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- W2044173342 abstract "This paper reports on investigation of the photospheric magnetic fieldline footpoint motion (usually referred to as shear motion) and magnetic flux emerging from below the surface in relation to energy storage in a solar flare. These causality relationships are demonstrated by using numerical magnetohydrodynamic simulations. From these results, one may conclude that the energy stored in solar flares is in the form of currents. The dynamic process through which these currents reach a critical value is discussed as well as how these currents lead to energy release, such as the explosive events of solar flares." @default.
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- W2044173342 date "1993-06-01" @default.
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- W2044173342 title "Numerical modeling of the energy storage and release in solar flares" @default.
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- W2044173342 doi "https://doi.org/10.1016/0021-9169(93)90087-f" @default.
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