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pro vyhledávání: '"Yermolaev, Mikhail Yu"'
Based on the data of the solar wind (SW) measurements of the OMNI base for the period 1976-2019, the behavior of SW types as well as plasma and interplanetary magnetic field (IMF) parameters for 21-24 solar cycles (SCs) is studied. It is shown that w
Externí odkaz:
http://arxiv.org/abs/2205.07206
Publikováno v:
AIP Conference Proceedings; 3/25/2010, Vol. 1216 Issue 1, p648-651, 4p, 2 Charts, 5 Graphs