Electron acceleration by a wavy shock front: details on angular distribution

Number of the records: 1

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SYSNO ASEP	0361493
Document Type	C - Proceedings Paper (int. conf.)
R&D Document Type	Conference Paper
Title	Electron acceleration by a wavy shock front: details on angular distribution
Author(s)	Vandas, Marek (ASU-R)_{RID, ORCID} Karlický, Marian (ASU-R)_{RID, ORCID}
Number of authors	2
Source Title	Advances in Plasma Astrophysics. - Cambridge : Cambridge University Press, 2011 / Bonanno A. - ISSN 1743-9213 - ISBN 9780521197410
Pages	s. 201-203
Number of pages	3 s.
Action	Symposium of the International Astronomical Union /274./
Event date	06.09.2010-10.09.2010
VEvent location	Giardini Naxos
Country	IT - Italy
Event type	WRD
Language	eng - English
Country	GB - United Kingdom
Keywords	acceleration of particles ; shock waves ; solar corona
Subject RIV	BN - Astronomy, Celestial Mechanics, Astrophysics
R&D Projects	IAA300030805 GA AV ČR - Academy of Sciences of the Czech Republic (AV ČR)
	GA205/09/0170 GA ČR - Czech Science Foundation (CSF)
CEZ	AV0Z10030501 - ASU-R (2005-2011)
UT WOS	000305161800045
DOI	10.1017/S1743921311006934
Annotation	We studied numerically electron acceleration by a perpendicular wavy shock. Distribution function of accelerated electrons is highly anisotropic, with many sharp peaks. The peaks are caused by (usually single) reflections of electrons by the shock and subsequent transmission.
Workplace	Astronomical Institute
Contact	Radka Svašková, bibl@asu.cas.cz, Tel.: 323 620 326
Year of Publishing	2012

Number of the records: 1