Publication Date:
2006-04-06
Description:
The origin of Mars surface units and the extent of subsequent cratering play key roles in determining surface texture. At scale sizes of 0.1-10 meters, however, there is a growing body of evidence that wind is the dominant force. The direct and indirect evidence which implies that meter-scale surface texture on Mars is controlled by the wind is presented. Since radar is uniquely sensitive to structure on these scales, radio wave scattering data can provide insight on aeolian activity available from no other source.
Keywords:
LUNAR AND PLANETARY EXPLORATION
Type:
NASA. Washington Rept. of Planetary Geology Program, 1983; p 273-275
Format:
text