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Article Dans Une Revue Astronomy and Astrophysics - A&A Année : 2004

Relating magnetic field strengths to hard X-ray emission in solar flares

Résumé

The observation of hard X-ray (HXR) emission in solar flares provides important diagnostic information about the acceleration and subsequent transport of energetic electrons in the flare process. However, while hard X-rays are thought to be emitted from the flare footpoints through thick-target bremsstrahlung interactions, the details of the transport of accelerated electrons through the solar atmosphere still remains unclear.
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hal-03730778 , version 1 (05-09-2022)

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C. P. Goff, Sarah A. Matthews, Lidia van Driel-Gesztelyi, Louise K. Harra. Relating magnetic field strengths to hard X-ray emission in solar flares. Astronomy and Astrophysics - A&A, 2004, 423, pp.363-372. ⟨hal-03730778⟩
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