A project, created for analysis of the processes in solar flares' decay phase
In this project we're applying two models of solar-stellar flares for coronal flare [1] and flare in UV spectra [2]
[1] Aschwanden, M.J. and Tsiklauri, D.: 2009. The hydrodynamic evolution of impulsively heated coronal loops: explicit analytical approximations. The Astrophysical Journal Supplement Series, 185, 171.
[2] Cargill, P.J., Mariska, J.T., and Antiochos, S.K.: 1995. Cooling of solar plasmas. I. Theoretical considerations. The Astrophysical Journal, 439, 1034.