RUS  ENG JOURNALS   PEOPLE   ORGANISATIONS   CONFERENCES   SEMINARS   VIDEO LIBRARY   PERSONAL OFFICE
 General information Latest issue Forthcoming papers Archive Impact factor Guidelines for authors License agreement Search papers Search references RSS Latest issue Current issues Archive issues What is RSS

 Trudy MIAN: Year: Volume: Issue: Page: Find

 Tr. Mat. Inst. Steklova, 2013, Volume 281, Pages 199–214 (Mi tm3472)

Collision of a solar wind shock wave with the Earth's bow shock. Wave flow pattern

E. A. Pushkar, A. S. Korolev

Moscow State Industrial University, Moscow, Russia

Abstract: The wave pattern of the flow developed when a solar wind shock wave propagates along the surface of the Earth's bow shock is studied. The investigation is carried out in the three-dimensional non-plane-polarized formulation within the framework of the ideal magnetohydrodynamic model in which the medium is assumed to be inviscid and non-heat-conducting and to have the infinite conductivity. The global three-dimensional pattern of the interaction which is a function of the latitude and longitude of elements on the surface of the bow shock is constructed as a mosaic of solutions to the problem of breakdown of a discontinuity developed between the states behind the impinging and bow shocks on the moving curve of intersection of their fronts. The investigation is carried out for typical solar wind parameters and interplanetary magnetic field strength in the Earth's orbit and for several Mach numbers of the interplanetary shock wave, which makes it possible to trace the evolution of the flow developed as a function of the intensity of the shock perturbation of the solar wind. The solution obtained is necessary for interpreting measurements carried out by spacecraft located in the neighborhood of the Lagrange point and the Earth's magnetosphere.

DOI: https://doi.org/10.1134/S0371968513020167

Full text: PDF file (358 kB)
References: PDF file   HTML file

English version:
Proceedings of the Steklov Institute of Mathematics, 2013, 281, 189–203

Bibliographic databases:

Document Type: Article
UDC: 533.6.011.72+537.84+550.385.41

Citation: E. A. Pushkar, A. S. Korolev, “Collision of a solar wind shock wave with the Earth's bow shock. Wave flow pattern”, Modern problems of mechanics, Collected papers. Dedicated to Academician Andrei Gennad'evich Kulikovskii on the occasion of his 80th birthday, Tr. Mat. Inst. Steklova, 281, MAIK Nauka/Interperiodica, Moscow, 2013, 199–214; Proc. Steklov Inst. Math., 281 (2013), 189–203

Citation in format AMSBIB
\Bibitem{PusKor13} \by E.~A.~Pushkar, A.~S.~Korolev \paper Collision of a~solar wind shock wave with the Earth's bow shock. Wave flow pattern \inbook Modern problems of mechanics \bookinfo Collected papers. Dedicated to Academician Andrei Gennad'evich Kulikovskii on the occasion of his 80th birthday \serial Tr. Mat. Inst. Steklova \yr 2013 \vol 281 \pages 199--214 \publ MAIK Nauka/Interperiodica \publaddr Moscow \mathnet{http://mi.mathnet.ru/tm3472} \crossref{https://doi.org/10.1134/S0371968513020167} \elib{http://elibrary.ru/item.asp?id=20193389} \transl \jour Proc. Steklov Inst. Math. \yr 2013 \vol 281 \pages 189--203 \crossref{https://doi.org/10.1134/S0081543813040160} \isi{http://gateway.isiknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcApp=PARTNER_APP&SrcAuth=LinksAMR&DestLinkType=FullRecord&DestApp=ALL_WOS&KeyUT=000322390600016} 

• http://mi.mathnet.ru/eng/tm3472
• https://doi.org/10.1134/S0371968513020167
• http://mi.mathnet.ru/eng/tm/v281/p199

 SHARE:

Citing articles on Google Scholar: Russian citations, English citations
Related articles on Google Scholar: Russian articles, English articles

This publication is cited in the following articles:
1. A. S. Korolev, E. A. Pushkar, “Stolknovenie mezhplanetnoi udarnoi volny s okolozemnoi golovnoi udarnoi volnoi. Gidrodinamicheskie parametry i magnitnoe pole”, Izvestiya Rossiiskoi akademii nauk. Mekhanika zhidkosti i gaza, 2014, no. 2, 148–168
2. D. V. Donskoi, E. A. Pushkar, “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 Dyn., 51:3 (2016), 406–418
3. D. V. Donskoi, E. A. Pushkar, “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 Dyn., 52:3 (2017), 442–453
•  Number of views: This page: 118 Full text: 12 References: 31