X-Ray Emission from Flare Collapsing Trap

Details X-Ray Emission from Flare Collapsing Trap X-Ray Emission from Flare Collapsing Trap

Feb 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006ssrv..122..161k&link_type=abstract

Space Science Reviews, Volume 122, Issue 1-4, pp. 161-168

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Computation

Solar Flares, X-Ray Emission, Loop-Top Sources

Scientific paper

An acceleration process in the collapsing magnetic trap, formed in the flare with cusp magnetic field topology, is described. Computations show that high-energy electrons are accumulated in the central part of the collapsing magnetic trap due to an increase of their pitch angles. The effect explains in a natural way the formation of X-ray loop-top sources. Then, using the model with the collapsing trap and considering only the adiabatic heating process, a possible explanation for the motion of the X-ray loop-top source observed at the beginning of some cusp-type flares is presented.

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