Electron acceleration in a wavy shock front

Number of the records: 1

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SYSNO ASEP	0361489
Document Type	J - Journal Article
R&D Document Type	Journal Article
Subsidiary J	Článek ve WOS
Title	Electron acceleration in a wavy shock front
Author(s)	Vandas, Marek (ASU-R)_{RID, ORCID} Karlický, Marian (ASU-R)_{RID, ORCID}
Number of authors	2
Source Title	Astronomy & Astrophysics. - : EDP Sciences - ISSN 0004-6361 Roč. 531, July (2011), A55/1-A55/8
Number of pages	8 s.
Language	eng - English
Country	FR - France
Keywords	shock waves ; acceleration of particles ; magnetic fields ; solar radio radiation
Subject RIV	BN - Astronomy, Celestial Mechanics, Astrophysics
R&D Projects	IAA300030701 GA AV ČR - Academy of Sciences of the Czech Republic (AV ČR)
	ME09009 GA MŠMT - Ministry of Education, Youth and Sports (MEYS)
	GA205/09/0170 GA ČR - Czech Science Foundation (CSF)
	GAP209/10/1680 GA ČR - Czech Science Foundation (CSF)
CEZ	AV0Z10030501 - ASU-R (2005-2011)
UT WOS	000293017700047
DOI	10.1051/0004-6361/201016135
Annotation	On average, a wavy shock front does not significantly increase an acceleration efficiency. Energy gain remarkably exceeds an average level for some combinations of initial parameters. Distribution functions of accelerated electrons have a patchy structure, which is prone to inducing plasma instabilities that will generate plasma waves. This may have relevance to the problem of type II burst origin.
Workplace	Astronomical Institute
Contact	Radka Svašková, bibl@asu.cas.cz, Tel.: 323 620 326
Year of Publishing	2012

Number of the records: 1