A 360-DEGREE AND 360-ORDER MODEL OF VENUS TOPOGRAPHY

被引：26

作者：

RAPPAPORT, N

PLAUT, JJ

机构：

[1] Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109

来源：

ICARUS | 1994年 / 112卷 / 01期

关键词：

D O I：

10.1006/icar.1994.1167

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

This report presents the most recent spherical harmonic topography model of Venus developed at Jet Propulsion Laboratory. It was produced by a spherical harmonic analysis of the most complete set of Magellan altimetry data, augmented by Pioneer Venus and Venera data. The harmonic coefficients of the topography were computed to degree and order 360. Compared to previous topography models, this one has the highest correlation with the gravity field of Venus. (C) 1994 Academic Press, Inc.

引用

页码：27 / 33

页数：7

共 12 条

[1] THE SPECTRA OF THE TOPOGRAPHY OF THE EARTH, VENUS AND MARS [J].

BALMINO, G .

GEOPHYSICAL RESEARCH LETTERS, 1993, 20 (11) :1063-1066

[2]

BANERDT WB, 1944, ICARUS, V112, P117

[3] VENUS TOPOGRAPHY - A HARMONIC-ANALYSIS [J].

BILLS, BG ;

KOBRICK, M .

JOURNAL OF GEOPHYSICAL RESEARCH-SOLID EARTH AND PLANETS, 1985, 90 (NB1) :827-836

[4]

DAVIES ME, 1922, CELESTIAL MECH, V53, P377

[5]

FORD G, 1986, PIONEER VENUS HYPSOM

[6] VENUS TOPOGRAPHY AND KILOMETER SCALE SLOPES [J].

FORD, PG ;

PETTENGILL, GH .

JOURNAL OF GEOPHYSICAL RESEARCH-PLANETS, 1992, 97 (E8) :13103-13114

[7] VENUS SPHERICAL HARMONIC GRAVITY MODEL TO DEGREE-60 AND ORDER-60 [J].

KONOPLIV, AS ;

SJOGREN, WL .

ICARUS, 1994, 112 (01) :42-54

[8] VENUS GRAVITY AND TOPOGRAPHY - 60TH DEGREE AND ORDER MODEL [J].

KONOPLIV, AS ;

BORDERIES, NJ ;

CHODAS, PW ;

CHRISTENSEN, EJ ;

SJOGREN, WL ;

WILLIAMS, BG ;

BALMINO, G ;

BARRIOT, JP .

GEOPHYSICAL RESEARCH LETTERS, 1993, 20 (21) :2403-2406

[9] ISOSTATIC COMPENSATION OF EQUATORIAL HIGHLANDS ON VENUS [J].

KUCINSKAS, AB ;

TURCOTTE, DL .

ICARUS, 1994, 112 (01) :104-116

[10] VENUS - GLOBAL GRAVITY AND TOPOGRAPHY [J].

MCNAMEE, JB ;

BORDERIES, NJ ;

SJOGREN, WL .

JOURNAL OF GEOPHYSICAL RESEARCH-PLANETS, 1993, 98 (E5) :9113-9128

← 1 2 →