A time dependent relation between EUV solar flare light-curves from lines with differing formation temperatures | Journal of Space Weather and Space Climate

Developing New Space Weather Tools: Transitioning fundamental science to operational prediction systems

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Fig. 1

Panels a–c show the temperature, emission measure and radiative loss found for a canonical C-class solar flare by Raftery et al. (2009). These values are used to compute and the quasi-static ratio shown in Panels d and e. A quasi-static ratio much greater than 1 implies evolves quasi-statically with respect to . The diamonds in Panel a correspond with when the indicated measurements peaked.

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