| タイトル | Geothermal Heating, Convective Flow and Ice Thickness on Mars |
| 著者（英） | Cuzzi, J.; Rosenberg, N. D.; Travis, B. J. |
| 著者所属（英） | NASA Ames Research Center |
| 発行日 | 2001-01-01
2001 |
| 言語 | eng |
| 内容記述 | Our 3D calculations suggest that hydrothermal circulation may occur in the martian regolith and may significantly thin the surface ice layer on Mars at some locations due to the upwelling of warm convecting fluids driven solely by background geothermal heating. Additional information is contained in the original extended abstract. |
| NASA分類 | Lunar and Planetary Science and Exploration |
| 権利 | No Copyright |
