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Detailed Reference Information |
González, S.A., Fejer, B.G., Heelis, R.A. and Hanson, W.B. (1992). Ion composition of the topside equatorial ionosphere during solar minimum. Journal of Geophysical Research 97: doi: 10.1029/91JA03111. issn: 0148-0227. |
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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¿104 cm-3 during the day and 104 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 103 cm-3 during equinox daytime. ¿ American Geophysical Union 1992 |
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Abstract |
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Keywords
Ionosphere, Equatorial ionosphere, Ionosphere, Ion chemistry and composition |
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Publisher
American Geophysical Union 2000 Florida Avenue N.W. Washington, D.C. 20009-1277 USA 1-202-462-6900 1-202-328-0566 service@agu.org |
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