Summary: Astronomy & Astrophysics manuscript no. epfinfin c ESO 2012
February 13, 2012
Kinematics and helicity evolution of a loop-like eruptive
prominence
K. Koleva1, M.S. Madjarska2, P. Duchlev1, C. J. Schrijver5, J.-C. Vial3,4, E. Buchlin3,4, and M. Dechev1
1
Institute of Astronomy and National Astronomical Observatory,
Bulgarian Academy of Sciences, 72 Tsarigradsko Chaussee Blvd., 1784 Sofia, Bulgaria
2
Armagh Observatory, College Hill, Armagh BT61 9DG, N. Ireland
3
CNRS, Institut d'Astrophysique Spatiale, UMR8617, 91405 Orsay, France
4
Univ Paris-Sud, Institut d'Astrophysique Spatiale, UMR8617, 91405 Orsay, France
5
Solar and Astrophysics Lab., Lockheed Martin Advanced Techn. Ctr., 3251 Hanover St., Bldg. 252, Palo Alto, CA
94304-1191, USA
Received date, accepted date
ABSTRACT
Aims. We aim at investigating the morphology, kinematic and helicity evolution of a loop-like prominence during its

Source: Armagh Observatory

Collections: Physics