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- W2314659622 endingPage "21" @default.
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- W2314659622 abstract "It is believed that magnetic energy is stored in the corona via photospheric motions in the form of force-free magnetic fields and/or electric current sheets. To produce flares, both a large storage and a fast release of magnetic free energy are needed, and they may be associated with the coexistence of a spontaneously formed electric current sheet and a highly stressed background magnetic field. The current sheet just serves as a trigger for the impulsive release of the magnetic energy stored in the high stressed field. Any fast release of magnetic energy must be accompanied with various types of MHD waves and shocks, including slow shocks and, perhaps, intermediate shocks. A realistic shock near the sun consists of several segments, which are of different types and pieced together according to certain rules, and it evolves and changes its structure while propagating outward into the interplanetary medium." @default.
- W2314659622 created "2016-06-24" @default.
- W2314659622 creator A5069396700 @default.
- W2314659622 date "1991-01-01" @default.
- W2314659622 modified "2023-10-02" @default.
- W2314659622 title "Magnetic Energy Storage and Release" @default.
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- W2314659622 doi "https://doi.org/10.5636/jgg.43.supplement1_11" @default.
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