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

The first measurement of the adiabatic index in the solar corona using time-dependent spectroscopy of hinode/eis observations

Tools
- Tools
+ Tools

Van Doorsselaere, Tom, Wardle, Nick, Del Zanna, Giulio, Jansari, Kishan, Verwichte, E. (Erwin) and Nakariakov, V. M. (Valery M.). (2011) The first measurement of the adiabatic index in the solar corona using time-dependent spectroscopy of hinode/eis observations. The Astrophysical Journal. Letters, Vol.727 (No.2). L32. ISSN 2041-8205

Full text not available from this repository.
Official URL: http://dx.doi.org/10.1088/2041-8205/727/2/L32

Abstract

We use observations of a slow magnetohydrodynamic wave in the corona to determine for the first time the value of the effective adiabatic index, using data from the Extreme-ultraviolet Imaging Spectrometer on board Hinode. We detect oscillations in the electron density, using the CHIANTI atomic database to perform spectroscopy. From the time-dependent wave signals from multiple spectral lines the relationship between relative density and temperature perturbations is determined, which allows in turn to measure the effective adiabatic index to be γeff = 1.10 ± 0.02. This confirms that the thermal conduction along the magnetic field is very efficient in the solar corona. The thermal conduction coefficient is measured from the phase lag between the temperature and density, and is shown to be compatible with Spitzer conductivity.

Item Type: Journal Article
Subjects: Q Science > QB Astronomy
Q Science > QC Physics
Divisions: Faculty of Science > Physics
Library of Congress Subject Headings (LCSH): Adiabatic invariants, Sun -- Corona, Solar oscillations, Astronomical spectroscopy
Journal or Publication Title: The Astrophysical Journal. Letters
Publisher: Institute of Physics Publishing, Inc.
ISSN: 2041-8205
Date: February 2011
Volume: Vol.727
Number: No.2
Page Range: L32
Identification Number: 10.1088/2041-8205/727/2/L32
Status: Peer Reviewed
Publication Status: Published
Access rights to Published version: Restricted or Subscription Access
Funder: European Community (EC), Engineering and Physical Sciences Research Council (EPSRC)
Grant number: 220555 (EC)
URI: http://wrap.warwick.ac.uk/id/eprint/40039

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