Corotating Variations of Cosmic Rays Near the South Heliospheric Pole

Details Corotating Variations of Cosmic Rays Near the South Heliospheric Pole Corotating Variations of Cosmic Rays Near the South Heliospheric Pole

May 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995sci...268.1024k&link_type=abstract

Science, Volume 268, Issue 5213, pp. 1024-1025

Physics

54

Scientific paper

Three-dimensional simulations of the heliospheric modulation of galactic cosmic ray protons show that corotating variations in the intensity can persist to quite high heliographic latitudes. Variations are seen at latitudes considerably higher than the maximum latitude extension of the heliographic current sheet, in regions where the solar wind velocity and magnetic field show no significant variation. Similar conclusions may apply also to lower energy particles, which may be accelerated at lower latitudes. Cosmic ray variations caused by corotating interaction regions present at low heliographic latitudes can propagate to significantly higher latitudes.

Affiliated with

Also associated with

No associations

Rating

Corotating Variations of Cosmic Rays Near the South Heliospheric Pole 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 Corotating Variations of Cosmic Rays Near the South Heliospheric Pole, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Corotating Variations of Cosmic Rays Near the South Heliospheric Pole will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1549582