Collision of a solar wind shock wave with the Earth’s bow shock. Wave flow pattern
Author:
Publisher
Pleiades Publishing Ltd
Subject
Mathematics (miscellaneous)
Link
http://link.springer.com/content/pdf/10.1134/S0081543813040160.pdf
Reference21 articles.
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2. K. Keika et al., “Deformation and evolution of solar wind discontinuities through their interactions with the Earth’s bow shock,” J. Geophys. Res. 114, A00C26, doi: 10.1029/2008JA013481 (2009).
3. G. Pallocchia et al., “Interplanetary shock transmitted into the Earth’s magnetosheath: Cluster and Double Star observations,” Ann. Geophys. 28, 1141–1156 (2010).
4. A. A. Samsonov et al., “Propagation of a sudden impulse through the magnetosphere initiating magnetospheric Pc5 pulsations,” J. Geophys. Res. 116, A10216, doi: 10.1029/2011JA016706 (2011).
5. A. A. Samsonov, Z. Němeček, and J. Šafránková, “Numerical MHD modeling of propagation of interplanetary shock through the magnetosheath,” J. Geophys. Res. 111, A08210, doi: 10.1029/2005JA011537 (2006).
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1. 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;Fluid Dynamics;2017-05
2. Impact of the Interplanetary Magnetic Field to Impingement of a Solar Wind Rotational Discontinuity on the Earth’s Bow Shock;30th International Symposium on Shock Waves 2;2017
3. Impact of the interplanetary magnetic field on thewave flow pattern in the neighborhood of the Earth’s bow shock under sharp variations in the solar wind dynamic pressure;Fluid Dynamics;2016-05
4. Collision of an interplanetary shock wave with the Earth’s bow shock. Hydrodynamic parameters and magnetic field;Fluid Dynamics;2014-03
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