Short-term variation of cosmic ray diurnal anisotropy and solar activity

Details Short-term variation of cosmic ray diurnal anisotropy and solar activity Short-term variation of cosmic ray diurnal anisotropy and solar activity

Feb 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008cosre..46...94m&link_type=abstract

Cosmic Research, Volume 46, Issue 1, pp.94-96

Physics

1

94.20Wq

Scientific paper

A correlative analysis has been made between cosmic ray intensity and solar activity (sunspot numbers) during high amplitude days for the period 1991-1995. The high amplitude days with the time of maximum in the corotational/azimuthal direction do not indicate any significant correlation with solar activity. The diurnal amplitude significantly remains constant and high (0.5%) during the entire period. Our observations suggest that the direction of the anisotropy of high amplitude anisotropic wave train events contribute significantly to the short-term behavior of the cosmic ray diurnal anisotropy. The correlation coefficient is found to remain positive during solar activity maximum for all the high amplitude anisotropic wave train events.

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