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Magnetohydrodynamic waves in coronal polar plumes
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UNSPECIFIED (2006) Magnetohydrodynamic waves in coronal polar plumes. In: Discussion Meeting on MHD Waves and Oscillations in the Solar Plasma, Royal Soc, London, ENGLAND, MAR 14-15, 2005. Published in: PHILOSOPHICAL TRANSACTIONS OF THE ROYAL SOCIETY A-MATHEMATICAL PHYSICAL AND ENGINEERING SCIENCES, 364 (1839). pp. 473-483. doi:10.1098/rsta.2005.1711 ISSN 1364-503X.
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Official URL: http://dx.doi.org/10.1098/rsta.2005.1711
Abstract
Polar plumes are cool, dense, linear, magnetically open structures that arise from predominantly unipolar magnetic footpoints in the solar polar coronal holes. As the Alfven speed is decreased in plumes in comparison with the surrounding medium, these structures are natural waveguides for fast and slow magnetoacoustic waves. The simplicity of the geometry of polar plumes makes them an ideal test ground for the study of magnetohydrodynamic (MHD) wave interaction with solar coronal structures. The review covers recent observational findings of compressible and incompressible waves in polar plumes with imaging and spectral instruments, and interpretation of the waves in terms of MHD theory.
Item Type: | Conference Item (UNSPECIFIED) | ||||
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Subjects: | Q Science | ||||
Journal or Publication Title: | PHILOSOPHICAL TRANSACTIONS OF THE ROYAL SOCIETY A-MATHEMATICAL PHYSICAL AND ENGINEERING SCIENCES | ||||
Publisher: | ROYAL SOCIETY | ||||
ISSN: | 1364-503X | ||||
Official Date: | 15 February 2006 | ||||
Dates: |
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Volume: | 364 | ||||
Number: | 1839 | ||||
Number of Pages: | 11 | ||||
Page Range: | pp. 473-483 | ||||
DOI: | 10.1098/rsta.2005.1711 | ||||
Publication Status: | Published | ||||
Title of Event: | Discussion Meeting on MHD Waves and Oscillations in the Solar Plasma | ||||
Location of Event: | Royal Soc, London, ENGLAND | ||||
Date(s) of Event: | MAR 14-15, 2005 |
Data sourced from Thomson Reuters' Web of Knowledge
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