The determination of the low-energy cutoff to the spectrum of accelerated electrons is decisive for the estimation of the total nonthermal energy in solar flares. Because thermal bremsstrahlung dominates the low-energy part of flare X-ray spectra, this cutoff energy is difficult to determine with spectral fitting alone. We have used a new method that combines spatial, spectral, and temporal analysis to determine the cutoff energy for the M1.2 flare observed with RHESSI on 2002 April 15. A low-energy cutoff of 24 ± 2 keV is required to ensure that the assumed thermal emissions always dominate over nonthermal emissions at low energies (20 keV) and that the spectral fitting results are consistent with the RHESSI light curves and images. With this cutoff energy, we obtain a total nonthermal energy in electrons of (1.6 ± 1) × 1030 ergs that is comparable to the peak energy in the thermal plasma, estimated from RHESSI observations to be (6 ± 0.6) × 1029 ergs assuming a filling factor of 1.
展开▼
