Cosmic ray perturbations produced by fast streams coming from quiet solar regions - Coronal holes

Details Cosmic ray perturbations produced by fast streams coming from quiet solar regions - Coronal holes Cosmic ray perturbations produced by fast streams coming from quiet solar regions - Coronal holes

Jun 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977cosp.meets....i&link_type=abstract

COSPAR, Plenary Meeting, 20th, Tel Aviv, Israel, June 7-18, 1977, Paper. 12 p.

Astronomy and Astrophysics

Astronomy

Radiation Distribution, Solar Corona, Solar Cosmic Rays, Solar Flux Density, Solar Wind, Forbush Decreases, Interplanetary Magnetic Fields, Neutron Flux Density, Plasma Density, Polarity, Solar Magnetic Field, Solar Wind Velocity, Spaceborne Astronomy

Scientific paper

The satellite data on solar wind (density, bulk velocity and magnetic field) together with the solar activity data have been used to identify high-velocity, low-density streams emitted by quiet solar regions (coronal holes) in cycle n. 20. For the identified events, a small cosmic ray depression is generally observed, its time behavior traces that of the solar wind speed (about 0.5 percent of intensity depression at high-latitude neutron stations for an increase of 100 km/sec in the solar wind velocity).

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