Geosynchronous Relativistic Electron Events Associated with High-Speed Solar Wind Streams in 2006

Details Geosynchronous Relativistic Electron Events Associated with High-Speed Solar Wind Streams in 2006 Geosynchronous Relativistic Electron Events Associated with High-Speed Solar Wind Streams in 2006

Dec 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009jass...26..439l&link_type=abstract

Journal of Astronomy and Space Sciences. Vol. 26, no. 4, 439-450

Astronomy and Astrophysics

Astronomy

High-Speed Solar Wind Stream, Relativistic Electron Event

Scientific paper

Recurrent enhancements of relativistic electron events at geosynchronous orbit (GREEs) were observed in 2006. These GREE enhancements were associated with high-speed solar wind streams coming from the same coronal hole. For the first six months of 2006, the occurrence of GREEs has 27 day periodicity and the GREEs were enhanced with various flux levels. Several factors have been studied to be related to GREEs: (1) High speed stream, (2) Pc5 ULF wave activity, (3) Southward IMF Bz, (4) substorm occurrence, (5) Whistler mode chorus wave, and (6) Dynamic pressure. In this paper, we have examined the effectiveness about those parameters in selected periods.

Affiliated with

Also associated with

No associations

Rating

Geosynchronous Relativistic Electron Events Associated with High-Speed Solar Wind Streams in 2006 does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Geosynchronous Relativistic Electron Events Associated with High-Speed Solar Wind Streams in 2006, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Geosynchronous Relativistic Electron Events Associated with High-Speed Solar Wind Streams in 2006 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1694496