Derivation of the 3D Structure of Flares in the Homologous Flare Series of 1992 February

Details Derivation of the 3D Structure of Flares in the Homologous Flare Series of 1992 February Derivation of the 3D Structure of Flares in the Homologous Flare Series of 1992 February

Dec 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999spro.proc..413m&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

In February 1992, three flares, which we consider constitute a
homologous flare series, occurred in the active region NOAA7070, and
were observed by the Yohkoh SXT. In this paper, we discuss the 3D
structure of arcade type flare by making use of the different
perspectives of the flare in the homologous flare series.

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