise was 100 m yr<inline-formula><mml:math id="M53" 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>, then the confidence test should fail 95 % of
the time and we would miss such a weak trend. Thus, in interpreting Fig. 7, it is important to understand how small a trend we can detect given our
level of noise and sampling strategy. (We assume that our noise is
substantially larger than any natural variability.)</p>
      <p id="d1e1086">To establish the detection capability of our time series, we ran Monte Carlo
simulations in which we added Gaussian noise to specified linear trends,
sampled during the same years in which we had data (see Fig. S2). In these
simulations, we assume a velocity vector (<inline-formula><mml:math id="M54" display="inline"><mml:mo lspace="0mm">∼</mml:mo></mml:math></inline-formula> 100 m yr<inline-formula><mml:math id="M55" 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>) that is
directed along the <inline-formula><mml:math id="M56" display="inline"><mml:mi>x</mml:mi></mml:math></inline-formula> axis. We evaluated several cases in which the magnitudes of
the errors are equal in both direction (2.5–20 m yr<inline-formula><mml:math id="M57" 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>). The magnitudes of our
errors, however, are direction dependent (mean errors of <inline-formula><mml:math id="M58" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mi>x</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn mathvariant="normal">2.9</mml:mn></mml:mrow></mml:math></inline-formula>
and <inline-formula><mml:math id="M59" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mi>y</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn mathvariant="normal">6.1</mml:mn></mml:mrow></mml:math></inline-formula> m yr<inline-formula><mml:math id="M60" 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> for the area in Fig. 7). When computing speed,
the error is almost entirely dominated by the component of uncertainty
directed along flow. In our case, the mean component of error in the
direction of flow is 3.7 m yr<inline-formula><mml:math id="M61" 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>, with 5.6 m yr<inline-formula><mml:math id="M62" 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> in the cross-flow direction.
Thus, we ran our simulations with a typical flow direction (<inline-formula><mml:math id="M63" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mi>x</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn mathvariant="normal">3.7</mml:mn></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M64" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mi>y</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn mathvariant="normal">5.6</mml:mn></mml:mrow></mml:math></inline-formula> m yr<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>), best-case flow direction (<inline-formula><mml:math id="M66" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mi>x</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn mathvariant="normal">2.9</mml:mn></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M67" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mi>y</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn mathvariant="normal">6.1</mml:mn></mml:mrow></mml:math></inline-formula> m yr<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>), and worst-case flow direction
(<inline-formula><mml:math id="M69" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mi>x</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn mathvariant="normal">2.9</mml:mn></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M70" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mi>y</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn mathvariant="normal">6.1</mml:mn></mml:mrow></mml:math></inline-formula> m yr<inline-formula><mml:math id="M71" 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>). These simulations
(Fig. S2) indicate that if the entire region had a uniform trend of 1.0 m yr<inline-formula><mml:math id="M72" 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>, then
with <inline-formula><mml:math id="M73" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mi>x</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn mathvariant="normal">3.7</mml:mn></mml:mrow></mml:math></inline-formula> m yr<inline-formula><mml:math id="M74" 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> we would detect a significant trend 94 % of
the time, while with <inline-formula><mml:math id="M75" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mi>x</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn mathvariant="normal">6.1</mml:mn><mml:mspace linebreak="nobreak" width="0.125em"/></mml:mrow></mml:math></inline-formula> m yr<inline-formula><mml:math id="M76" 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> the detection rate drops to
58 %. For a trend of 1.5 m yr<inline-formula><mml:math id="M77" 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>, the detection rate is 89 % with <inline-formula><mml:math id="M78" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mi>x</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn mathvariant="normal">6.1</mml:mn></mml:mrow></mml:math></inline-formula>, dropping to 50 % for <inline-formula><mml:math id="M79" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mi>x</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn mathvariant="normal">10</mml:mn></mml:mrow></mml:math></inline-formula> m yr<inline-formula><mml:math id="M80" 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>, which is well above
