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Autor Dohm, James M. |
Documentos disponibles escritos por este autor (22)
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Kim, Kyeong J. ; Dohm, James M. ; Williams, Jean-Pierre ; Ruiz Pérez, Javier ; Yu, Byeong-Hyeok ; Hare, Trent M. ; Hasebe, Nobuyuki ; Yamashita, Naoyuki ; Karouji, Yuzuru ; Kobayashi, Shingo ; Hareyama, Makoto ; Shibamura, Eido ; Kobayashi, Masanori ; Uston, Claude d' ; Gasnault, Olivier ; Forni, Olivier ; Reedy, R.C. | 2011![]()
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The present-day thermal state of the martian interior is a very important issue for understanding the 22 internal evolution of the planet. Here, in order to obtain an improved upper limit for the heat flow at 23 the north polar region, we use th[...]![]()
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King, Kyeong Ja ; Dohm, James M. ; Williams, Jean-Pierre ; Ruiz Pérez, Javier ; Hare, Trent M. ; Hasebe, Nobuyuki ; Karouji, Yuzuru ; Kobayashi, Shingo ; Hareyama, Makoto ; Shibamura, Eido ; Kobayashi, Masanori ; Uston, Claude d' ; Gasnault, Olivier ; Forni, Olivier ; Maurice, Sylvestre | Elsevier | 2012Using Geographic Information Systems (GIS), we performed comparative analysis among stratigraphic information and the Kaguya (SELENE) GRS data of the 2500-km-diameter South Pole-Aitken (SPA) basin and its surroundings. Results indicate chat the [...]![]()
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Variations in martian surface heat flow, similar to those observed in terrestrial continental tectonothermally stable areas, could result in elevation differences of kilometric scale through differential thermal isostasy. This effect is enhanced[...]![]()
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