POLAR IONOSPHERE OF VENUS NEAR THE TERMINATOR FROM EARLY PIONEER VENUS ORBITER RADIO OCCULTATIONS

被引:47
作者
KLIORE, AJ [1 ]
WOO, R [1 ]
ARMSTRONG, JW [1 ]
PATEL, IR [1 ]
CROFT, TA [1 ]
机构
[1] SRI INT,MENLO PK,CA 94025
关键词
D O I
10.1126/science.203.4382.765
中图分类号
O [数理科学和化学]; P [天文学、地球科学]; Q [生物科学]; N [自然科学总论];
学科分类号
07 ; 0710 ; 09 ;
摘要
Fourteen profiles of electron density in the ionosphere of Venus were obtained by the dual-frequency radio occultation method with the Pioneer Venus orbiter between 5 and 30 December 1978. The solar zenith angles for these measurements were between about 85° and 92°, and the latitudes ranged from about 81° to 88° (ecliptic north). In addition to the expected decrease in peak electron density from about 1.5 × 105 to 0.5 × 105 per cubic centimeter with increasing solar zenith angle, a region of almost constant electron density above about 250 kilometers was observed. The ionopause height varies from about 300 to 700 kilometers and seems to be influenced by diurnal changes in solar wind conditions. The structures of the profiles are consistent with models in which O2+ dominates near the ionization peak and is replaced by O+ at higher altitudes. Copyright © 1979 AAAS.
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页码:765 / 768
页数:4
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