Structure of cosmic ray currents

Details Structure of cosmic ray currents Structure of cosmic ray currents

Aug 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001icrc...10.4139a&link_type=abstract

Proceedings of the 27th International Cosmic Ray Conference. 07-15 August, 2001. Hamburg, Germany. Under the auspices of the Int

Physics

Scientific paper

We classify three types of structures of cosmicray currents in the solar wind. They are identified based on the data of the world neutron monitor network and with the use of the global survey method. A few simple models are suggested to describe the observed structures and in particular to explain the moments at which the current changes its direction. These moments are associated with the crossing discontinuities in the solar wind. Some peculiarities when the cosmic ray current is changing before the Earth enters the perturbed regions associated with the Forbush-decreases, magnetic storms, the boundaries of wide magnetic sectors are discussed.

Affiliated with

Also associated with

No associations

Rating

Structure of cosmic ray currents 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 Structure of cosmic ray currents, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Structure of cosmic ray currents will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-801407