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

Periodic spectral line asymmetries in solar coronal structures from slow mangnetoacoustic waves

Tools
- Tools
+ Tools

Verwichte, E. (Erwin), Marsh, M., Foullon, C. (Claire), Van Doorsselaere, Tom, De Moortel, I., Hood, A. W. and Nakariakov, Valery M.. (2010) Periodic spectral line asymmetries in solar coronal structures from slow mangnetoacoustic waves. Astrophysical Journal Letters, 724 (2). L194-L198. ISSN 2041-8213

Full text not available from this repository.
Official URL: http://dx.doi.org/10.1088/2041-8205/724/2/L194

Abstract

Recent spectral observations of upward moving quasi-periodic intensity perturbations in solar coronal structures have shown evidence of periodic line asymmetries near their footpoints. These observations challenge the established interpretation of the intensity perturbations in terms of propagating slow magnetoacoustic waves. We show that slow waves inherently have a bias toward enhancement of emission in the blue wing of the emission line due to in-phase behavior of velocity and density perturbations. We demonstrate that slow waves cause line asymmetries when the emission line is averaged over an oscillation period or when a quasi-static plasma component in the line of sight is included. Therefore, we conclude that slow magnetoacoustic waves remain a valid explanation for the observed quasi-periodic intensity perturbations.

Item Type: Journal Article
Subjects: Q Science > QB Astronomy
Divisions: Faculty of Science > Physics
Journal or Publication Title: Astrophysical Journal Letters
Publisher: IOP Publishing Ltd
ISSN: 2041-8213
Date: 1 December 2010
Volume: 724
Number: 2
Number of Pages: 5
Page Range: L194-L198
Identification Number: 10.1088/2041-8205/724/2/L194
Status: Peer Reviewed
Publication Status: Published
Access rights to Published version: Restricted or Subscription Access
Funder: Royal Society (Great Britain), Engineering and Physical Sciences Research Council (EPSRC), Science and Technology Facilities Council (Great Britain) (STFC), STFC on the CFSA, European Community, Royal Society University
Grant number: ST/F002769/1 (STFC), 220555
URI: http://wrap.warwick.ac.uk/id/eprint/4812

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