Analysis of OGO-5 and OSO-7 X-ray data

Details Analysis of OGO-5 and OSO-7 X-ray data Analysis of OGO-5 and OSO-7 X-ray data

Feb 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975cait.reptq....m&link_type=abstract

Final Report California Inst. of Tech., Pasadena.

Physics

Magnetic Field Reconnection, Ogo-5, Oso-7, Solar Flares, Solar X-Rays, Conductive Heat Transfer, Cooling, Magnetic Fields, Thermal Plasmas

Scientific paper

The physical nature of solar flares implied by the data was studied. The empirical results were obtained primarily from the OGO-5 and OSO-7 X-ray data in combination with optical data. The principal conclusions regarding the physics of flares are the following. (1) Flares are produced by magnetic field reconnection. (2) The resulting thermal X-ray plasma is cooled primarily by heat conduction rather than by radiative cooling. (3) The heating and cooling of the thermal X-ray plasma are approximately in balance during the maximum phase of the flare.

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