David Shean

Prof. David Shean

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Research Focus & Metrics

Academic Career Length

22Years (2005-Present)

(Calculated once Scilit publication data is synced: current year − year of first publication + 1)

Representative Publications

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16 July 2021 in Science
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Journal Article
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DSDan Shugar
Dan Shugar
MJM. Jacquemart
M. Jacquemart
DSDavid Shean
David Shean
SBS. Bhushan
S. Bhushan
KUK. Upadhyay
K. Upadhyay
MWMatthew Westoby
Matthew Westoby
A deadly cascade: A catastrophic landslide in Uttarakhand state in India on February 2021 damaged two hydropower plants, and more than 200 people were killed or are missing. Shugar et al. describe the cascade of events that led to this disaster. A massive rock and ice avalanche roared down a Himalayan valley, turning into a deadly debris flow upstream from the first of the two hydropower plants. The sequence of events highlights the increasing risk in the Himalayas caused by increased warming and development. Science , abh4455, this issue p. 300

1 June 2016 in ISPRS Journal of Photogrammetry and Remote Sensing
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Journal Article
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DSDavid Shean
David Shean
OAOleg Alexandrov
Oleg Alexandrov
ZMZachary M. Moratto
Zachary M. Moratto
BSBenjamin E. Smith
Benjamin E. Smith
IJIan Joughin
Ian Joughin
PMPaul Morin
Paul Morin

30 January 2020 in Frontiers in Earth Science
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Journal Article
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DSDavid Shean
David Shean
SBShashank Bhushan
Shashank Bhushan
PMPaul Montesano
Paul Montesano
DRDavid R. Rounce
David R. Rounce
AAAnthony Arendt
Anthony Arendt
BOBatuhan Osmanoglu
Batuhan Osmanoglu
High-mountain Asia (HMA) constitutes the largest glacierized region outside of the Earth's polar regions. Although available observations are limited, long-term records indicate sustained HMA glacier mass loss since ~1850, with accelerated loss in recent decades. Recent satellite data capture the spatial variability of this mass loss, but spatial resolution is coarse and some estimates for regional and HMA-wide mass loss disagree. To address these issues, we generated 5,797 high-resolution digital elevation models (DEMs) from available sub-meter commercial stereo imagery (DigitalGlobe WorldView-1/2/3 and GeoEye-1) acquired over HMA glaciers from 2007 to 2018 (primarily 2013–2017). We also reprocessed 28,278 ASTER DEMs over HMA from 2000 to 2018. We combined these observations to generate robust elevation change trend maps and geodetic mass balance estimates for 99% of HMA glaciers between 2000 and 2018. We estimate total HMA glacier mass change of −19.0 ± 2.5 Gt yr−1 (−0.19 ± 0.03 m w.e. yr−1). We document the spatial pattern of HMA glacier mass change with unprecedented detail, and present aggregated estimates for HMA glacierized sub-regions and hydrologic basins. Our results offer improved estimates for the HMA contribution to global sea level rise in recent decades with total cumulative sea-level rise contribution of ~0.7 mm from exorheic basins between 2000 and 2018. We estimate that the range of excess glacier meltwater runoff due to negative glacier mass balance in each basin constitutes ~12–53% of the total basin-specific glacier meltwater runoff. These results can be used for calibration and validation of glacier mass balance models, satellite gravimetry observations, and hydrologic models needed for present and future water resource management.

25 September 2009 in Science
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SBShane Byrne
Shane Byrne
CDColin M. Dundas
Colin M. Dundas
MKMegan R. Kennedy
Megan R. Kennedy
MMMichael T. Mellon
Michael T. Mellon
AMAlfred S. McEwen
Alfred S. McEwen
FSFrank P. Seelos
Frank P. Seelos
Martian Impact: Impact craters form frequently on Mars, exposing material that would otherwise remain hidden below the surface. Byrne et al. (p. 1674 ) identified mid-latitude craters that formed over the last few years, imaged them in great detail with a camera on board the Mars Reconnaissance Orbiter, and monitored subsequent changes. The craters excavated buried water ice, which was later seen sublimating away. In addition, some craters might have excavated completely through the ice. The observations are consistent with models and other observations that suggest water ice should be stable decimeters to about 1 meter below the martian surface at latitudes poleward of about 40°; and suggest that, in the recent past, Mars had a wetter atmosphere than at present.

28 April 2021 in Geophysical Research Letters
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DRDavid Rounce
David Rounce
RHRegine Hock
Regine Hock
RMR. W. McNabb
R. W. McNabb
RMRomain Millan
Romain Millan
CSC. Sommer
C. Sommer
DSDavid Shean
David Shean
Supraglacial debris affects glacier mass balance as a thin layer enhances surface melting, while a thick layer reduces it. While many glaciers are debris‐covered, global glacier models do not account for debris because its thickness is unknown. We provide the first globally distributed debris thickness estimates using a novel approach combining sub‐debris melt and surface temperature inversion methods. Results are evaluated against observations from 22 glaciers. We find the median global debris thickness is ∼0.15 ± 0.06 m. In all regions, the net effect of accounting for debris is a reduction in sub‐debris melt, on average, by 37%, which can impact regional mass balance by up to 0.40 m water equivalent (w.e.) yr‐1. We also find recent observations of similar thinning rates over debris‐covered and clean ice glacier tongues is primarily due to differences in ice dynamics. Our results demonstrate the importance of accounting for debris in glacier modeling efforts.

5 May 2005 in Journal of Geophysical Research
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DSDavid Shean
David Shean
JHJames W. Head
James W. Head
DMDavid R. Marchant
David R. Marchant