Transition Region Emission and Energy Input to Thermal Plasma during the Impulsive Phase of Solar Flares | Zendy

J. C. Raymond | Zendy; Gordon D. Holman | Zendy; A. Ciaravella | Zendy; A. V. Panasyuk | Zendy; YuanKuen Ko | Zendy; J. Kohl | Zendy

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Transition Region Emission and Energy Input to Thermal Plasma during the Impulsive Phase of Solar Flares

Author(s) -

J. C. Raymond,

Gordon D. Holman,

A. Ciaravella,

A. V. Panasyuk,

YuanKuen Ko,

J. Kohl

Publication year - 2007

Publication title -

the astrophysical journal

Language(s) - English

Resource type - Journals

SCImago Journal Rank - 2.376

H-Index - 489

eISSN - 1538-4357

pISSN - 0004-637X

DOI - 10.1086/512604

Subject(s) - solar flare , plasma , flare , physics , thermal conduction , thermal , thermal energy , thermal radiation , astrophysics , radiation , radiative transfer , corona (planetary geology) , radiant energy , atomic physics , optics , nuclear physics , meteorology , thermodynamics , astrobiology , venus

The energy released in a solar flare is partitioned between thermal andnon-thermal particle energy and lost to thermal conduction and radiation over abroad range of wavelengths. It is difficult to determine the conductive lossesand the energy radiated at transition region temperatures during the impulsivephases of flares. We use UVCS measurements of O VI photons produced by 5 flaresand subsequently scattered by O VI ions in the corona to determine the 5.0

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