Relationship of cosmic ray diurnal anisotropy and high speed solar wind streams.

Details Relationship of cosmic ray diurnal anisotropy and high speed solar wind streams. Relationship of cosmic ray diurnal anisotropy and high speed solar wind streams.

Oct 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996injpb..70..367s&link_type=abstract

Indian J. Phys., Part B, Vol. 70B, No. 5, p. 367 - 373

Physics

Cosmic Rays: Solar Modulation, Cosmic Rays: Solar Wind

Scientific paper

It is accepted that high speed solar wind streams originated from the Sun can be identified into two categories: the coronal hole associated or corotating streams and flare-generated streams. In this analysis, the authors examine the effects of these two types of solar wind streams on diurnal anisotropy of cosmic ray daily variation for the period of 1980 - 1982. Amplitudes and time of maxima of diurnal vectors have been obtained from harmonic analysis, using the hourly counts of Deep River neutron monitor. It has been found that the solar flare-generated high speed solar wind streams are most effective to produce isotropic and anisotropic changes in cosmic ray intensity. They observe relatively smaller amplitude of the diurnal anisotropy during the period of flare-generated streams.

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