Forbush Decreases in the Cosmic Radiation

Other

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

52

Scientific paper

The experimental observations of Forbush decreases in recent years are reviewed and related to different theoretical models which have been proposed. The observational data from both ground-based and spacecraft experiments were selected to illustrate the important characteristics of Forbush decreases. The form of the rigidity dependence of the cosmic-ray modulation during the decreases and effects of the geomagnetic field upon the magnitude of the decreases are discussed. Recent results to deduce the cosmic-ray flow patterns from the observed anisotropies during the decreases are presented. Other features such as differences in onset times, recovery times, precursory increases are discussed. In considering the theoretical models particular emphasis is placed upon the agreement of the predictions of the model with the experimental observations. A theoretical model is suggested which is not original but represents a synthesis of several models previously proposed. Future important measurements and analyses necessary to an understanding of Forbush decreases are outlined.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Forbush Decreases in the Cosmic Radiation 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 Forbush Decreases in the Cosmic Radiation, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Forbush Decreases in the Cosmic Radiation will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-1729767

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.