Rotation of an erupting filament observed by STEREO EUVI and COR1 instruments (Corrigendum)⋆
1 INAF – Turin Astronomical Observatory, Pino Torinese (TO), Italy
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
3 Department of Applied Mathematics and Theoretical Physics, University of Cambridge, Wilberforce Road, Cambridge CB3 0WA, UK
This article has no abstract.
Key words: Sun: filaments, prominences / Sun: corona / Sun: coronal mass ejections (CMEs) / errata, addenda
© ESO, 2012