HIGHER-ORDER STATISTICS OF PLANETARY GRAVITIES AND TOPOGRAPHIES

被引:5
|
作者
KAULA, WM
机构
[1] Department of Earth & Space Sciences, University of California, Los Angeles, Los Angeles
关键词
D O I
10.1029/93GL03086
中图分类号
P [天文学、地球科学];
学科分类号
07 ;
摘要
The statistical properties of Earth, Venus, Mars, Moon, and a 3-D mantle convection model are compared. The higher order properties are expressed by third and fourth moments: i.e., as mean products over equilateral triangles (defined as coskewance) and equilateral quadrangles (defined as coexance). For point values, all the fields of real planets have positive skewness, ranging from slightly above zero for Lunar gravity to 2.6sigma3 for Martian gravity (sigma is rms magnitude). Six of the eight excesses are greater than Gaussian (3sigma4), ranging from 2.0sigma4 for Earth topography to 18.6sigma4 for Martian topography. The coskewances and coexances drop off to zero within 20-degrees arc in most cases. The mantle convective model has zero skewness and excess slightly less than Gaussian, probably arising from viscosity variations being only radial.
引用
收藏
页码:2583 / 2586
页数:4
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