PERTURBATIONS OF SATELLITE ORBITS BY TESSERAL HARMONICS IN THE EARTHS GRAVITATIONAL POTENTIAL

被引：13

作者：

COOK, GE

机构：

来源：

关键词：

D O I：

10.1016/0032-0633(63)90192-2

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：797 / 815

页数：19

共 15 条

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[J]. GEOPHYSICAL JOURNAL OF THE ROYAL ASTRONOMICAL SOCIETY, 1961, 4 : 53 - 72
[3] Erdelyi A., 1953, HIGHER TRANSCENDENTA, VI
[4] MOTION OF A SATELLITE IN THE EARTHS GRAVITATIONAL FIELD
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[J]. PROCEEDINGS OF THE ROYAL SOCIETY OF LONDON SERIES A-MATHEMATICAL AND PHYSICAL SCIENCES, 1960, 254 (1276): : 48 - 65
[5] A DETERMINATION OF THE ELLIPTICITY OF THE EARTHS EQUATOR FROM THE MOTION OF 2 SATELLITES
IZSAK, IG
[J]. ASTRONOMICAL JOURNAL, 1961, 66 (05) : 226 - 229
[6] JEFFREYS H, 1959, EARTH, P140
[7] KAULA WM, 1961, NASA TN D572
[8] KOZAI Y, 1961, 72 SMITHS ASTR OBS S
[9] USE OF ARTIFICIAL SATELLITES TO EXPLORE THE EARTHS GRAVITATIONAL FIELD - RESULTS FROM SPUTNIK-2 (1957-BETA)
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KINGHELE, DG
[J]. NATURE, 1958, 182 (4636) : 640 - 641
[10] THE MOTION OF A SATELLITE IN AN AXI-SYMMETRIC GRAVITATIONAL FIELD
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[J]. GEOPHYSICAL JOURNAL OF THE ROYAL ASTRONOMICAL SOCIETY, 1961, 4 : 17 - 52