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21.
The initial parameters of disturbing fluxes of coronal mass ejections (CMEs) such as loop, front, spike, multiple structure
ejection, and structureless ejection, which cannot be determined from direct observations, are determined using the data on
the interplanetary coronal mass ejections (ICMEs) registered on the Helios and Pioneer Venus Orbiter spacecraft in the vicinity
of Venus. The method of MHD modeling the modified initial parameters of CMEs has been used for this purpose. The ICME parameters
have been analyzed in order to determine the types of the solar sources of the considered plasma flows. 相似文献