ION COMPOSITION OF THE TOPSIDE EQUATORIAL IONOSPHERE DURING SOLAR MINIMUM

被引:41
作者
GONZALEZ, SA
FEJER, BG
HEELIS, RA
HANSON, WB
机构
[1] UTAH STATE UNIV, CTR ATMOSPHER & SPACE SCI, LOGAN, UT 84322 USA
[2] UNIV TEXAS, CTR SPACE SCI, PHYS PROGRAMS, RICHARDSON, TX 75083 USA
关键词
D O I
10.1029/91JA03111
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We have used observations from both the Bennett ion mass spectrometer and the retarding potential analyzer on board the Atmosphere Explorer E satellite to study the longitudinally averaged O+, H+, and He+ concentrations from 150 to 1100 km in the equatorial ionosphere during the 1975-1976 solar minimum. Our results suggest that the ion mass spectrometer measurements need to be increased by a factor of 2.15 to agree with the densities from the retarding potential analyzer and with ground-based measurements. The peak H+ concentrations are about 2.5 x 10(4) cm-3 during the day and 10(4) cm-3 at night and vary little with season. The O+/H+ transition altitude lies between 750 and 825 km during the day and between 550 and 600 km at night. He+ is a minor species at all altitudes; its concentration is highly variable with a maximum value of about 10(3) cm-3 during equinox daytime.
引用
收藏
页码:4299 / 4303
页数:5
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