Results of the LEBAN diagnostic procedure applied to two SMM-observed flares

Details Results of the LEBAN diagnostic procedure applied to two SMM-observed flares Results of the LEBAN diagnostic procedure applied to two SMM-observed flares

Mar 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988jphys..49..309s&link_type=abstract

(IAU, ESA, CNRS, et al., Colloquium on UV and X-ray Spectroscopy of Astrophysical and Laboratory Plasmas, 102nd, Beaulieu-sur-Me

Other

2

Coronal Loops, Solar Flares, Solar Maximum Mission, Magnetohydrodynamic Turbulence, Solar Limb, Solar Magnetic Field, X Ray Spectroscopy

Scientific paper

The LEBAN procedure has been applied to analyze two SMM-observed flares (on Nov. 12, 1980, about 17:00 UT and on Nov. 18, 1980, about 15:00 UT). Estimated flare loop lengths and cross-sections have been compared with those derived from deconvolved HXIS images and/or estimated in different way by other authors. If the loop semilength L is known from other observations, this makes it possible to estimate the portion beta of the loop which was heated. Time variations of other important parameters characterizing the flare plasma are also discussed.

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