Skip to content Skip to navigation
University of Warwick
  • Study
  • |
  • Research
  • |
  • Business
  • |
  • Alumni
  • |
  • News
  • |
  • About

University of Warwick
Publications service & WRAP

Highlight your research

  • WRAP
    • Home
    • Search WRAP
    • Browse by Warwick Author
    • Browse WRAP by Year
    • Browse WRAP by Subject
    • Browse WRAP by Department
    • Browse WRAP by Funder
    • Browse Theses by Department
  • Publications Service
    • Home
    • Search Publications Service
    • Browse by Warwick Author
    • Browse Publications service by Year
    • Browse Publications service by Subject
    • Browse Publications service by Department
    • Browse Publications service by Funder
  • Statistics
  • Help & Advice
University of Warwick

The Library

  • Login

Coronal seismology by means of kink oscillation overtones

Tools
- Tools
+ Tools

Andries, J., Van Doorsselaere, Tom, Roberts, B. (Bernard), Verth, G., Verwichte, E. (Erwin) and Erdélyi, R. (Robertus) (2009) Coronal seismology by means of kink oscillation overtones. Space Science Reviews, Vol.149 (No.1-4). pp. 3-29. ISSN 0038-6308

Full text not available from this repository.
Official URL: http://dx.doi.org/10.1007/s11214-009-9561-2

Abstract

The detection of overtones of coronal loop kink oscillations has been an important advance in the development of coronal seismology. It has significantly increased the potential of coronal seismology and has thus initiated important theoretical and observational improvements. New detections of overtones have been made and a reduction of the error bars has been obtained. The efforts of theoreticians to extend eigenmode studies to more general coronal loop models is no longer a matter of checking the robustness of the model but now also allows for the estimation of certain equilibrium parameters. The frequencies of the detected (longitudinal) overtones are in particular sensitive to changes in the equilibrium properties along the loop, especially the density and the magnetic field expansion. Also, attempts have been made to use the limited longitudinal resolution in combination with the theoretical eigenmodes as an additional seismological tool.

Item Type: Journal Item
Subjects: Q Science > QB Astronomy
Divisions: Faculty of Science > Physics
Library of Congress Subject Headings (LCSH): Magnetohydrodynamics, Magnetohydrodynamic waves, Sun -- Corona, Solar oscillations, Solar magnetic fields
Journal or Publication Title: Space Science Reviews
Publisher: Springer
ISSN: 0038-6308
Date: December 2009
Volume: Vol.149
Number: No.1-4
Number of Pages: 27
Page Range: pp. 3-29
Identification Number: 10.1007/s11214-009-9561-2
Status: Peer Reviewed
Publication Status: Published
Funder: Science and Technology Facilities Council (Great Britain) (STFC), Seventh Framework Programme (European Commission) (FP7), Országos Tudományos Kutatási Alapprogramok [Hungarian Scientific Research Fund] (OTKA)
Grant number: K67746 (OTKA)
URI: http://wrap.warwick.ac.uk/id/eprint/6398

Data sourced from Thomson Reuters' Web of Knowledge

Request changes to a record

Actions (login required)

View Item View Item
twitter

Email us: publications@warwick.ac.uk
Contact Details
About Us