| |
| | [No title] |
 | | Samples of a number of natural rock surfaces, collected at the Lunar Crater Volcanic Field, Nevada, and in the Eastern Desert, Egypt [5], were used as analogues to blocks of the martian surface. |
 | | GPR data collected around terrestrial impact craters discriminates in situ bedrock, ejecta, alluvium, and calcic soils, thereby highlighting the potential of the instrument in a variety of planetary settings. |
 | | Muhleman D. O.* Janssen M. Clancy R. Frerking M. Gulkis S. McCleese D. Zurek R. Haberle R. Temperature/Pressure and Water Vapor Sounding with Microwave Spectroscopy Two intense microwave spectral lines exist in the martian atmosphere that allow unique sounding capabilities: water vapor at 183 GHz and the (2-1) rotational line of CO at 230 GHz. |
| www.lpi.usra.edu /meetings/programs/msattiiwa.txt (8518 words) |
|