the expected level of error.</p>
      <?pagebreak page2221?><p id="d1e1444">While Fig. 7 provides detail about the spatial distribution of trends, it
reveals little about the nature of those trends. To provide more detail,
Fig. 8 shows the full winter time series for four points (NL, SW1, SW2,
SW3) shown in Fig. 7. The first point, NL (North Lake) corresponds to an
area on the ice sheet were GPS data have been collected over a multi-year
period (Joughin et al., 2008a; Stevens et al., 2016). While only a few
months of each winter are measured by GIMP, the GPS data measure flow over
the <inline-formula><mml:math id="M81" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 9-month period with little or no melt. Despite this
difference in sampling, most of the GPS points agree well with the
radar-derived speeds. Although the GPS data suggest a weak trend of <inline-formula><mml:math id="M82" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>1.3 m yr<inline-formula><mml:math id="M83" 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> (<inline-formula><mml:math id="M84" display="inline"><mml:mrow><mml:mi>p</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0</mml:mn></mml:mrow></mml:math></inline-formula>.06),
the longer radar record reveals no significant trend.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F8" specific-use="star"><caption><p id="d1e1487">Winter velocities and corresponding trends for the points SW1–3
and NL (see Fig. 7 for location) with error bars from the formal error
estimates that are distributed with the velocity estimates. Also shown are
GPS derived speeds at NL (Stevens et al., 2016).</p></caption>
          <?xmltex \igopts{width=312.980315pt}?><graphic xlink:href="https://tc.copernicus.org/articles/12/2211/2018/tc-12-2211-2018-f08.png"/>

        </fig>

      <p id="d1e1496">The point SW1 is located in the T2015 region and it has a trend <inline-formula><mml:math id="M85" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>1.2 m yr<inline-formula><mml:math id="M86" 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> (<inline-formula><mml:math id="M87" display="inline"><mml:mrow><mml:mi>p</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0</mml:mn></mml:mrow></mml:math></inline-formula>.02), which explains about half of the variance in the
speed (<inline-formula><mml:math id="M88" display="inline"><mml:mrow><mml:msup><mml:mi>r</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0</mml:mn></mml:mrow></mml:math></inline-formula>.54). Farther to the south at SW2, there is a significant
acceleration trend (1.3 m yr<inline-formula><mml:math id="M89" 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>, <inline-formula><mml:math id="M90" display="inline"><mml:mrow><mml:msup><mml:mi>r</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0</mml:mn></mml:mrow></mml:math></inline-formula>.47). Downstream of this
point, there is a slowdown trend at SW3 (<inline-formula><mml:math id="M91" display="inline"><mml:mo lspace="0mm">-</mml:mo></mml:math></inline-formula>4.0 m yr<inline-formula><mml:math id="M92" 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>) but with a high
degree of interannual variability (<inline-formula><mml:math id="M93" display="inline"><mml:mrow><mml:msup><mml:mi>r</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0</mml:mn></mml:mrow></mml:math></inline-formula>.37).</p>
</sec>
</sec>
<sec id="Ch1.S4">
  <title>Discussion</title>
      <p id="d1e1615">We have presented data at several sites around Greenland. Here we discuss
the results in the context of overall data quality as well as the processes
that contributed to the behaviour at each site.</p>
<sec id="Ch1.S4.SS1">
  <title>Data quality</title>
      <p id="d1e1623">Overall the times series shown in Figs. 4–8 indicate a high level of
temporal consistency between data sets. Such consistency is important for
tracking and understanding changes in glacier speeds on timescales of weeks
to decades. Although Jakobshavn Isbræ has some of the most rapidly varying
seasonal behaviour, the monthly time series captures this variability nearly
as well as the 11- and 12-day individual estimates. To the extent that
points in the finer-resolution time series depart from the monthly data at
both Jakobshavn and Køge Bugt, it is not always clear whether the data
reveal actual short-term behaviour (e.g. response to a calving event) or
instead are the result of noise.</p>
      <p id="d1e1626">Relative to the individual snapshot estimates, the monthly time series
provide the advantage of greater accuracy through averaging of multiple
estimates. As mentioned above, this accuracy comes at the expense of
potential deviation of the actual time stamp from the nominal time stamp.
Inspection of the results in Figs. 4 and 5, however, reveals no detectable
skew of the monthly data relative to individual estimates. Some of the
winter estimates deviate from the more frequently sampled data, but this
behaviour is due to averaging of a rapidly varying signal rather than
temporal skew in the data. Thus, the data indicate that the trade-off made
between accuracy and temporal resolution may often favour the monthly time
series for studies on seasonal variation. Exceptions may occur when trying
to study and isolate the effect of specific events (e.g. high melt or
calving), where the finer temporal resolution becomes important.
