Collision of an interplanetary rotational discontinuity with the earth's bow shock. hydrodynamic parameters and magnetic field

DOI10.1134/S0015462815010147zbMath1325.76206OpenAlexW2061123093MaRDI QIDQ893523

Eugene A. Pushkar'

Publication date: 19 November 2015

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

Full work available at URL: https://doi.org/10.1134/s0015462815010147

zbMATH Keywords

solar windbow shockearth's magnetosphereinterplanetary rotational discontinuity

Mathematics Subject Classification ID

Magnetohydrodynamics and electrohydrodynamics (76W05) Meteorology and atmospheric physics (86A10)

Related Items (2)

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

Cites Work

• Unnamed Item
• 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
• 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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