Residual cosmic ray modulation in the periods of solar activity minima

Details Residual cosmic ray modulation in the periods of solar activity minima Residual cosmic ray modulation in the periods of solar activity minima

Aug 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001icrc....9.3737k&link_type=abstract

Proceedings of the 27th International Cosmic Ray Conference. 07-15 August, 2001. Hamburg, Germany. Under the auspices of the Int

Physics

Scientific paper

The residual cosmic ray modulation caused by the subsonic solar wind behind a front of the standing shockwave has been considered. Under the assumption that the wind is turbulent and the energy is uniformly distributed, we have estimated the residual modulation depth. In this case, the Bohm's value for a diffusion coefficient has been taken. It is believed that the residual modulation disappeared in the period of the Maunder minimum, and a value of the corresponding increase of radiocarbon and 10 Be is found. The comparison with observation data shows the satisfactory agreement.

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