Ion‐Acoustic Type Instability in Protoplanetary Disk Full article
Conference |
International symposium on plasmas in the laboratory and in the universe: new insights and new challenges 16-19 Sep 2003 , Como |
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Source | Plasmas in the laboratory and in the universe: New Insights and New Challenges Compilation, 2004. ISBN 0-7354-0176-4. |
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Journal |
AIP Conference Proceedings
ISSN: 0094-243X , E-ISSN: 1551-7616 |
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Output data | Year: 2004, Volume: 703, Pages: 280-283 Pages count : 4 DOI: 10.1063/1.1718468 | ||||||||
Authors |
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Affiliations |
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Funding (3)
1 | Siberian Branch of the Russian Academy of Sciences | 148 |
2 | Russian Foundation for Basic Research | 02-01-00864 |
3 | The Ministry of Education and Science of the Russian Federation | 0072/836 |
Abstract:
The computer simulations showed that gravitational instability development in the two‐phase medium of gas‐dust circumstellar disk is the mechanism of protoplanets formation. At the non‐linear stage of instability development, the soliton density waves of high gas density form.
Cite:
Nikitin S.A.
, Snytnikov V.N.
, Vshivkov V.A.
Ion‐Acoustic Type Instability in Protoplanetary Disk
In compilation Plasmas in the laboratory and in the universe: New Insights and New Challenges. 2004. – C.280-283. – ISBN 0-7354-0176-4. DOI: 10.1063/1.1718468 WOS Scopus РИНЦ
Ion‐Acoustic Type Instability in Protoplanetary Disk
In compilation Plasmas in the laboratory and in the universe: New Insights and New Challenges. 2004. – C.280-283. – ISBN 0-7354-0176-4. DOI: 10.1063/1.1718468 WOS Scopus РИНЦ
Identifiers:
Web of science | WOS:000189484400042 |
Scopus | 2-s2.0-38149060053 |
Elibrary | 29489535 |
OpenAlex | W1502892762 |