Study of the post-flare loops on 29 July 1973. I - Dynamics of the X-ray loops

Physics

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Dynamic Models, Loops, Solar Flares, X Ray Fluorescence, X Ray Imagery, Bandpass Filters, Graphs (Charts), H Alpha Line, Morphology, Solar Activity, Solar Limb, Solar Physics, Spatial Filtering

Scientific paper

We derive an empirical model of the X-ray emitting post-flare loops
observed during the decay phase of the 29 July 1973 flare. We find that
the loops are elliptical, with the brightest emitting region at the
tops. We determine the height, velocity of growth, and ratio of height
to width of the loops at times from 3 to 12 hr after the flare onset.

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