IMF control of the location of Venusian bow shock: The effect of the magnitude 
of IMF component tangential to the bow shock surface

Chai, L.; Fraenz, M.; Wan, W.; Rong, Z.; Zhang, L.; Wie, Y.; Dubinin, E.; Zhong, J.; Han, X.; Barabash, S.

doi:10.1002/2014JA019878

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IMF control of the location of Venusian bow shock: The effect of the magnitude of IMF component tangential to the bow shock surface

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Fraenz, M.
MPI for Aeronomy, Max Planck Institute for Solar System Research, Max Planck Society;
Department Planets and Comets, Max Planck Institute for Solar System Research, Max Planck Society;

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Dubinin, E.
Department Planets and Comets, Max Planck Institute for Solar System Research, Max Planck Society;
MPI for Aeronomy, Max Planck Institute for Solar System Research, Max Planck Society;

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Chai, L., Fraenz, M., Wan, W., Rong, Z., Zhang, L., Wie, Y., Dubinin, E., Zhong, J., Han, X., & Barabash, S. (2014). IMF control of the location of Venusian bow shock: The effect of the magnitude of IMF component tangential to the bow shock surface. Journal Geophysical Research, 119, 9464-9475. doi:10.1002/2014JA019878.

引用: https://hdl.handle.net/11858/00-001M-0000-0024-BAA3-0

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