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How the IMF B-y induces a B-y component in the closed magnetosphere and how it leads to asymmetric currents and convection patterns in the two hemispheres

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Haaland,  S.
Department Planets and Comets, Max Planck Institute for Solar System Research, Max Planck Society;

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Tenfjord, P., Ostgaard, N., Snekvik, K., Laundal, K. M., Reistad, J. P., Haaland, S., & Milan, S. E. (2015). How the IMF B-y induces a B-y component in the closed magnetosphere and how it leads to asymmetric currents and convection patterns in the two hemispheres. Journal Geophysical Research, 120(11), 9368-9384. doi:10.1002/2015JA021579.


引用: https://hdl.handle.net/11858/00-001M-0000-002A-2EDF-E
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