Nonetheless, in such cases the observed change needs to stand well above the
expected level of uncertainty.</p>
      <p id="d1e1629">Although the results reveal that the multi-sensor data sets work well for
studying glacier changes, Fig. 3 reveals some potential pitfalls for
process studies. For example, the smoothed velocity estimates across shear
margins from the Sentinel 1A/B data could yield unreliable results when
using<?pagebreak page2222?> the data to constrain a model to invert for basal shear stress.
Without conducting a detailed sensitivity study, it is difficult to assess
how much the results would be degraded using Sentinel 1A/B data instead of
TerraSAR-X data in any given application. Qualitatively, however, Fig. 3
indicates that if a study needs data that capture high strain rates, then
the finer-resolution TerraSAR-X velocities are preferred. This statement
applies to a relatively small fraction (<inline-formula><mml:math id="M94" display="inline"><mml:mo lspace="0mm">∼</mml:mo></mml:math></inline-formula> 1 % or less) of
the ice sheet (i.e. fast outlets). In other areas, the accuracy obtained by
averaging large numbers (e.g. Fig. 2a) of estimates may weigh in favour
of using the results that include Sentinel 1A/B data.</p>
</sec>
<sec id="Ch1.S4.SS2">
  <?xmltex \opttitle{Jakobshavn and K{\o}ge Bugt}?><title>Jakobshavn and Køge Bugt</title>
      <p id="d1e1646">The much slower 2016–2017 winter minimum and 2017 summer maximum seen in
Fig. 4a indicate a major recent slowdown at Jakobshavn Isbræ. To help
examine the cause of this slowdown, Fig. 9a shows the history of the terminus
position plotted relative to the glacier geometry, which is an update to an
earlier time series (Joughin et al., 2014). The ice thickness of Jakobshavn
Isbræ is exceptionally difficult to measure and several maps have been
published with substantial differences in bed topography (An et al., 2017;
Morlighem et al., 2017), with those differences being especially large along
any particular profile along-flow. Profiles that follow the greatest bed
depth for a particular DEM, however, show similar overdeepenings between
data sets. Thus, for consistency with past work, we use the Plummer et al. (2008) bed model and caution that the uncertainty in bed topography renders
the interpretation somewhat qualitative as would be the case with other bed
DEMs for this region.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F9"><caption><p id="d1e1651"><bold>(a)</bold> Surface and bed elevation, terminus (2009–2017), and
flotation height for Jakobshavn Isbræ updated from a similar figure
(Joughin et al., 2014). The bed data are from CRESIS (Plummer, 2008) and the
surface elevations are from the NASA Airborne Topographic Mapper (ATM)
(Krabill et al., 2004) and WorldView DEMs (Noh and Howat, 2015). <bold>(b)</bold> Surface
and bed elevation and terminus position for Køge Bugt. The surface
elevations are from the GIMP DEM (Howat, 2017), and the bed elevations are
from Bedmap 3 (Morlighem et al., 2017).</p></caption>
          <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://tc.copernicus.org/articles/12/2211/2018/tc-12-2211-2018-f09.png"/>

        </fig>

      <?pagebreak page2223?><p id="d1e1665">Past work has shown that the strong seasonal variations in speed on
Jakobshavn Isbræ correspond to the retreat and advance of the
often-grounded terminus across a basal overdeepening (Joughin et al., 2012,
2014). This earlier work demonstrated that, as the grounded-terminus height
changes, the sensitivity of the speed to the pressure boundary condition at
the terminus is sufficient to explain much of the seasonal variation. Over
the course of the seasonal cycle, the speed increases as the terminus
recedes into deeper water each summer and slows each winter as it advances
into shallower water (see Fig. 9a). Peak summer speeds occurred in 2012,
when the terminus retreated to the deepest point of the overdeepening. In
subsequent summers, the terminus retreated past the overdeepening to
shallower water, yielding smaller summer peaks.</p>
      <p id="d1e1669">In the winter of 2016–2017 the terminus advanced nearly 5 km farther seaward
than any time since the 2009–2010 winter, coinciding with speeds that were
at least 900 m yr<inline-formula><mml:math id="M95" 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> slower than all winter minima since 2008 (Fig. 4).
