On the spectral characteristics and atmospheric models of two types of white-light flares J/A+AS/110/99 J/A+AS/110/99 White-light flares models On the spectral characteristics and atmospheric models of two types of white-light flares C Fang M D Ding Astron. Astrophys. Suppl. Ser. 110 99 1995 1995A&AS..110...99F radio radiation Sun: flares X-rays: general Based on detailed analyses of the solar white-light flares (WLFs) of 1974 September 10, 1979 September 19 and 1991 October 24, the characteristics of two types of WLFs have been distinguished.
Atmospheric parameters for the non-thermal flare model, m0 = 2.5x10^-3^ Atmospheric parameters for the thermal flare model, m0 = 3.2x10^-3^ Atmospheric parameters for the pre-flare model, m0 = 2.62x10^-4^ h Heigh km m-m0 Column mass density, where m0 is the coronal mass density g/cm2 T Temperature K Vt Micro-turbulent velocity km/s N(H) Hydrogen density cm-3 Ne Electron density cm-3 table.texLaTeX version of the tables Patricia Bauer CDS 1994Oct28 J_A+AS_110_99.xml