Author:
Dremukhina L. A.,Yermolaev Yu. I.,Lodkina I. G.
Subject
Space and Planetary Science,Geophysics
Reference38 articles.
1. Akasofu, S.-I., The development of magnetic storms without a preceding enhancement of the solar plasma pressure, Planet. Space Sci., 1965, vol. 13, pp. 297–301.
2. Akasofu, S.-I., Solar-wind disturbances and the solar wind–magnetosphere energy coupling function, Sol. Space Sci. Rev., 1983, vol. 34, pp. 173–183.
3. Borovsky, J.E. and Denton, M.H., Differences between CME-driven storms and CIR-driven storms, J. Geophys. Res., 2006, vol. 28, pp. 121–190.
4. Boroyev, R.N., Relationship between substorm activity and the interplanetary medium parameters during the main phase of strong magnetic field, Adv. Space Res., 2019, vol. 63, pp. 300–308.
5. Burlaga, L.F., Sittler, E., Mariani, F., and Schwenn, R., Magnetic loop behind an interplanetary shock: Voyager, Helios, and IMP 8 observations, J. Geophys. Res., 1981, vol. 86, pp. 6673–6684.
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