IMF BY dependence of the extent of substorm westward electrojet
Author:
Publisher
Springer Science and Business Media LLC
Subject
General Earth and Planetary Sciences
Link
http://link.springer.com/content/pdf/10.1007/BF02702019.pdf
Reference35 articles.
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3. Akasofu S-I 1981 Energy coupling between the solar wind and the magnetosphere;Space Sci. Rev. 28 121–190.
4. Burch J L, Reiff P H, Menietti J D, Heelis R A, Hanson W B, Shawhan S D, Shelley E G, Sugiura M, Weimer D R and Winningham J D 1985 IMF BY-dependent plasma flow and Birkeland currents in the Dayside Magnetosphere: 1. Dynamics Explorer observations;J. Geophys. Res. 90 1577–1593.
5. Cowley S W H 1981 Magnetospheric asymmetries associated with the Y-component of the IMF;Planet. Space Sci. 29 79–96.
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2. Dayside cosmic noise absorption at the equatorward boundary of auroral oval as observed from Maitri, Antarctica ( L = 5; CGM 62.45°S, 55.45°E);Journal of Geophysical Research: Space Physics;2016-04
3. Substorm related CNA near equatorward boundary of the auroral oval in relation to interplanetary conditions;Advances in Space Research;2015-07
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