4.2 Article

Does the polar cap disappear under an extended strong northward IMF?

期刊

JOURNAL OF ATMOSPHERIC AND SOLAR-TERRESTRIAL PHYSICS
卷 71, 期 17-18, 页码 2006-2012

出版社

PERGAMON-ELSEVIER SCIENCE LTD
DOI: 10.1016/j.jastp.2009.09.005

关键词

Aurora; Double reconnection; Interplanetary magnetic field; Closed field fine

资金

  1. NASA CDAWeb
  2. TIMED GUVI
  3. DMSP SSUSI

向作者/读者索取更多资源

The suggestion that the polar cap can completely disappear under certain northward IMF conditions is still controversial. We know that the size of the polar cap is strongly controlled by the interplanetary magnetic field (IMF). Under a southward IMF, the polar cap is usually large and filled with weak diffuse polar rain electrons. The polar cap shrinks under a northward IMF. Here we use the global aurora[ images and coincident particle measurements on May 15, 2005 to show that the discrete arcs (due to precipitation of both electrons and ions) expanded from the dayside oval to the nightside oval and filled the whole polar ionosphere after a long (8 h) and strong (similar to 5-30 nT) northward IMF B,, The observations suggested that the polar cap disappeared under a closed magnetosphere. (C) 2009 Elsevier Ltd. All rights reserved.

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