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- W84962960 abstract "From the spectral fit parameters, we plot the line flux ratio against the fitted isothermal continuum temperature. The theoretical prediction by Phillips (2004) is shown for comparison. For each flare, there is a clear correlation between the line flux ratio and the continuum temperature. However, some of the correlation curves do not agree with each other. Since the relationship between the line flux ratio and the flare temperature should not vary from flare to flare, something is clearly different between the flares shown. All of the data differ quite significantly from the theoretical prediction — this issue is being actively explored." @default.
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- W84962960 date "2004-01-01" @default.
- W84962960 modified "2023-09-23" @default.
- W84962960 title "Characterizing thermal and non-thermal electron populations in solar flares using RHESSI" @default.
- W84962960 hasPublicationYear "2004" @default.
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