Turbulent Kinetic Energy in the Energy Balance of a Solar Flare

The energy released in solar flares derives from a reconfiguration of magnetic fields to a lower energy state, and is manifested in several forms, including bulk kinetic energy of the coronal mass ejection, acceleration of electrons and ions, and enhanced thermal energy that is ultimately radiated a...

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Hlavní autoři: Kontar, E. P., Pérez, J. E., Harra, L. K., Kuznetsov, A. A., Emslie, A. G., Jeffrey, N. L. S., Bian, N. H., Dennis, B. R.
Médium: Článek
Jazyk:English
Vydáno: American Physical Society 2017
Témata:
On-line přístup:http://eprints.uanl.mx/18082/1/402.pdf