High Speed Solar Wind Streams and Cosmic Ray Intensity Variation

Details High Speed Solar Wind Streams and Cosmic Ray Intensity Variation High Speed Solar Wind Streams and Cosmic Ray Intensity Variation

Jul 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003icrc....6.3731s&link_type=abstract

Proceedings of the 28th International Cosmic Ray Conference. July 31-August 7, 2003. Trukuba, Japan. Under the auspices of the I

Physics

6

Scientific paper

Two types of high speed solar wind streams namely flare generated streams (FGS) and corotating streams (CS) are taken to study the short-term changes in cosmic ray intensity. In this work we have selected in two types of streams for the period of 1991 to 1996. It is investigated that both of categories of these solar wind streams are found equally effective in producing cosmic ray intensity decreases. These streams are again group ed in to three classes (smaller, medium and longer) according to their duration of occurrence in days. Further, analysis of this study indicates that the medium solar wind streams are found more effective in producing transient decreases in cosmic ray intensity.

Affiliated with

Also associated with

No associations

Rating

High Speed Solar Wind Streams and Cosmic Ray Intensity Variation 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 High Speed Solar Wind Streams and Cosmic Ray Intensity Variation, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and High Speed Solar Wind Streams and Cosmic Ray Intensity Variation will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1146099