Through much of this advance, the terminus likely was floating (see orange
curve Fig. 9a), so the buttressing provided by the longer floating tongue
should have contributed to reducing the speeds relative to recent winters.
Speeds would also have been reduced if the extended terminus grounded on the
shallower areas downstream of the overdeepening in the latter part of the
2016–2017 winter.</p>
      <p id="d1e1684">In the summer of 2017, the terminus retreated inland by 1–2 km less
than it had during the five prior summers. Although the points of maximum
terminus retreat were similar for the summers of 2011 and 2017, the maximum
speed in 2017 was <inline-formula><mml:math id="M96" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 1800 m yr<inline-formula><mml:math id="M97" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> slower than in 2011. This
difference may be due to the ungrounding of the area above the terminus from
2011 to 2017. The terminus appears to have been grounded in water
<inline-formula><mml:math id="M98" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 1250 m deep in 2011, yielding a strong summer peak due to
the non-linear relation between speed and ice thickness (Howat et al., 2005;
Joughin et al., 2012). By 2017, the grounding line appears to have retreated
to the local high above the overdeepening (<inline-formula><mml:math id="M99" display="inline"><mml:mo lspace="0mm">∼</mml:mo></mml:math></inline-formula> 975 m depth at
<inline-formula><mml:math id="M100" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 12.2 km in Fig. 9a), with a floating terminus extending a
few kilometres farther downstream. The combination of this thinner ice at
the grounding line and the additional buttressing provided by the floating
ice tongue should be of sufficient magnitude to explain much of the
reduction in peak summer speed from 2011 to 2017. Other factors such as the
rapidly evolving ice-sheet geometry and changes in effective pressure at the
bed may also have played a role that could either enhance or suppress the
effects of changes in grounding-line/terminus thickness (Joughin et al.,
2012).</p>
      <p id="d1e1727">It is unclear whether external forcing, internal dynamics, or some
combination of both have contributed to the changes in terminus extent that
have produced the recent slowdown. Temperature records from the nearby
coastal station at Egedesminde indicate that 2017 was the second coldest
year, behind 2015, in the 21st century (GISS, 2018). Colder
temperatures should have produced a more rigid iceberg melange or extended
the period over which the melange was rigid, which could have suppressed
calving, allowing greater terminus advance (Amundson et al., 2010; Joughin et
al., 2008b). Cooler temperatures also may have suppressed calving through a
reduction in melt-driven hydrofracturing (Sohn et al., 1998). Thus, one
plausible hypothesis is that the recent colder temperatures may have
contributed to the advance and slowdown, although if there was cooler water
at the terminus it could have played a role as well. Whether this slowdown
could reduce summer thinning and increase winter thickening sufficiently to
stabilize the glacier over scales of years to decades is unclear.</p>
      <p id="d1e1730">Figure 9b shows the variation in terminus position and surface and bed
elevation profiles for the Køge Bugt glacier. Unlike at Jakobshavn Isbræ,
the bed of this glacier rises above sea level within several kilometres of
the terminus (between KB3 and KB6). In the region upstream of approximately
4 km in Fig. 9b, the bed is determined using mass-conservation methods
constrained by ice velocity and radar depth-sounding data (Morlighem et al.,
2017). Downstream of the terminus, bed depths are far more uncertain due to
limited availability of bathymetric data. The terminus position data show
good correspondence with the speed record (Fig. 5), with slow speeds
corresponding to times when the terminus advanced. With the uncertain nature
of the bed in the region over which this advance occurred, the terminus
could have been grounded or floating as it migrated. In some of the images
used to digitize the terminus position, large tabular icebergs were present,
suggesting that, at least at times, the terminus was at or near flotation.
