Global magnetic field of the Sun and long-term variations of galactic cosmic rays

The paper deals with the relation of long-term variations of 10 GV galactic cosmic rays (GCR) to the global solar magnetic field and solar wind parame ters. This study continues previous works, where the tilt of the heliospher ic current sheet (HCS) and other solar-heliospheric parameters are successf ully used to describe long-term variations of cosmic rays in the past two s olar cycles. The novelty of the present work is the use of the HCS tilt and other parameters reconstructed from Ha observations of filaments for the p eriod when direct global solar magnetic field observations were unavailable . Thus, we could extend the GCR simulation interval back to 1953. The analy sis of data for 1953-1999 revealed a good correlation (the correlation coef ficient > 0.88) between the solar-heliospheric parameters and GCR in differ ent cycles of solar activity. Moreover, the approach applied makes it possi ble to describe the behavior of cosmic rays in the epochs of solar maxima, which could not be done before. This indicates both the adequacy of the mod el and the reliability of the reconstructed global solar magnetic field par ameters. (C) 2001 Elsevier Science Ltd. All rights reserved.