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Interstellar magnetic field effects on the heliosphere

descriptionPublicationkeyboard_double_arrow_right Article , Other literature type 01 Jan 2003Publisher:AIPJournal:AIP Conference Proceedings, volume 679, pages 745-749 (issn: 0094-243X, Copyright policy )
Authors: Romana Ratkiewicz;

doi: 10.1063/1.1618700

Interstellar magnetic field effects on the heliosphere

Abstract

This paper summarizes the numerical results obtained by three‐dimensional MHD simulations of the interaction between the solar wind and interstellar medium in Ratkiewicz and Ben‐Jaffel [2002], Ratkiewicz and McKenzie [2002], and Ratkiewicz and Webb [2002]. We analyze the configuration in which Maxwell stresses lead to squeezing and/or pushing the heliospheric boundary. In particular, we explain the mechanism giving rise to a suction effect of the heliopause. Numerical results for the case of aligned interstellar MHD flow are compared with previous studies.

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This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
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popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
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