Whether grounded or floating, it likely is that the extra resistance
provided by the terminus advance produced the slower periods of flow,
similar to the case for Jakobshavn. The response at 6 km inland
(KB9) of KB3 is far more muted than the response a similar distance inland
on Jakobshavn Isbræ. This difference in behaviour may be due to the much
thinner ice at Køge Bugt, since the distance a stress perturbation at the
terminus is transmitted upstream should scale with ice thickness (Cuffey and
Paterson, 2010).</p>
      <p id="d1e1733">With the exception of its brief advances, the Køge Bugt terminus maintained
a relatively fixed position over nearly a decade, apparently near the top of
an overdeepening. Although this glacier appears to have been losing mass
rapidly between 2000 and 2012 (Enderlin et al., 2014), it seems unlikely
that there could have been strong thinning near the terminus over the period
since 2009. Any sustained thinning likely would have caused the terminus to
retreat down the reverse slope to the higher ground on the other side of the
overdeepening, from which point retreat would have been slowed or stopped by
the forward slope and elevations above sea level. The apparent loss measured
by Enderlin et al. (2014) was computed as a discharge anomaly relative to
2000, at which time speeds where similar to the minima seen in Fig. 4.
Thus, if the minimum in 2000 represents an anomalously slow period when the
glacier might even have been gaining mass, then the Køge Bugt glacier may be
losing mass far less quickly than previously indicated (Enderlin et<?pagebreak page2224?> al.,
2014), which is consistent with the terminus position data in Fig. 9.</p>
      <p id="d1e1736">It is interesting to compare Køge Bugt and Jakobshavn Isbræ and their
relation to their respective topographic settings. If the recent slowdown is
not the beginning of a period of stabilization, then the terminus of
Jakobshavn Isbræ likely will continue to retreat at least 60 km inland
until it recedes from the trough's deeper parts (Joughin et al., 2012). Once
this retreat occurs, the terminus would be in a position more like that of
Køge Bugt, which has almost completely pulled back out of its trough. Yet
the speeds of both glaciers are similar in magnitude. In the case of Køge Bugt, the glacier is able to maintain high slopes and driving stresses to
produce the high speed necessary to drain the high accumulation along the
south-east coast, despite the fact that much of this flow is over a bed well
above sea level. This behaviour indicates that once the terminus of
Jakobshavn Isbræ reaches the shallower part of its trough, it too may be
able to maintain a similar equilibrium.</p>
      <p id="d1e1740">If climate conditions similar to the present persisted over long periods (many
millennia integrated over multiple glacial cycles), then the Køge Bugt
terminus may have stayed near its current position for extended periods as
it has over the past decade. This stability likely would occur when sea
level was within several metres of its present level (e.g. other interglacials),
because its terminus could not retreat past this point and still maintain
contact with the ocean, which would be required in order to evacuate the
large volume of snowfall (retreat from the ocean would cause thickening and
re-advance). As a result of maintaining its terminus at or near this
position for extended periods, erosion may have been focused here to produce
the abrupt transition from a bed above sea level to a deep submarine trough.
Initially the head of the trough may have been located farther seaward than
at present, so that trough formation would have occurred as its head
migrated inland over time. If so, then abrupt transitions at the heads of
many subglacial troughs may be due to a combination of climate and geography
causing termini to maintain stable positions at the heads of their respective
troughs over extended periods. Thus, such points may represent the “last
stands” of these glaciers before a warming climate draws down the ice sheet
sufficiently to pull them completely from their troughs.</p>
</sec>
<sec id="Ch1.S4.SS3">
  <title>Regional outlet glacier changes</title>
      <p id="d1e1749">Figure 6 indicates collective speed-ups of glaciers in north-west (38 %) and
south-east (41 %) Greenland since 2000, but at rates varying with time. In
north-west Greenland, the speed-up was greatest over roughly the last 11 years, whereas in the south-east it was highest from 2001 to 2009.
Because the glaciers that sped up have also likely thinned substantially and
have different widths, these results cannot be directly scaled to estimate
increased discharge. The patterns of speed-up, however, are consistent with
estimates of discharge in 2012 (Enderlin et al., 2014) and suggest that
discharge has increased since then. In particular, speeds in north-west
Greenland have increased by nearly 10 % since 2012. Jakobshavn Isbræ was
not included in Fig. 6, so its recent slowdown could offset some of the
north-west discharge increases.</p>
      <p id="d1e1752">The data from both regions indicate that, for individual glaciers there is
substantial variability, with some glaciers slowing and other glaciers
speeding up in any given year as several earlier results have shown (e.g.
