The Effect Of Fast And Slow Solar Wind On The Venusian Upper Atmosphere.

I. C. Whittaker, M. Grande, G. Guymer, B. Pintér, S. Barabash, A. Federov, C. Mazelle, J. Sauvaud, R. Lundin, C. Russell, Y. Futaana, M. Fränz, T. L. Zhang, H. Andersson, K. Brinkfeldt, A. Grigoriev, M. Holmströ M, M. Yamauchi, K. Asamura, W. BaumjohannH. Lammer, A. J. Coates, D. O. Kataria, D. R. Linder, C. C. Curtis, K. C. Hsieh, B. R. Sandel, H. Gunell, H. E. Koskinen, E. Kallio, P. Riihelä, T. Säles, W. Schmidt, J. Kozyra, N. Krupp, J. Woch, J. Luhmann, S. McKenna-Lawlor, J. J. Thocaven, S. Orsini, R. Cerulli-Irelli, M. Mura, M. Milillo, M. Maggi, E. Roelof, P. Brandt, K. Szego, J. D. Winningham, R. A. Frahm, J. Scherrer, J. Sharber, P. Wurz, P. Bochsler

Allbwn ymchwil: Cyfraniad at gynhadleddCrynodebadolygiad gan gymheiriaid

Crynodeb

Using the ASPERA-4 instrument onboard Venus Express the change in the atmospheric boundary layers are investigated. Using the instrument when it is in the apoapsis period of the polar orbit allows pure Solar Wind measurements to be taken. Composition ratios are determined thus identifying periods of fast and slow solar wind. This is then applied to ion maps of the Venusian atmosphere to determine the response after noise calibration methods. The Species reactions to the differing Solar Wind are also used to investigate the inner boundary movements.
Iaith wreiddiolSaesneg
StatwsCyhoeddwyd - 01 Rhag 2008
DigwyddiadAmerican Geophysical Union Fall Meeting - San Francisco, Unol Daleithiau America
Hyd: 15 Rhag 200819 Rhag 2008
Rhif y gynhadledd: 2008

Cynhadledd

CynhadleddAmerican Geophysical Union Fall Meeting
Teitl crynoAGU
Gwlad/TiriogaethUnol Daleithiau America
DinasSan Francisco
Cyfnod15 Rhag 200819 Rhag 2008

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