Volume 385, Number 3, April III 2002
|Page(s)||1073 - 1077|
|Section||Planets and planetary systems|
|Published online||15 April 2002|
Intermittent behavior in the transition region and the low corona of the quiet Sun
US Naval Research Laboratory, Space Science Division, Washington, DC 20375, USA
2 Mullard Space Science Laboratory, University College London, Holmbury St Mary, Dorking, Surrey, RH5 6NT, UK
3 Institut d'Astrophysique Spatiale, Université Paris XI – CNRS, Bât. 121, 91405 Orsay Cedex, France
Corresponding author: S. Patsourakos, firstname.lastname@example.org
Accepted: 24 January 2002
We present an analysis of light-curves obtained in the O IV and Ne VIII transition region and low corona lines, that were simultaneously recorded in a quiet Sun region by SUMER/SOHO. By using the flatness spectrum of the observed light-curves we searched for intermittency signatures. It was found that a significant proportion of points in the observed area exhibit clear indications of intermittency, irrespectively of their intrinsic intensity. Our findings give favor to an impulsively heated transition region and corona via intermittent-type MHD turbulence.
Key words: Sun: corona / Sun: transition region / Sun: UV radiation
© ESO, 2002
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.