Moon et al., 2012). For example, many of the south-east glaciers that sped up
in 2008 slowed over the period from 2008 to 2010 and then sped up
slightly thereafter. The response of an individual glacier depends on its
internal dynamics (e.g. geometry, terminus position, bed conditions) and it
its recent history. Thus, as noted by many other studies, similar glaciers
subjected to similar forcing may exhibit substantially different responses,
making it difficult to determine the influence of the forcing. With
populations of glaciers such as shown in Fig. 6, however, it should be
easier to determine the average response to climate forcing once the records are
sufficiently long. Past studies have been hindered by the limited duration
of the satellite record, but GIMP and other projects are now producing
records of sufficiently long periods to begin multi-decadal analyses.</p>
</sec>
<sec id="Ch1.S4.SS4">
  <title>South-west Greenland ice sheet trends</title>
      <p id="d1e1762">For much of south-west Greenland, Fig. 7 indicates little in the way of
significant multi-annual trends in speed for the bare-ice and wet-snow zones
over the winters from 2000–2001 to 2016–2017. Where statistically significant
trends occur, they are generally associated with areas of focused outlet
flow at either marine or land-terminating glaciers. An exception is a region
(<inline-formula><mml:math id="M101" display="inline"><mml:mo lspace="0mm">∼</mml:mo></mml:math></inline-formula> centred on SW1 in Fig. 7) that lies within the T2015
region.</p>
      <p id="d1e1772">The results of our Monte Carlo simulation indicate that, given the levels of
noise in our data (Fig. S2), we would have a difficult time reliably
distinguishing a trend of 0.5 m yr<inline-formula><mml:math id="M102" 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> from zero using our data. For 1.0 m yr<inline-formula><mml:math id="M103" 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>,
we would detect most (94 %) trends with our typical errors and
58 % with our nominally worst-case example. We expect most errors to fall
within this range, so if much (<inline-formula><mml:math id="M104" display="inline"><mml:mo lspace="0mm">&gt;</mml:mo></mml:math></inline-formula> 50 %) of our study area had a
trend of 1.0 m yr<inline-formula><mml:math id="M105" 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>, while we did not detect the trend at every point, we
would expect to see a much higher rate of detections than that shown in
Fig. 7. For trends of <inline-formula><mml:math id="M106" display="inline"><mml:mo>≥</mml:mo></mml:math></inline-formula> 1.5 m yr<inline-formula><mml:math id="M107" 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> we should reliably detect most
(<inline-formula><mml:math id="M108" display="inline"><mml:mo lspace="0mm">&gt;</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M109" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 90 %) trends. Thus, our results indicate
that trends of <inline-formula><mml:math id="M110" display="inline"><mml:mo>&gt;</mml:mo></mml:math></inline-formula> 1.5 m yr<inline-formula><mml:math id="M111" 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> are rare in our study area, and
widespread trends of <inline-formula><mml:math id="M112" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 1 m yr<inline-formula><mml:math id="M113" 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> over a broad area are
unlikely, particularly in the areas not covered by the T2015 data.</p>
      <p id="d1e1891">Tedstone et al. (2015) use annual velocities rather than winter velocities, as we
have. Each type of data suffers from sampling problems. Our data do not
uniformly sample the winter period as described above. They do, however,
sample a period when seasonal variation should be minimal. (In this region,
the pre-Sentinel data are all acquired in<?pagebreak page2225?> October–April.) In order to
examine the sensitivity to the inconsistent sampling in our data, we compare
our data at NL with the GPS data (see Fig. 8), which uniformly sampled the
full winter (no-melt) period (Stevens et al., 2016). In the period of
overlap, the SAR observations show good agreement with GPS data, suggesting
that our results are not unduly biased by seasonal variability. To investigate
further, we used these 2006–2007 GPS data to compute partial winter
velocities over several 3-month intervals that roughly match the periods
covered by the pre-Sentinel SAR campaigns. Relative to the 9-month winter
average, the smallest bias was 0.3 m yr<inline-formula><mml:math id="M114" 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> (October–December) and the greatest
bias was 2.6 m yr<inline-formula><mml:math id="M115" 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> (February–April). Overall, these biases are small
relative to the noise and should be randomly distributed with time, which
would reduce their contribution to the trend. If somehow, they were not
randomly distributed, the worst they could skew the trend by is 0.16 m yr<inline-formula><mml:math id="M116" 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> (2.6 m yr<inline-formula><mml:math id="M117" 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>/16 yr). The T2015 data also have issues with sampling
because the image pairs they used span a range of values (352 to 400 days)
that could introduce similar and potentially larger biases (e.g. a period
of longer than a year could sample fast flow in the summer
disproportionately). Thus, some, but likely not all, of the observed
differences between our results and those of T2015 could be due to sampling
issues in one or both of the data sets.</p>
      <p id="d1e1942">If the processes that contribute to the T2015 slowdown occurred entirely in
the summer, then they would not be detected by our winter data, potentially
causing the difference between our winter and the T2015 annual velocities.
