X-ray spectroscopy of solar flares

Isothermal XSPEC fitting (chisoth / CHIANTI) of 47 SoLEXS-observed M-class flares to trace plasma temperature, emission measure and abundance evolution.

A joint SoLEXS + HEL1OS pipeline combines soft and hard X-ray diagnostics, constraining flare plasma properties across a broader energy range than either instrument alone.

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