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- W2020360131 abstract "A new numerical MHD model is developed to study the evolution of an active region due to photospheric converging motion, which leads to magnetic-energy buildup in the form of electric current. Because this new MHD model has incorporated finite conductivity, the energy conversion occurs from magnetic mode to thermal mode through Joule dissipation. In order to test the causality relationship between the occurrence of flare and photospheric motion, a multiple-pole configuration with neutral point is used. Using these results it is found that in addition to the converging motion, the initial magnetic-field configuration and the redistribution of the magnetic flux at photospheric level enhance the possibility for the development of a flare." @default.
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- W2020360131 date "1986-01-01" @default.
- W2020360131 modified "2023-09-27" @default.
- W2020360131 title "Numerical simulation of flare energy build-up and release via joule dissipation" @default.
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- W2020360131 doi "https://doi.org/10.1016/0273-1177(86)90115-8" @default.
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