GSTDTAP  > 气候变化
DOI10.1029/2020GL088556
Radar sounding of subsurface structure in eastern Coprates and Capri Chasmata, Mars
R. Noguchi; K. Ishiyama; A. Kumamoto; C. Uemura; Y. Kasaba; T. Usui; A. Oura; D. Shoji
2020-08-04
发表期刊Geophysical Research Letters
出版年2020
英文摘要

We surveyed the subsurface structure in eastern Coprates and Capri Chasmata in the equatorial region using high‐resolution visible images, digital terrain models, and radar sounding data. We identified subsurface reflectors in four areas of the chasmata. At the stratigraphic exposure on the chasmata walls, the corresponding depth of the reflector is ~60 m. The bulk dielectric constants of the layers above the reflectors are calculated as 3.4‐‐4.0, suggesting a rock‐air mixture with ~39.3 and 46.1 % porosity, or a rock‐air‐ice mixture with < 21.2 % water‐ice fraction. This high porosity corresponds to non‐welded and unconsolidated sediments emplaced by aeolian, fluvial and volcanic activities. If water‐ice actually exists, further studies and discussions are required for the mechanism to maintain it within low‐latitudes.

领域气候变化
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文献类型期刊论文
条目标识符http://119.78.100.173/C666/handle/2XK7JSWQ/287728
专题气候变化
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R. Noguchi,K. Ishiyama,A. Kumamoto,et al. Radar sounding of subsurface structure in eastern Coprates and Capri Chasmata, Mars[J]. Geophysical Research Letters,2020.
APA R. Noguchi.,K. Ishiyama.,A. Kumamoto.,C. Uemura.,Y. Kasaba.,...&D. Shoji.(2020).Radar sounding of subsurface structure in eastern Coprates and Capri Chasmata, Mars.Geophysical Research Letters.
MLA R. Noguchi,et al."Radar sounding of subsurface structure in eastern Coprates and Capri Chasmata, Mars".Geophysical Research Letters (2020).
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