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Phase mixing of a three dimensional magnetohydrodynamic pulse

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UNSPECIFIED (2002) Phase mixing of a three dimensional magnetohydrodynamic pulse. In: 10th European Solar Physics Meeting, PRAGUE, CZECH REPUBLIC, SEP 09-14, 2002. Published in: SOLAR VARIABILITY: FROM CORE TO OUTER FRONTIERS, VOLS 1 & 2, 506 pp. 67-70. ISBN 92-9092-816-6. ISSN 0379-6566.

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Abstract

Phase mixing of a three dimensional magnetohydrodynamic (MHD) pulse is studied in the compressive, three-dimensional (without an ignorable coordinate) regime. It is shown that the coupling to the compressive modes dramatically enhances the efficiency of decay of an Alfvenic part of a compressible MHD pulse. However, the dynamics of weakly non-plane Alfven waves can still be qualitatively understood in terms of the previous 2.5D models.

Item Type: Conference Item (UNSPECIFIED)
Subjects: Q Science > QB Astronomy
Series Name: ESA SPECIAL PUBLICATIONS
Journal or Publication Title: SOLAR VARIABILITY: FROM CORE TO OUTER FRONTIERS, VOLS 1 & 2
Publisher: EUROPEAN SPACE AGENCY
ISBN: 92-9092-816-6
ISSN: 0379-6566
Official Date: 2002
Dates:
DateEvent
2002UNSPECIFIED
Volume: 506
Number of Pages: 4
Page Range: pp. 67-70
Publication Status: Published
Title of Event: 10th European Solar Physics Meeting
Location of Event: PRAGUE, CZECH REPUBLIC
Date(s) of Event: SEP 09-14, 2002

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