Computer Science
Scientific paper
Jun 1999
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999aipc..471..621d&link_type=abstract
The solar wind nine conference. AIP Conference Proceedings, Volume 471, pp. 621-624 (1999).
Computer Science
Solar Wind Plasma, Sources Of Solar Wind
Scientific paper
On the basis of cosmic ray (CR) neutron monitor data of the station Climax (University of Chicago, P.I. Prof. J. A. Simpson), as well as of solar activity (SA) data for 1953-1997 (about 4 solar cycles), the CR/SA hysteresis phenomenon is investigated. We consider the time lag between the processes in the interplanetary space responsible for CR modulation and the corresponding processes on the Sun. By these results we estimate the average dimension of the Heliosphere and CR modulation parameters, over about 4 solar cycles. The results obtained for the last 4 cycles are used for determining the long-term CR variations during 1750-1970 on the basis of solar activity data (the last 18 years are used to compare the observed and expected CR intensities).
Dorman Irina V.
Dorman Lev I.
Iucci N.
Parisi Mario
Villoresi G.
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