Does the duration of the magnetic storm recovery phase depend on the development rate in its main phase? 2. A new method

In contrast to our previous work (Yermolaev et al., 2015), in which we used the magnetic storm recovery phase duration, the exponential time of the recovery phase of magnetic storms generated by three interplanetary driver types (CIR, Sheath, and ICME) is introduced in the present work. The dependen...

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Veröffentlicht in:	Geomagnetism and Aeronomy 2016-05, Vol.56 (3), p.276-280
Hauptverfasser:	Yermolaev, Yu. I., Lodkina, I. G., Nikolaeva, N. S., Yermolaev, M. Yu
Format:	Artikel
Sprache:	eng
Schlagworte:	Atmospheric sciences Data compression Data processing Data recovery Earth and Environmental Science Earth Sciences Geomagnetism Geophysics/Geodesy Magnetic fields Magnetic storms Recovery Sheaths Storms
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