"Terrain softening" is a distinct style of landform degradation observed on Mars. The morphology and distribution of softened terrain have led to the hypothesis that it is the result of quasiviscous relaxation of topology due to the creep deformation of subsurface ice. In order to test this hypothes
β¦ LIBER β¦
Response timescales for martian ice masses and implications for ice flow on Mars
β Scribed by Koutnik, Michelle R.; Waddington, Edwin D.; Winebrenner, Dale P.; Pathare, Asmin V.
- Book ID
- 121988383
- Publisher
- Elsevier Science
- Year
- 2013
- Tongue
- English
- Weight
- 827 KB
- Volume
- 225
- Category
- Article
- ISSN
- 0019-1035
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## Abstract Over the last 28 years ice core records have been systematically recovered from ten highβelevation ice fields, nine of which are located in the low latitudes. Each core has provided new information about the regional climate and environmental change, and together their records challenge