Sustaining the hot solar corona requires an energy flux of up to about 107 erg cm-2s-1 whose source must be the photospheric motions below. However, the precise way this energy is transferred and damped still remains an open question. Here a review of recent advances in theoretical models for coronal heating, in the light of the fundamental observational results of the last decade, will be presented.
Models for magnetic heating of the solar atmosphere / Del Zanna, Luca. - In: MEMORIE DELLA SOCIETÀ ASTRONOMICA ITALIANA. - ISSN 1824-016X. - STAMPA. - 74:(2003), pp. 675-682.
Models for magnetic heating of the solar atmosphere
DEL ZANNA, LUCA
2003
Abstract
Sustaining the hot solar corona requires an energy flux of up to about 107 erg cm-2s-1 whose source must be the photospheric motions below. However, the precise way this energy is transferred and damped still remains an open question. Here a review of recent advances in theoretical models for coronal heating, in the light of the fundamental observational results of the last decade, will be presented.
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