Simulating 0.4-2.5 GHz Brightness Temperatures of the Ross Ice Shelf, Antarctica

被引:3
作者
Brogioni, M. [1 ]
Jezek, K. C. [2 ]
Johnson, J. T. [3 ]
Leduc-Leballeur, M. [1 ]
Yardim, C. [3 ]
Tsang, L. [4 ]
Wang, S. [5 ]
Macelloni, G. [1 ]
机构
[1] CNR, Inst Appl Phys N Carrara, I-50019 Sesto Fiorentino, Italy
[2] Ohio State Univ, Climate Res Ctr, Columbus, OH 43210 USA
[3] Ohio State Univ, ElectroSci Lab, Columbus, OH 43210 USA
[4] Univ Michigan, Dept Elect Engn & Comp Sci, Radiat Lab, Ann Arbor, MI 48109 USA
[5] Penn State Univ, Environm Syst Inst, Dept Geog & Earth, University Pk, PA 16802 USA
关键词
Ice shelf; Ice; Ocean temperature; Microwave radiometry; Temperature measurement; Sea measurements; Microwave integrated circuits; Antarctica; ice shelf; low frequency; microwave radiometry; modeling; SEA-ICE; FIRN; SHEET;
D O I
10.1109/LGRS.2024.3368613
中图分类号
P3 [地球物理学]; P59 [地球化学];
学科分类号
0708 ; 070902 ;
摘要
Ice shelves are important parts of the cryosphere that influence ice sheet dynamics and mass loss. The internal temperatures of ice shelves are currently known only from a few borehole sites or from glaciological models. Microwave radiometry in the 0.4-2.5 GHz range is capable of receiving thermal emissions from deep within an ice shelf and thereby providing information on internal temperatures. This letter reports modeling studies of the brightness temperature of the Ross Ice Shelf (RIS) from 0.4 to 2.5 GHz that provide insight into the potential of microwave radiometers for measuring ice shelf internal properties.
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页数:5
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