Consequences of chromospheric irradiation in white light flares: An observer's point of view

Details Consequences of chromospheric irradiation in white light flares: An observer's point of view Consequences of chromospheric irradiation in white light flares: An observer's point of view

Sep 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993adspr..13..317n&link_type=abstract

Advances in Space Research, Volume 13, Issue 9, p. 317-320.

Computer Science

1

Scientific paper

Irradiation of the photosphere by chromospheric flare continuum has been suggested as a mechanism of energy transport in white light flares. In this model the flare optical continuum originates from both the chromosphere (Hfb emission) and the photosphere (H- emission). Consequences of the irradiation model include different dependences on viewing angle of the two continuum components and reduction in minimum required chromospheric energy deposition rate, for a given visible light flare intensity, relative to models which assume only a chromospheric source. Testable predictions of the irradiation model, relating to specific effects on spatial variation and timing of flare emissions, are discussed.

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