Abstract
The topological model of a flare, with a reasonable accuracy, predicts the location of a flare energy source in the corona. In order to clarify an origin of this energy, we have to consider the non-potential part of magnetic field in an active region. In this Chapter, we discuss the main electric currents related to magnetic reconnection in a large solar flare. More specifically, we continue a study of the Bastille day 2000 flare which topological model was considered in a previous Chapter.
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Somov, B.V. (2013). Electric Currents Related to Reconnection. In: Plasma Astrophysics, Part II. Astrophysics and Space Science Library, vol 392. Springer, New York, NY. https://doi.org/10.1007/978-1-4614-4295-0_7
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