North-South anisotropy during the quasi-stationary modulation of galactic cosmic rays

Details North-South anisotropy during the quasi-stationary modulation of galactic cosmic rays North-South anisotropy during the quasi-stationary modulation of galactic cosmic rays

Oct 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992ncimc..15..527s&link_type=abstract

Nuovo Cimento C, Serie 1 (ISSN 0390-5551), vol. 15 C, no. 5, p. 527-538.

Physics

3

Anisotropy, Coronal Holes, Galactic Cosmic Rays, Interplanetary Space, Modulation, Solar Wind Velocity, Charged Particles, Nucleonics

Scientific paper

High-speed solar-wind streams coming from coronal holes produce, in the interplanetary space, a quasi-stationary modulation of galactic cosmic rays. The Rome cosmic-ray group has analyzed this modulation taking into account not only the charged-particle isotropic intensity but also the North-South anisotropy (ANS), derived from ground-based measurements. The obtained results for the period October 1964-December 1987 are summarized. Data from the Bartels solar rotation No. 2034 (May 23-June 18, 1982) are used to illustrate the ANS phenomenology.

Affiliated with

Also associated with

No associations

Rating

North-South anisotropy during the quasi-stationary modulation of galactic 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 North-South anisotropy during the quasi-stationary modulation of galactic cosmic rays, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and North-South anisotropy during the quasi-stationary modulation of galactic cosmic rays will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1870785