Components of the 11- and 22-year variation of cosmic rays

Details Components of the 11- and 22-year variation of cosmic rays Components of the 11- and 22-year variation of cosmic rays

Jun 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992p%26ss...40..811p&link_type=abstract

Planetary and Space Science (ISSN 0032-0633), vol. 40, no. 6, June 1992, p. 811-827.

Physics

7

Galactic Cosmic Rays, Solar Activity Effects, Solar Cycles, Geomagnetism, Neutrons, Solar Magnetic Field, Solar Terrestrial Interactions

Scientific paper

Results based on the data from two independent pairs of neutron monitor stations with widely varying geomagnetic cutoffs are presented. Long-term cosmic ray observations by means of neutron monitors permit distinguishing modulation effects related to the 22-year solar magnetic cycle from effects due to the 11-year solar activity cycle. Utilizing the long-term data from the neutron monitor stations it was possible to study the rigidity dependence of solar modulation during the positive and negative phases of the solar magnetic cycle.

Affiliated with

Also associated with

No associations

Rating

Components of the 11- and 22-year variation of cosmic rays 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 Components of the 11- and 22-year variation of cosmic rays, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Components of the 11- and 22-year variation of cosmic rays will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1522894