THE IMPLICATION FOR THE PRESENCE OF A MAGNETOSPHERE ON URANUS IN THE RELATIONSHIP OF EUV AND RADIO-EMISSION

被引：23

作者：

SHEMANSKY, DE

SMITH, GR

机构：

[1] UNIV ARIZONA,LUNAR & PLANETARY LAB,TUCSON,AZ 85721

[2] NW COMMUNITY COLL,POWELL,WY 82435

来源：

关键词：

D O I：

10.1029/GL013i001p00002

中图分类号：

P [天文学、地球科学];

学科分类号：

07 ;

摘要：

引用

页码：2 / 5

页数：4

共 29 条

[1] BARNES A, 1984, URANUS NEPTUNE, P527
[2] DISSOCIATIVE EXCITATION OF H-2, HD, AND D2 BY ELECTRON-IMPACT
CARNAHAN, BL
ZIPF, EC
[J]. PHYSICAL REVIEW A, 1977, 16 (03): : 991 - 1002
[3] H-3+ - AB-INITIO CALCULATION OF VIBRATION SPECTRUM
CARNEY, GD
PORTER, RN
[J]. JOURNAL OF CHEMICAL PHYSICS, 1976, 65 (09) : 3547 - 3565
[4] CHENG AF, 1984, URANUS NEPTUNE, P541
[5] CHENG AF, 1984, URANUS NEPTUNE, P557
[6] APPLICATION OF CLOSE-COUPLING METHOD TO EXCITATION OF ELECTRONIC STATES AND DISSOCIATION OF H-2 BY ELECTRON-IMPACT
CHUNG, S
LIN, CC
[J]. PHYSICAL REVIEW A, 1978, 17 (06): : 1874 - 1891
[7] CLARKE JT, 1985, B AM ASTRON SOC, V17, P745
[8] DISSOCIATION OF MOLECULAR HYDROGEN BY ELECTRON IMPACT
CORRIGAN, SJ
[J]. JOURNAL OF CHEMICAL PHYSICS, 1965, 43 (12) : 4381 - &
[9] POSSIBLE NIGHTSIDE SOURCE DOMINANCE IN NONTHERMAL RADIO EMISSIONS FROM URANUS
CURTIS, SA
[J]. NATURE, 1985, 318 (6041) : 47 - 48
[10] HILL TW, 1984, URANUS NEPTUNE, P497