@inbook{1d88f501e43d433f81aa0730c5e850be,
title = "Basic magnetic configuration and energy supply processes for an interacting flux model of eruptive solar flares",
abstract = "A review is given of our current understanding of: The basic magnetic configuration of a flare, including loop and arcade structures, prominence models and interactions of separate flux systems; the process of preflare energy storage in excess of potential due to photospheric motions; the conditions for flare occurrence, including shear in the corona and complexity and the roles of spot motions, flux cancellation and prominences; theories for eruption by magnetic nonequilibrium. In the course of this, the elements of a new Interacting Flux Model for flares are outlined.",
author = "Priest, {E. R.}",
note = "Publisher Copyright: {\textcopyright} 1992, Springer Science and Business Media Deutschland GmbH. All rights reserved.",
year = "1992",
doi = "10.1007/3-540-55246-4_71",
language = "English",
series = "Lecture Notes in Physics",
publisher = "Springer Science and Business Media",
pages = "1--20",
booktitle = "Lecture Notes in Physics",
address = "United States",
}