Dependence of the Postnoon Auroral Intensity upon the IMF Parameters

Abstract Based on auroral observations with a multi‐channel scanning photometer at Zhongshan Station, Antarctica and interplanetary magnetic field (IMF) data obtained by WIND Satellite at the upstream of the bow shock in 1997 and 1998, the dependence of the high‐latitude postnoon auroral intensity u...

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Bibliographic Details
Published in:Chinese Journal of Geophysics
Format: Article in Journal/Newspaper
Language:English
Published: Wiley 2002
Subjects:
Online Access:http://dx.doi.org/10.1002/cjg2.259
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