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www.ann-geophys.net/30/927/2012/
doi:10.5194/angeo-30-927-2012
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On the relaxation of magnetospheric convection when Bz turns northward
School of Electrical and Computer Engineering, Cornell University, Ithaca, NY, USA
Abstract. The solar wind inputs considerable energy into the upper atmosphere, particularly when the interplanetary magnetic field (IMF) is southward. According to Poynting's theorem (Kelley, 2009), this energy becomes stored as magnetic fields and then is dissipated by Joule heat and by energizing the plasmasheet plasma. If the IMF turns suddenly northward, very little energy is transferred into the system while Joule dissipation continues. In this process, the polar cap potential (PCP) decreases. Experimentally, it was shown many years ago that the energy stored in the magnetosphere begins to decay with a time constant of two hours. Here we use Poynting's theorem to calculate this time constant and find a result that is consistent with the data.
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Citation: Kelley, M. C.: On the relaxation of magnetospheric convection when Bz turns northward, Ann. Geophys., 30, 927-928, doi:10.5194/angeo-30-927-2012, 2012. Bibtex EndNote Reference Manager XML
