Time variations of hard X-ray bursts observed with the solar X-ray telescope aboard HINOTORI (with a movie)

Physics

Scientific paper

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Solar X-Rays, Spaceborne Telescopes, X Ray Telescopes, Bursts, Fourier Transformation, Image Processing, Motion Pictures, Solar Instruments

Scientific paper

The authors have developed a new method for synthesizing hard X-ray maps from the raw data of the Solar X-Ray Telescope (SXT) aboard Hinotori. Using this method they analyzed five typical SXT events and summarized their images in a movie with a time resolution of about 8 s. It shows that (1) three different classes of bursts, i.e., the gradual thermal burst, the multiple impulsive burst, and the extended outburst, have different structures and show quite different variations from each other, and that (2) the source of the extended outburst is located in the corona above 104 km and its shape appears to be a large loop.

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