Computer Science
Scientific paper
Feb 1992
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992nascp3137..490h&link_type=abstract
In NASA. Goddard Space Flight Center, The Compton Observatory Science Workshop p 490-501 (SEE N92-21874 12-90)
Computer Science
1
Gamma Rays, Magnetic Field Configurations, Photosphere, Potential Fields, Solar Flares, Solar Magnetic Field, Solar Radiation, Flux Density, Line Of Sight, Morphology
Scientific paper
The vector magnetic field configuration of the solar active region AR 6659 that produced very high levels of flare activity in Jun. 1991 is described. The morphology and evolution of the photospheric fields are described for the period 7-10 Jun., and the flares taking place around these dates and their locations relative to the photospheric fields are indicated. By comparing the observed vector field with the potential field calculated from the observed line-of-sight flux, we identify the nonpotential characteristics of the fields along the magnetic neutral lines where the flares were observed. These results are compared with those from the earlier study of gamma-ray flares.
Hagyard Mona J.
Kenney E. G.
Smith Edward. J.
Trussart F.-M.
West Edward A.
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