Wavelet image of a heliospheric storm in cosmic rays |
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| Authors: | V I Kozlov V V Markov |
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| Institution: | (1) Institute of Cosmophysical Research and Aeronomy, Siberian Division, Russian Academy of Sciences, pr. Lenina 31, Yakutsk, 677007, Russia |
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| Abstract: | During the sign reversal of the global solar magnetic field, the variations in the ratio of the quadrupole component of the field to its dipole part manifest themselves in a change of the two-sector structure of the heliospheric current sheet (HCS) into the four-sector and, then, multisector structures. At that time, a soliton-like wave packet (soliton of the envelope), precisely which is responsible for a wavelet image of heliospheric storm in cosmic rays, is formed in HCS. |
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