Differences in the Dynamics of the Asymmetrical Part of the Magnetic Disturbance during the Periods of Magnetic Storms Induced by Different Interplanetary Sources

Author:

Dremukhina L. A.,Yermolaev Yu. I.,Lodkina I. G.

Publisher

Pleiades Publishing Ltd

Subject

Space and Planetary Science,Geophysics

Reference41 articles.

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2. Barkhatov, N.A., Levitin, A.E., and Tserkovnyuk, O.M., Relation of the indices characterizing the symmetric (SYM) and asymmetric (ASY) ring currents to the AE (AU, AL) indices of auroral electrojet activity, Geomagn. Aeron. (Engl. Transl.), 2008, vol. 48, no. 4, pp. 499–503.

3. Barkhatova, O.M., Nonlinear relationships of auroral (AU, AL) and midlatitude (SYM-H and ASY-H) geomagnetic activity indices in the main phase of magnetic storm, Soln.–Zemnaya Fiz., 2013, vol. 23, pp. 100–108.

4. 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.

5. 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. 302–308.

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