DISTRIBUTION OF SLOPES ON A CRATERED PLANETARY SURFACE.
Abstract
The distribution of slopes over any finite span on a surface excavated by primary impact craters is derived from a representation of the surface as a 'moving average' of impact events. The cumulants are always positive, and are large for typical mare crater densities. In some cases the distribution can be approximated by a rapidly convergent Gram-Charlier Type A series. The slope distribution has much heavier tails, than a Gaussian distribution with the same variance. Under some conditions, the slopes have approximately a symmetric stable distribution law with characteristic exponent one smaller than the crater diameter population index. Observations of slopes in Mare Cognitum are in good agreement with theory. (Author)
Document Details
- Document Type
- Technical Report
- Publication Date
- Jan 01, 1969
- Accession Number
- AD0695448
Entities
People
- Allan H. Marcus
Organizations
- Johns Hopkins University