Abstract
Estimates of snow and firn density are required for satellite-altimetry-based retrievals of ice sheet mass balance that rely on volume-to-mass conversions. Therefore, biases and errors in presently used density models confound assessments of ice sheet mass balance and by extension ice sheet contribution to sea level rise. Despite this importance, most contemporary firn densification models rely on simplified semi-empirical methods, which are partially reflected by significant modeled density errors when compared to observations. In this study, we present a new driftingsnow compaction scheme that we have implemented into SNOWPACK, a physics-based land surface snow model. We show that our new scheme improves existing versions of SNOWPACK by increasing simulated near-surface (defined as the top 10 m) density to be more in line with observations (near-surface bias reduction from 44.9 to 5.4 kgm 3). Furthermore, we demonstrate high-quality simulation of near-surface Antarctic snow and firn density at 122 observed density profiles across the Antarctic ice sheet, as indicated by reduced model biases throughout most of the near-surface firn column when compared to two semi-empirical firn densification models (SNOWPACK mean bias D 9:7 kgm 3, IMAU-FDM mean bias D 32:5 kgm 3, GSFC-FDM mean bias D 15:5 kgm 3). Notably, our analysis is restricted to the near surface where firn density is most variable due to accumulation and compaction variability driven by synoptic weather and seasonal climate variability. Additionally, the GSFC-FDM exhibits lower mean density bias from 7-10m (SNOWPACK bias D 22:5 kgm 3, GSFC-FDM bias D 10:6 kgm 3) and throughout the entire near surface at high-accumulation sites (SNOWPACK bias D 31:4 kgm 3, GSFC-FDM bias D 4:7 kgm 3). However, we found that the performance of SNOWPACK did not degrade when applied to sites that were not included in the calibration of semi-empirical models. This suggests that SNOWPACK may possibly better represent firn properties in locations without extensive observations and under future climate scenarios, when firn properties are expected to diverge from their present state.
Original language | English |
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Pages (from-to) | 1065-1085 |
Number of pages | 21 |
Journal | Cryosphere |
Volume | 15 |
Issue number | 2 |
DOIs | |
Publication status | Published - 1 Mar 2021 |
Bibliographical note
Funding Information:Acknowledgements. Eric Keenan, Nander Wever, Jan T. M. Lenaerts, and Brooke Medley acknowledge support from the National Aeronautics and Space Administration (NASA), grant 80NSSC18K0201 (ROSES-2016: studies with ICESat-2 and CryoSat-2). Eric Keenan, Nander Wever, and Jan T. M. Lenaerts are also supported by BELSPO Research Contract, grant BR/165/A2:Mass2Ant. Peter Kuipers Munneke is funded by the Netherlands Earth System Science Centre (NESSC). Carleen Reijmer acknowledges the support of the Dutch Polar program of the Dutch Research Council NPP-NWO. This work utilized the RMACC Summit supercomputer, which is supported by the National Science Foundation (awards ACI-1532235 and ACI-1532236), the University of Colorado Boulder, and Colorado State University. The Summit supercomputer is a joint effort of the University of Colorado Boulder and Colorado State University. Data storage is supported by the University of Colorado Boulder “PetaLibrary”. Thank you to Xavier Fettweis, Charles Amory, and the anonymous reviewer for providing helpful and insightful comments which helped to improve the paper considerably. The authors thank Lynn Montgomery for their useful insight into the SUMup dataset and constructive comments on this paper.
Funding Information:
Financial support. This research has been supported by
Publisher Copyright:
© 2021 Copernicus GmbH. All rights reserved.
Copyright:
Copyright 2021 Elsevier B.V., All rights reserved.
Funding
Acknowledgements. Eric Keenan, Nander Wever, Jan T. M. Lenaerts, and Brooke Medley acknowledge support from the National Aeronautics and Space Administration (NASA), grant 80NSSC18K0201 (ROSES-2016: studies with ICESat-2 and CryoSat-2). Eric Keenan, Nander Wever, and Jan T. M. Lenaerts are also supported by BELSPO Research Contract, grant BR/165/A2:Mass2Ant. Peter Kuipers Munneke is funded by the Netherlands Earth System Science Centre (NESSC). Carleen Reijmer acknowledges the support of the Dutch Polar program of the Dutch Research Council NPP-NWO. This work utilized the RMACC Summit supercomputer, which is supported by the National Science Foundation (awards ACI-1532235 and ACI-1532236), the University of Colorado Boulder, and Colorado State University. The Summit supercomputer is a joint effort of the University of Colorado Boulder and Colorado State University. Data storage is supported by the University of Colorado Boulder “PetaLibrary”. Thank you to Xavier Fettweis, Charles Amory, and the anonymous reviewer for providing helpful and insightful comments which helped to improve the paper considerably. The authors thank Lynn Montgomery for their useful insight into the SUMup dataset and constructive comments on this paper. Financial support. This research has been supported by