Snow Densification and Recent Accumulation Along the iSTAR Traverse, Pine Island Glacier, Antarctica

E. M. Morris*, R. Mulvaney, R. J. Arthern, D. Davies, R. J. Gurney, P. Lambert, J. De Rydt, A. M. Smith, R. J. Tuckwell, M. Winstrup

*Corresponding author for this work

Research output: Contribution to journalArticlepeer-review

6 Citations (Scopus)
10 Downloads (Pure)

Abstract

Neutron probe measurements of snow density from 22 sites in the Pine Island Glacier basin have been used to determine mean annual accumulation using an automatic annual layer identification routine. A mean density profile which can be used to convert radar two-way travel times to depth has been derived, and the effect of annual fluctuations in density on estimates of the depth of radar reflectors is shown to be insignificant, except very near the surface. Vertical densification rates have been derived from the neutron probe density profiles and from deeper firn core density profiles available at 9 of the sites. These rates are consistent with the rates predicted by the Herron and Langway model for stage 1 densification (by grain-boundary sliding, grain growth and intracrystalline deformation) and stage 2 densification (predominantly by sintering), except in a transition zone extending from ≈8 to ≈13 m from the surface in which 10–14% of the compaction occurs. Profiles of volumetric strain rate at each site show that in this transition zone the rates are consistent with the Arthern densification model. Comparison of the vertical densification rates and volumetric strain rates indicates that the expected relation to mean annual accumulation breaks down at high accumulation rates even when corrections are made for horizontal ice velocity divergence.

Original languageEnglish
Pages (from-to)2284-2301
Number of pages18
JournalJournal of Geophysical Research: Earth Surface
Volume122
Issue number12
Early online date4 Dec 2017
DOIs
Publication statusPublished - Dec 2017

Fingerprint Dive into the research topics of 'Snow Densification and Recent Accumulation Along the iSTAR Traverse, Pine Island Glacier, Antarctica'. Together they form a unique fingerprint.

Cite this