| Issue |
A&A
Volume 537, January 2012
|
|
|---|---|---|
| Article Number | C1 | |
| Number of page(s) | 1 | |
| Section | The Sun | |
| DOI | https://doi.org/10.1051/0004-6361/201016297e | |
| Published online | 19 December 2011 | |
Rotation of an erupting filament observed by STEREO EUVI and COR1 instruments (Corrigendum)⋆
1 INAF – Turin Astronomical Observatory, Pino Torinese (TO), Italy
e-mail: bemporad@oato.inaf.it
2 Royal Observatory of Belgium, Brussels, Belgium Institute of Geodynamics of the Romanian Academy, Bucharest, Romania
Research Center for Atomic Physics and Astrophysics, Faculty of Physics, University of Bucharest, Romania
e-mail: marilena@oma.be
3 Department of Applied Mathematics and Theoretical Physics, University of Cambridge, Wilberforce Road, Cambridge CB3 0WA, UK
e-mail: durgesh@iucaa.ernet.in
This article has no abstract.
Key words: Sun: filaments, prominences / Sun: corona / Sun: coronal mass ejections (CMEs) / errata, addenda
© ESO, 2012
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.
