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Solar Wind Interaction with Venus, Mars and Comets

Published online by Cambridge University Press:  25 April 2016

M.K. Wallis

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To model and quantify the comet-like interactions with the atmosphere of Venus the extent and time-variability of the suprathermal exospheric coronas need to be established. An extensive suprathermal O corona hypothesized to arise via dissociative recombination of the dominant ion was confirmed by the Orbiter’s UV spectrometer. Uncertainties remain, firstly because the O-corona’s extension beyond the observed limit of 1500 km altitude depends on the poorly-known partition between dissociation channels, secondly because the ionosphere varies substantially with solar UV inputs, and thirdly because the ionosphere and therefore O-corona decrease strongly from dayside to nightside (Kliore et al., Adv. Space Res. 5(11), 1985).

Type
Research Article
Information
Transactions of the International Astronomical Union , Volume 20 , Issue 1 , 1988 , pp. 683 - 689
Copyright
Copyright © Kluwer 1988 

References

Ajello, J.M.: 1978, Astrophys. J. 222, p 1068;CrossRefGoogle Scholar
Ajello, J.M. et al.: 1987, Astrophys. J. 317, p 317;CrossRefGoogle Scholar
Bertaux, J.L.: 1984, IAU Colloquiue No. 81 eds. Kondo, Y., Bruhweiler, F.C. and Savage, B.D., p 3;Google Scholar
Chassetière, E. et al.: 1986, Astron. Astrophys. 160, p 160;Google Scholar
Chassetière, E., Bertaux, J.L.: 1986, Astron. Astrophys. 174, p 174;Google Scholar
Cummings, A.C. et al.: 1984, Astrophys. J. Lett. 287, p L99;CrossRefGoogle Scholar
Dalaudier, F. et al.: 1984, Astron. Astrophys. 134, p 134;Google Scholar
Fahr, H.J.: 1973, Solar Phys. 30, p 30;CrossRefGoogle Scholar
1983, Solar Wind V, NASA CP-2280, p 541;Google Scholar
Fahr, H.J. 1986a, in: The Sun and the Heliosphere in Three Dimensions, ed. by Marsden, R.G., Reidel Publ. Comp., pp 420–434;Google Scholar
Fahr, H.J. 1986b, Advances in Space Res. 6(2), p 13;CrossRefGoogle Scholar
Fahr, H.J., Ripken, H.W.: 1984, Astron. Astrophys. 139, p 139;Google Scholar
Fahr, H.J. 1985, IAU Colloquiue No. 85, eds. by Giese, R. and Lamy, P., pp 205–233;Google Scholar
Fahr, H.J., et al.: 1985, Astron. Astrophys. 142, p 142;Google Scholar
Fahr, H.J., et al.: 1987, Ann. Geophysicae: Space Phys., 5(4). p 316;Google Scholar
Fahr, H.J., Ruciński, D.: 1987, submitted to Ann. Geophysicae;Google Scholar
Fahr, H.J., Ziemkiewicz-Dabrowska, J.: 1987, submitted to Astron. Astrophys.;Google Scholar
Fish, L.A.: 1986, in: The Sun and the Heliosphere in Three Dimensions, ed. by Marsden, R.G., Reidel Publ. Comp., pp 401–413;CrossRefGoogle Scholar
Gaffey, J.D. et al.: 1987, submitted to J. Geophys. Res.;Google Scholar
Gruntman, M.A.: 1986, Planet. Sp. Sci. 34, p 34;CrossRefGoogle Scholar
Grzedzielski, S., Ratkiewicz, R.: 1975, Acta Astron. 25, p 25;Google Scholar
Holzer, T.E., Leer, E.: 1973, Astrophys. Space Science 24, p 24;CrossRefGoogle Scholar
Holzer, T.E.; 1977, Rev. Geophys. Space Physics 15, p 15;CrossRefGoogle Scholar
Isenberg, P.A.: 1986, J. Geophys. Res. 91, p 91;Google Scholar
Isenberg, P.A.: 1987, J. Geophys. Res. 92, p 92;Google Scholar
Isenberg, P.A. et al.: 1985, J. Geophys. Res. 90, p 90;Google Scholar
Jokipii, J.R.: 1986, J. Geophys. Res. 91, p 91;Google Scholar
Lallement, R. et al.: 1985, J. Geophys. Res. 90, p 90;Google Scholar
Lee, M.A. et al.: 1987, submitted to J. Geophys. Res.;Google Scholar
Möbius, E.: 1986, Advances in Space Res. 6(2), p 26;CrossRefGoogle Scholar
Nass, H.U., Fahr, H.J.: 1986, Advances in Space Res. 6(1), p 365;CrossRefGoogle Scholar
Petelski, E.F. et al.: 1980, Astron. Astrophys. 87, p 87;Google Scholar
Price, C.P., Wu, C.S.: 1987, Geophys. Res. Lett. 14(8), p 856;CrossRefGoogle Scholar
Ripken, H.W., Fahr, H.J.: 1980, Mitteilungen Astron. Gesselschaft 50, p 50;Google Scholar
Ripken, H.W., Fahr, H.J.: 1983, Astron. Astrophys. 122, p 122;Google Scholar
Ruciński, D., Fahr, H.J.: 1987, submitted to Astron. Astrophys.;Google Scholar
Wallis, M.K.: 1984, Astron. Astrophys. 130, p 130;Google Scholar
Weller, C.S., Meier, R.R.: 1981, Astrophys. J. 246, p 246;CrossRefGoogle Scholar
Winske, D.C. et al.: 1985 J. Geophys. Res. 90, p 90;Google Scholar
Winske, D.C., Gary, S.P.: 1986 J. Geophys. Res. 91, p 91;Google Scholar
Witt, N. et al.: 1979, Astron. Astrophys. 73, p 73;Google Scholar
Witt, N.: 1981, Astron. Astrophys. 95, p 95;Google Scholar
Wu, C.S. et al.: 1986, Geophys. Res. Lett. 13, p 865 CrossRefGoogle Scholar