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Modulation of Venus ion densities associated with solar variations

Journal Article · · Geophys. Res. Lett.; (United States)
The dayside ion concentrations in the Venus ionosphere obtained by the Pioneer Venus orbiter ion mass spectrometer exhibit a modulation corresponding to the 27-day solar variation. Comparisons were made of the amplitudes of modulation of CO/sub 2//sup +/, C/sup +/, and O/sub 2//sup +/, with the amplitudes of the 27-day variation in the 10.7 cm solar radio flux and the simultaneously measured EUV fluxes at He II (304 A) and Lyman ..beta.. (1026 A), together with a theoretical analysis of the effects of solar variability on the ionosphere and neutral atmosphere of Venus. This analysis leads us to the conclusion that the observed modulation of dayside ion densities is primarily due to the variability in the ionizing EUV radiations and, to a much lesser extent, the result of the variability with solar activity of the neutral atmosphere via the variability in exospheric temperature. In this connection, we also show, theoretically, why the percentage variation of exospheric temperature on Venus (as observed in the ONMS data) for a given variation in F/sub 10.7/, is only half of the exospheric temperature variation for Earth.
Research Organization:
NASA/Goddard Space Flight Center, Greenbelt, Maryland 20771
OSTI ID:
5425649
Journal Information:
Geophys. Res. Lett.; (United States), Journal Name: Geophys. Res. Lett.; (United States) Vol. 8:7; ISSN GPRLA
Country of Publication:
United States
Language:
English