Model of the solar cosmic ray burst on March 19, 1990

Details Model of the solar cosmic ray burst on March 19, 1990 Model of the solar cosmic ray burst on March 19, 1990

Apr 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007cosre..45...97e&link_type=abstract

Cosmic Research, Volume 45, Issue 2, pp.97-101

Physics

96.60.Qe

Scientific paper

The causes of oscillation of the solar cosmic ray flux and alternating-sign anisotropy with a period of three hours to two minutes in March 1990 measured on the Granat satellite are analyzed in this paper. It is shown that they are caused by the motion of solar cosmic ray protons with the energy 1 100 MeV in loop structures of solar magnetic fields of the chromosphere and the corona transferred into the interplanetary medium by plasma of the solar wind. A model description of the observation data is presented.

Affiliated with

Also associated with

No associations

Rating

Model of the solar cosmic ray burst on March 19, 1990 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 Model of the solar cosmic ray burst on March 19, 1990, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Model of the solar cosmic ray burst on March 19, 1990 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1078573