High-Speed Solar wind Streams and Cosmic-Ray Intensity Variations During 1991-1996

Details High-Speed Solar wind Streams and Cosmic-Ray Intensity Variations During 1991-1996 High-Speed Solar wind Streams and Cosmic-Ray Intensity Variations During 1991-1996

May 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003soph..214..195s&link_type=abstract

Solar Physics, v. 214, Issue 1, p. 195-200 (2003).

Physics

16

Scientific paper

High-speed plasma streams identified in the solar wind measurements can be separated into two categories: coronal-hole-associated streams and flare-generated streams. Effects of these plasma streams on cosmic-ray intensity are studied for the period of 1991-1996. It is investigated that both of these high-speed solar wind plasma streams (CS and FGS) are found equally effective in producing the cosmic-ray intensity decrease on short-term basis.

Affiliated with

Also associated with

No associations

Rating

High-Speed Solar wind Streams and Cosmic-Ray Intensity Variations During 1991-1996 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 Variations During 1991-1996, 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 Variations During 1991-1996 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-985090