Why P/OF should look for evidences of over-dense structures in solar flare hard X-ray sources

Details Why P/OF should look for evidences of over-dense structures in solar flare hard X-ray sources Why P/OF should look for evidences of over-dense structures in solar flare hard X-ray sources

Apr 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986sfcp.nasa..142n&link_type=abstract

In NASA. Marshall Space Flight Center Solar Flares and Coronal Physics Using P/OF as a Research Tool p 142-145 (SEE N86-24614

Physics

Occultation, Pinhole Cameras, Solar Flares, Solar X-Rays, Chromosphere, Density (Mass/Volume), High Resolution, Spatial Resolution

Scientific paper

White-light and hard X-ray (HXR) observations of two white-light flares (WLFs) show that if the radiative losses in the optical continuum are powered by fast electrons directly heating the WLF source, then the column density constraints imposed by the finite range of the electrons requires that the WLF consist of an over-dense region in the chromosphere, with density exceeding 10 to the 14th power/cu cm. Thus, we recommend that P/OF search for evidences of over-dense structures in HXR images obtained simultaneously with optical observations of flares.

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