TY - JOUR
T1 - Surface formation, preservation, and history of low-porosity crusts at the WAIS Divide site, West Antarctica
AU - Fegyveresi, John M.
AU - Alley, Richard B.
AU - Muto, Atsuhiro
AU - Orsi, Anaïs J.
AU - Spencer, Matthew K.
N1 - Funding Information:
Acknowledgements. We acknowledge the following funding sources for support of this work: US National Science Foundation Division of Polar Programs grants 0539578, 1043528, 1142085, and 1619793. We also acknowledge Donald E. Voigt, Joan J. Fitzpatrick, Eric D. Cravens, and the staff of the US National Ice Core Laboratory in Denver, Colorado, as well as the WAIS Divide Science Coordination Office at the University of New Hampshire and the Ice Drilling Design and Operations group at the University of Wisconsin. We thank numerous colleagues involved with the WAIS Divide project, especially Kendrick Taylor, Mark Twickler, and Joseph Souney. We thank Bess Koffman, Gifford Wong, Dominic Winski, Aron Buffen, and Logan Mitchell for assistance with snow pit preparation. We thank Jonathan Thom and the University of Wisconsin-Madison Automatic Weather Station Program for assistance with weather station sensor installation. Lastly, we thank our reviewers, whose thoughtful suggestions and questions served to clarify and improve the manuscript. Any use of trade, firm, or product names is for descriptive purposes only and does not imply endorsement.
Publisher Copyright:
© Author(s) 2018.
PY - 2018/1/26
Y1 - 2018/1/26
N2 - Observations at the West Antarctic Ice Sheet (WAIS) Divide site show that near-surface snow is strongly altered by weather-related processes such as strong winds and temperature fluctuations, producing features that are recognizable in the deep ice core. Prominent "glazed" surface crusts develop frequently at the site during summer seasons. Surface, snow pit, and ice core observations made in this study during summer field seasons from 2008-2009 to 2012-2013, supplemented by automated weather station (AWS) data with short-and longwave radiation sensors, revealed that such crusts formed during relatively low-wind, lowhumidity, clear-sky periods with intense daytime sunshine. After formation, such glazed surfaces typically developed cracks in a polygonal pattern likely from thermal contraction at night. Cracking was commonest when several clear days occurred in succession and was generally followed by surface hoar growth; vapor escaping through the cracks during sunny days may have contributed to the high humidity that favored nighttime formation of surface hoar. Temperature and radiation observations show that daytime solar heating often warmed the near-surface snow above the air temperature, contributing to upward mass transfer, favoring crust formation from below, and then surface hoar formation. A simple surface energy calculation supports this observation Subsequent examination of the WDC06A deep ice core revealed that crusts are preserved through the bubbly ice, and some occur in snow accumulated during winters, although not as commonly as in summertime deposits. Although no one has been on site to observe crust formation during winter, it may be favored by greater wintertime wind packing from stronger peak winds, high temperatures and steep temperature gradients from rapid midwinter warmings reaching as high as -15°C, and perhaps longer intervals of surface stability. Time variations in crust occurrence in the core may provide paleoclimatic information, although additional studies are required. Discontinuity and cracking of crusts likely explain why crusts do not produce significant anomalies in other paleoclimatic records.
AB - Observations at the West Antarctic Ice Sheet (WAIS) Divide site show that near-surface snow is strongly altered by weather-related processes such as strong winds and temperature fluctuations, producing features that are recognizable in the deep ice core. Prominent "glazed" surface crusts develop frequently at the site during summer seasons. Surface, snow pit, and ice core observations made in this study during summer field seasons from 2008-2009 to 2012-2013, supplemented by automated weather station (AWS) data with short-and longwave radiation sensors, revealed that such crusts formed during relatively low-wind, lowhumidity, clear-sky periods with intense daytime sunshine. After formation, such glazed surfaces typically developed cracks in a polygonal pattern likely from thermal contraction at night. Cracking was commonest when several clear days occurred in succession and was generally followed by surface hoar growth; vapor escaping through the cracks during sunny days may have contributed to the high humidity that favored nighttime formation of surface hoar. Temperature and radiation observations show that daytime solar heating often warmed the near-surface snow above the air temperature, contributing to upward mass transfer, favoring crust formation from below, and then surface hoar formation. A simple surface energy calculation supports this observation Subsequent examination of the WDC06A deep ice core revealed that crusts are preserved through the bubbly ice, and some occur in snow accumulated during winters, although not as commonly as in summertime deposits. Although no one has been on site to observe crust formation during winter, it may be favored by greater wintertime wind packing from stronger peak winds, high temperatures and steep temperature gradients from rapid midwinter warmings reaching as high as -15°C, and perhaps longer intervals of surface stability. Time variations in crust occurrence in the core may provide paleoclimatic information, although additional studies are required. Discontinuity and cracking of crusts likely explain why crusts do not produce significant anomalies in other paleoclimatic records.
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U2 - 10.5194/tc-12-325-2018
DO - 10.5194/tc-12-325-2018
M3 - Article
AN - SCOPUS:85041171204
SN - 1994-0416
VL - 12
SP - 325
EP - 341
JO - Cryosphere
JF - Cryosphere
IS - 1
ER -