MHD simulation of the distribution of the gasdynamic parameters and magnetic field behind the Earth's bow shock under sharp variations in the solar wind dynamic pressure
DOI10.1134/S0015462817030127zbMath1370.76190OpenAlexW2713913635MaRDI QIDQ2402757
D. V. Donskoj, Eugene A. Pushkar'
Publication date: 14 September 2017
Published in: Fluid Dynamics (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1134/s0015462817030127
contact discontinuitysolar windbow shockEarth's magnetosphereinterplanetary magnetic fieldvariations in dynamic pressure
Shock waves and blast waves in fluid mechanics (76L05) Magnetohydrodynamics and electrohydrodynamics (76W05) Planetary atmospheres (85A20)
Cites Work
- Impact of the interplanetary magnetic field on the wave flow pattern in the neighborhood of the Earth's bow shock under sharp variations in the solar wind dynamic pressure
- Collision of an interplanetary shock wave with the Earth's bow shock. Hydrodynamic parameters and magnetic field
- Three-dimensional magnetohydrodynamic description of the process of collision of a solar wind shock wave and the Earth's bow shock
- Three-dimensional magnetohydrodynamic description of the process of impingement of a solar wind rotational discontinuity on the Earth's bow shock
- Collision of an interplanetary rotational discontinuity with the earth's bow shock. hydrodynamic parameters and magnetic field
- Oblique non-plane-polarized MHD shock waves and their interaction
- Collision of a solar wind shock wave with the Earth's bow shock. Wave flow pattern
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