Gasdynamics of the solar wind interaction with the interstellar medium

descriptionPublicationkeyboard_double_arrow_right Article 01 Feb 1990 English Publisher:Springer Science and Business Media LLCJournal:Space Science Reviews, volume 52, pages 89-120 (issn: 0038-6308, eissn: 1572-9672,

Copyright policy )

Authors: V. B. Baranov;

doi: 10.1007/bf00704240

Gasdynamics of the solar wind interaction with the interstellar medium

- Summary
- Metrics

Abstract

A survey of the present-day situation in gasdynamical models of solar wind interaction with the local interstellar medium is presented. A role of these models in interpreting a number of observed physical phenomena is investigated. Experimental data and possible observations are considered from the viewpoint of their interpretation on the basis of theoretical models. Our attention is concentrated on the main limitations of the gasdynamical models, in particular, two-shocks model developed by Baranovet al. (1981, 1982).

Related Organizations

Institute for Problems in Mechanics
Russian Federation
Russian Academy of Sciences
Russian Federation

Impact byBIP!

	selected citations These citations are derived from selected sources. 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).	116
	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.	Top 10%
	influence This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).	Top 1%
	impulse This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.	Top 1%