Multi-wavelength observations and modelling of a canonical solar flare

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Table 2:

Input parameters used for EBTEL simulation. The parameters were constrained by data when possible and the ranges of parameters investigated are shown.
Parameter	Observed	EBTEL
Loop half-length [cm]	$3\times 10^{9}$	$(3 \pm 0.2)\times10^{9}$
Non-thermal flux
- Amplitude [erg cm^-2 s^-1]	$7\times 10^{9}$	$5 \times 10^{8\pm1}$
- Width [s]	$\sim$ 100	$100\pm50$
- Total [erg cm^-2]	$\sim$ 1.7 $\times$ 10¹²	$2.5\times10^{10\pm1}$
Direct heating rate
- Amplitude [erg cm^-3 s^-1]	-	$0.7\pm 0.3$
- Width [s]	-	$100\pm50$
- Background [erg cm^-3 s^-1]	-	$\le$ $1\times10^{-6}$
- Total [erg cm^-3]	-	$175\pm150$
Direct/non-thermal heating	(best fit parameters)	$\sim$ 4

Source LaTeX | All tables | In the text

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