RUSSIAN JOURNAL OF EARTH SCIENCES, VOL. 17, ES2002, doi:10.2205/2017ES000597, 2017
Figure 4. Comparison of the auroral response, as characterized by hourly $AE$ index, with a strength of the SW driver, determined by the IMF $Bz$ component, for the calm ($\log S_{\mathrm{IMF}}<0$, blue dots) and turbulent ($\log S_{\mathrm{IMF}}>0$, red dots) IMF for the period 1994–1995 (from [Romanova and Pilipenko, 2008]).
Citation: Pilipenko V. A., O. V. Kozyreva, M. J. Engebretson, A. A. Soloviev (2017), ULF wave power index for space weather and geophysical applications: A review, Russ. J. Earth Sci., 17, ES2002, doi:10.2205/2017ES000597.
Copyright 2017 by the Geophysical Center RAS.
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