Numerical MHD Simulation of the Coupled Evolution of Plasma and Magnetic Field in the Solar Chromosphere. I. Gradual and Impulsive Energisation

Author:

Alekseeva L. M.,Kshevetskii S. P.

Publisher

Springer Science and Business Media LLC

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference34 articles.

1. Alekseeva, L.M.: 1980, Physical nature of the anode explosion in plasma channels. Sov. Tech. Phys. Lett. 6(11).

2. Alekseeva, L.M.: 1997a, Generation of magnetic field by acceleration of Hall plasma and some consequences of this process. In: Bordage, M.C., Gleizes, A. (eds.) XXIII Internat. Conf. on Phenomena in Ionized Gases 2, Université Paul Sabatier, Toulouse, 156.

3. Alekseeva, L.M.: 1997b, Hall effect as a producer of effective gravity and of quasi-acoustic-gravity waves in plasma flows. In: Bordage, M.C., Gleizes, A. (eds.) XXIII Internat. Conf. on Phenomena in Ionized Gases 1, Université Paul Sabatier, Toulouse, 206.

4. Alekseeva, L.M.: 1999, Effective gravity due to the Hall effect and quasi-acoustic-gravity waves in accelerated plasma flows. J. Plasma Phys. 61, 671. DOI . ADS .

5. Alekseeva, L.M.: 2006, The Hall effect as the producer of current sheets in astrophysical plasmas. Astron. Lett. 32, 274. DOI . ADS .

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