Three-dimensional magnetohydrodynamic description of the process of impingement of a solar wind rotational discontinuity on the Earth's bow shock

DOI10.1134/S0015462811020141zbMath1233.76126MaRDI QIDQ665626

Eugene A. Pushkar'

Publication date: 5 March 2012

Published in: Fluid Dynamics (Search for Journal in Brave)

zbMATH Keywords

solar windbow shockEarth's magnetospheremagnetosheathinteraction between discontinuitiesrotational discontinuity

Mathematics Subject Classification ID

Magnetohydrodynamics and electrohydrodynamics (76W05) Hydrodynamic and hydromagnetic problems in astronomy and astrophysics (85A30)

Related Items (5)

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 ⋮ 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 ⋮ Collision of an interplanetary shock wave with the Earth's bow shock. Hydrodynamic parameters and magnetic field ⋮ Collision of an interplanetary rotational discontinuity with the earth's bow shock. hydrodynamic parameters and magnetic field ⋮ Collision of a solar wind shock wave with the Earth's bow shock. Wave flow pattern

Cites Work

• Three-dimensional magnetohydrodynamic description of the process of collision of a solar wind shock wave and the Earth's bow shock
• Oblique interaction of an Alfvén discontinuity and a fast magnetohydrodynamic shock wave propagating in opposite directions
• Nonregular interaction of shock waves in magnetohydrodynamics
• Oblique non-plane-polarized MHD shock waves and their interaction

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