Impulsive and hot thermal solar flares
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Saku Tsuneta
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Article
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1987
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Springer
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English
β 563 KB
Some X-class flares (hot thermal flares, HTF) observed with the Hinotori satellite show unique behavior: slow time variability, a compact hard X-ray source containing dense (n > 1011 cm -3) and hot (T > 3 x 1O r K) plasma, and unusually weak ruicrowave emission in spite of the intense magnetic field