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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.
Full text not available from this repository.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 |
| Date: | 2002 |
| 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 |
| URI: | http://wrap.warwick.ac.uk/id/eprint/9000 |
Data sourced from Thomson Reuters' Web of Knowledge
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