If the entire slowdown occurred from June to August, then a summer
slowdown trend of 6 m yr<inline-formula><mml:math id="M118" 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> would be required to produce the
annually averaged slowdown of 1.5 m yr<inline-formula><mml:math id="M119" 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> found in the T2015 data. Over a
period of several years, such a trend would yield summer velocities that
were lower than winter velocities, which has not been observed thus far.
Moreover, when Stevens et al. (2016) examined the NL GPS data, they found
significant winter slowdown (<inline-formula><mml:math id="M120" display="inline"><mml:mo lspace="0mm">-</mml:mo></mml:math></inline-formula>1.13 m yr<inline-formula><mml:math id="M121" 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>) but no significant trend for
the summer. Thus, it is difficult to explain the difference between the
winter and annual velocities as being largely the result of changes in speed
confined to summer or early autumn periods.</p>
      <p id="d1e1989">Since the Tedstone et al. (2015) data set ends in 2014, while ours extend
to the winter of 2016–2017, differences in observation period may explain some of
the differences. Figure 8 indicates that speeds were lower in the winter of
2012–2013 after strong melt in the 2012. Thus, if we only compute trends
through to 2013, the area of significant slowdown surrounding SW1 expands (not
shown) to include the area around NL.</p>
      <p id="d1e1992">It is important to note that at the 95 % confidence level (i.e. exceeds
2<inline-formula><mml:math id="M122" display="inline"><mml:mi mathvariant="italic">σ</mml:mi></mml:math></inline-formula> in the Fig. 1 of T2015), the T2015 data only show significant
differences at elevations below <inline-formula><mml:math id="M123" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 700 m, which represents a
relatively small portion of the area (see magenta contour in Fig. 7).
Factoring in that we do find some trends in this area, statistically the
differences between the two data sets are not all that great, even if the
magnitudes and distribution do differ somewhat.</p>
      <p id="d1e2009">In summary, our data suggest some trends toward slowdown in the T2015
region, though not as strongly as the T2015 results. There is enough
uncertainty in both data sets that at this point it is difficult to
unambiguously resolve the magnitude of any such trends. As more data become
available, the longer time series should produce more certain results. Our
results for the 325 km stretch of ice sheet to the south of the T2015
region, however, indicate no slowdown trends with magnitude <inline-formula><mml:math id="M124" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M125" display="inline"><mml:mo>&gt;</mml:mo></mml:math></inline-formula> 1 m yr<inline-formula><mml:math id="M126" 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 on a few small outlets). This lack of
change raises the possibility that any change in the T2015 region may not be
directly related to melt forcing but instead may be related to the rapid
thinning on Jakobshan Isbræ (e.g. water piracy) or some other local
rather than regional process.</p>
</sec>
</sec>
<sec id="Ch1.S5" sec-type="conclusions">
  <title>Conclusions</title>
      <p id="d1e2045">By analysing results from new and earlier GIMP products, we demonstrate a
17-year growing record of temporally consistent ice-sheet velocity data.
The varying mix of sensors through time introduces some differences in
spatial resolution, which should be considered in any analysis that could be
affected. Early results in the time series were derived from only a few
image pairs, and for some years there are no data. Over time as TerraSAR-X,
TandDEM-X, Landsat 8, Sentinel 1A/B have come online, temporal sampling and
accuracy have improved greatly. Several other SARs are scheduled for launch
in the next decade. In particular, the NASA ISRO (Indian Space Agency) SAR
(NISAR) is scheduled for launch in 2021. It will sample all areas of the
ice sheet at least 66 times per year (33 cycles each from ascending and
descending orbits) with 12-day sampling. Its L-band frequency will improve
correlation for difficult to map areas, such as south-east Greenland.
