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This would then increase the mean velocity of the up-flowing heated plasma derived from the least-squares fits to the points in these figures to be closer to 100 km/s, similar to the range of velocities derived from EUV line blue shifts · 1982

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astro-ph.SR 1

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Flare Impulsive-phase Durations

astro-ph.SR · 2026-04-06 · unverdicted · novelty 3.0

Observed time delays in solar flare X-ray emissions are interpreted as the sum of beam heating duration and plasma rise time to loop tops, implying acceleration occurs at the loop top and is quenched by rising density.

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  • Flare Impulsive-phase Durations astro-ph.SR · 2026-04-06 · unverdicted · none · ref 3

    Observed time delays in solar flare X-ray emissions are interpreted as the sum of beam heating duration and plasma rise time to loop tops, implying acceleration occurs at the loop top and is quenched by rising density.