Venusian bow shock as seen by the ASPERA-4 ion instrument on Venus Express

I. Whittaker, G. Guymer, M. Grande, B. Pintér, S. Barabash, A. Federov, C. Mazelle, J. A. Sauvaud, R. Lundin, C. T. Russell, Y. Futaana, M. Fränz, T. L. Zhang, H. Andersson, A. Grigoriev, M. Holmström, M. Yamauchi, K. Asamura, W. Baumjohann, H. Lammer, A. J. Coates, D. O. Kataria, D. R. Linder, C. C. Curtis, K. C. Hsieh, H. E. J. Koskinen, E. Kallio, P. Riihelä, W. Schmidt, J. Kozyra, S. McKenna-Lawlor, J. J. Thocaven, S. Orsini, R. Cerulli-Irelli, A. Mura, M. Milillo, M. Maggi, E. Roelof, P. Brandt, R. A. Frahm, J. R. Sharber, P. Wurz, P. Bochsler
  • Journal of Geophysical Research Atmospheres, September 2010, Wiley
  • DOI: 10.1029/2009ja014826

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The following have contributed to this page: Prof. Dr. Wolfgang Baumjohann