The initial trajectories of eruptive solar prominences


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Abstract

Trajectories of eruptive prominences are compared with the shapes of coronal neutral surfaces calculated in a potential approximation using photospheric measurements. Space-based Solar Dymamics Observatory and STEREO observations carried out at different viewing angles enable a precise determination of a prominence’s position at successive times during its eruption. In the initial segments of their trajectories, eruptive prominences move along neutral surfaces (Br = 0) of the potential coronal magnetic field. This can be used to predict the directions of subsequent coronal mass ejections and to estimate their geoefficiency.

About the authors

B. P. Filippov

Institute of Terrestrial Magnetism, Ionosphere, and Radio Wave Propagation

Author for correspondence.
Email: bfilip@izmiran.ru
Russian Federation, Troitsk, Moscow, 142190

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