Articles | Volume 29, issue 3
https://doi.org/10.5194/angeo-29-511-2011
© Author(s) 2011. This work is distributed under
the Creative Commons Attribution 3.0 License.
the Creative Commons Attribution 3.0 License.
https://doi.org/10.5194/angeo-29-511-2011
© Author(s) 2011. This work is distributed under
the Creative Commons Attribution 3.0 License.
the Creative Commons Attribution 3.0 License.
10 Mar 2011
Comparison of accelerated ion populations observed upstream of the bow shocks at Venus and Mars
M. Yamauchi
Swedish Institute of Space Physics, Box 812, 98128 Kiruna, Sweden
Y. Futaana
Swedish Institute of Space Physics, Box 812, 98128 Kiruna, Sweden
A. Fedorov
Centre d'Etude Spatiale des Rayonnements, Université de Toulouse, 31038 Toulouse, France
R. A. Frahm
Southwest Research Institute, San Antonio, TX 78228-0510, USA
J. D. Winningham
Southwest Research Institute, San Antonio, TX 78228-0510, USA
E. Dubinin
Max-Planck-Institut für Sonnensystemforschung, 37191 Katlenburg-Lindau, Germany
R. Lundin
Swedish Institute of Space Physics, Box 812, 98128 Kiruna, Sweden
S. Barabash
Swedish Institute of Space Physics, Box 812, 98128 Kiruna, Sweden
M. Holmström
Swedish Institute of Space Physics, Box 812, 98128 Kiruna, Sweden
C. Mazelle
Centre d'Etude Spatiale des Rayonnements, Université de Toulouse, 31038 Toulouse, France
J.-A. Sauvaud
Centre d'Etude Spatiale des Rayonnements, Université de Toulouse, 31038 Toulouse, France
T. L. Zhang
Space Research Institute, Austrian Academy of Sciences, 8042 Graz, Austria
W. Baumjohann
Space Research Institute, Austrian Academy of Sciences, 8042 Graz, Austria
A. J. Coates
Mullard Space Science Laboratory, University College London, Surrey, RH5 6NT, UK
M. Fraenz
Max-Planck-Institut für Sonnensystemforschung, 37191 Katlenburg-Lindau, Germany
