Flare Loop Geometry

Details Flare Loop Geometry Flare Loop Geometry

Dec 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999spro.proc..343n&link_type=abstract

Solar Physics with Radio Observations, Proceedings of the Nobeyama Symposium, held in Kiyosato, Japan, Oct. 27-30, 1998, Edited

Physics

Scientific paper

We discuss how much we can learn about the geometry of flare loops from the X-ray imagery presently available. The stereoscopic techniques, which make use of different projections caused by solar rotation, are not applicable to flare loops, because of their dynamic nature. With an assumption that the loop is contained in a plane, a single image provides a family of loop shapes as a function of the inclination angle of the loop plane with respect to the plane normal to the surface. It appears that various ways exist that may enable us to constrain the inclination angle.

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