Collectively the data from the global constellation will allow GIMP and
other products to steadily improve with time. The growing duration of these
records will also allow more robust analyses of the processes controlling
fast flow and how they are affected by climate and other forcings.</p>
</sec>

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

      <p id="d1e2052">The velocity data sets are distributed through the GIMP
project page at NSIDC (<uri>http://nsidc.org/data/measures/gimp</uri>, last access: 4 January 2018);
see also Table 1.</p>
  </notes><app-group>
        <supplementary-material position="anchor"><p id="d1e2058">The supplement related to this article is available online at: <inline-supplementary-material xlink:href="https://doi.org/10.5194/tc-12-2211-2018-supplement" xlink:title="pdf">https://doi.org/10.5194/tc-12-2211-2018-supplement</inline-supplementary-material>.</p></supplementary-material>
        </app-group><notes notes-type="competinginterests">

      <p id="d1e2067">The authors declare that they have no conflict of
interest.</p>
  </notes><ack><title>Acknowledgements</title><p id="d1e2073">The data described in this paper were produced with support from the NASA
MEaSUREs programme (NASA grants NNX08AL98A and NNX13AI21A), with some basic
algorithm development funded under NISAR (NNX16AK53G). The RADARSAT data
were acquired by the Canadian Space Agency (CSA), and the PALSAR data were
acquired by the Japanese Space Agency (JAXA). The German Space Agency (DLR)
acquired, processed and distributed the TerraSAR-X and TanDEM-X data, and we
gratefully acknowledge the help with these data provided by Dana Floricioiu
at DLR. The Sentinel 1A/B data were acquired through the European
Commission's Copernicus programme and were processed by the European Space
Agency. The RADARSAT data through 2010, the ALOS-PALSAR data, and the
Copernicus Sentinel 1A/B data were archived and delivered by the Alaska
Satellite Facility (ASF). The 2012/13 RADARSAT data were archived and
delivered by CSA. All source data
are available from their respective space agency and/or ASF. The Landsat 8
data were provided by through a joint effort by the United States Geological
Survey (USGS) and NASA and distributed via Google. The NL GPS data were
collected as part of a collaboration with Sarah Das, Mark Behn, and Laura Stevens.
Comments by Mai Maki, Andrew Tedstone, Peter Nienow, Amaury Dehecq,
Noel Gourmelen, and
the two anonymous reviewers helped to improve the
manuscript.<?xmltex \hack{\newline}?><?xmltex \hack{\newline}?>Edited by: Marco Tedesco
<?xmltex \hack{\newline}?>
Reviewed by: two anonymous referees</p></ack><ref-list>
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    <!--<article-title-html>Greenland Ice Mapping Project: ice flow velocity variation at sub-monthly to decadal timescales</article-title-html>
<abstract-html><p>We describe several new ice velocity maps produced by the
Greenland Ice Mapping Project (GIMP) using Landsat 8 and Copernicus Sentinel
1A/B data. We then focus on several sites where we analyse these data in
conjunction with earlier data from this project, which extend back to the
year 2000. At Jakobshavn Isbræ and Køge Bugt, we find good agreement when
comparing results from different sensors. In a change from recent behaviour,
Jakobshavn Isbræ began slowing substantially in 2017, with a midsummer
peak that was even slower than some previous winter minima. Over the last
decade, we identify two major slowdown events at Køge Bugt that coincide
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glaciers in north-west and south-west Greenland to produce a record of speed-up
since 2000. Collectively these glaciers continue to speed up, but there are
regional differences in the timing of periods of peak speed-up. In addition,
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the ice sheet and find little in the way of statistically significant changes
over the period covered by our data. Finally, although the consistency of the
data is generally good over time and across sensors, our analysis
indicates that substantial differences can arise in regions with high strain
rates (e.g. shear margins) where sensor resolution can become a factor. For
applications such as constraining model inversions, users should factor in
the impact that the data's resolution has on their results.</p></abstract-html>
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