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Location of the Bow Shock and Ion Composition Boundaries at Venus—initial Determinations from Venus Express ASPERA-4

C. Martinecz,M. Fraenz,J. Woch,N. Krupp,E. Roussos,E. Dubinin,U. Motschmann,S. Barabash,R. Lundin,M. Holmstroem,H. Andersson,M. Yamauchi,A. Grigoriev,Y. Futaana,K. Brinkfeldt,H. Gunell,R. A. Frahm,J. D. Winningham,J. R. Sharber,J. Scherrer,A. J. Coates,D. R. Linder,D. O. Kataria,E. Kallio,T. Sales,W. Schmidt,P. Riihela,H. E. J. Koskinen,J. U. Kozyra,J. Luhmann,C. T. Russell,E. C. Roelof,P. Brandt,C. C. Curtis,K. C. Hsieh, B. R. Sandell,M. Grande,J. -A. Sauvaud,A. Fedorov, Ja. Thocaven,C. Mazelle,S. McKenna-Lawler,S. Orsini,R. Cerulli-Irelli,M. Maggi,A. Mura,A. Milillo,P. Wurz,A. Galli,P. Bochsler,K. Asamura,K. Szego,W. Baumjohann,T. L. Zhang,H. Lammer

Planetary and Space Science（2008）

Cited 82|Views49
Key words
Venus,solar wind interaction,solar wind dynamic pressure,Venus Express,bow shock,ion composition boundary
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