Dependence of geomagnetic activity during magnetic storms on the solar wind parameters for different types of streams: 2. Main phase of storm |
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Authors: | N S Nikolaeva Yu I Yermolaev I G Lodkina |
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Institution: | 1. Space Research Institute, Russian Academy of Sciences, Moscow, Russia
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Abstract: | The paper analyses the development of the main phase of magnetic storms with Dst ≤ −50 nT, the interplanetary source of which consists of eight types of solar wind streams: magnetic clouds (MC, 17 storms);
corotating interaction regions (CIR, 49 storms); Ejecta (50 storms); compressed region (Sheath) before Ejecta ShE (34 storms); the Sheath before a magnetic cloud ShMC (6 storms); all Sheath before all ICME, ShE + ShMC (40 storms); all ICME, MC + Ejecta (67 storms); and an indeterminate type of stream IND (34 storms). |
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