UV Diagnostics of Stellar and Solar Flares

Astronomy and Astrophysics – Astronomy

Scientific paper

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Scientific paper

The UV spectral regime provides a comprehensive view of the plasma dynamics and atmospheric temperature structure during stellar flares. We review the major developments in UV spectroscopy of flares on low mass stars that shape our understanding of the flare process and challenge the predictions of current radiative hydrodynamic models. We put the ultraviolet properties in context with the radiation in the neighboring X-ray and visible wavelength regimes. We also show how SDO/EVE data of several Cycle 24 solar flares allow for new comparisons to be made between solar and stellar flares.

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