Abstract In the present analysis, the mass spectrometer data from the ISS-b satellite, available in the form of contour plots at an average height of 1100 km for every alternate hour, is used. This analysis showed some interesting results in terms of the diurnal variation of the transition heights; at times dominance of He+ over the other ions, and the seasonal variations of different constituents. In the development of ion composition models, it is suggested that this type of result should be taken into consideration.
Ion composition behaviour in low and mid-latitudes during high solar activity
Advances in Space Research ; 4 , 1 ; 111-117
1984-01-01
7 pages
Aufsatz (Zeitschrift)
Elektronische Ressource
Englisch
Solar wind composition and expectations for high solar latitudes
Elsevier | 1993
|Solar Wind Composition and Expectations for High Solar Latitudes
Online Contents | 1993
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