Abstract The temperature diagnostics of hot flare plasma, obtained from two Solar Maximum Mission instruments (HXIS and BCS), is compared. A good general agreement between the HXIS and BCS-Fe temperature scales has been found. However, for the growth phase of some flares a systematic difference, THXIS>TFe, has been found, which is not likely to be due to the typical non-thermal electron beams. Possible explanation of this effect is briefly discussed.
Intercomparison of flare observations with two SMM spectrometers: BCS and HXIS
Advances in Space Research ; 8 , 11 ; 231-239
1989-01-01
9 pages
Article (Journal)
Electronic Resource
English
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