Instability of Kelvin-Helmholtz and magnetohydrodynamic modes on the boundary of geomagnetic tail

Author:

Cheremnykh O.K., ,Cheremnykh S.O.,Kozak L.V.,Kronberg E.A., , ,

Publisher

National Academy of Sciences of Ukraine (Co. LTD Ukrinformnauka)

Subject

Anesthesiology and Pain Medicine

Reference58 articles.

1. Kelvin-Helmholtz Instability in a Bounded Plasma Flow;Burinskaya;Plasma Phys Reports,2008

2. 2. Gossard E. E., Hooke W. H. (1975). Waves in the Atmosphere: Atmospheric Infrasound and Gravity Waves, Their Generation and Propagation. Elsevier Science Ltd., 472 p.

3. 3. Grigoriev Yu. N., Ershov I. V., Zyryanov K. I. (2008). Numerical modeling of Kelvin - Helmholtz waves in a weakly nonequilibrium molecular gas. Computational technol., 13(5), 25-38 (In Russian).

4. The combined Rayleigh - Taylor - Kelvin - Helmholtz instability on a magnetopause;Guglielmi;Solar-Terrestrial phys,2010

5. 5. Ershkovich A. I., Nusinov A. A., Chernikov A. A. (1972). On the Kelvin - Helmholtz instability in cometary tails of type I. Astron. J., 49, 866-871 (In Russian).

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