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What is Soft X-Ray Analysis of Solar Flares about?

This study analyzes soft X-ray spectra from three C-class solar flares using the Solar X-ray Monitor (XSM) on the Chandrayaan-2 mission to investigate plasma temperature distributions and elemental abundances. The findings indicate that the plasma during the impulsive phase of flares is better described by multithermal models rather than isothermal ones, revealing two distinct temperature components. Additionally, the study observes variations in elemental abundances, which support the chromospheric evapora

Author

unnimaya kc

Language

EN