Titlebook: Observational Plasma Astrophysics: Five Years of Yohkoh and Beyond; Tetsuya Watanabe,Takeo Kosugi,Alphonse C. Sterling Book 1998 Springer

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Studies of Coronal Temperatureorly known. There are few, if any, full sun temperature maps of the solar corona in the literature. The soft x-ray telescope (SXT) on . is able to provide useful temperature maps for regions where the x-ray signal is sufficiently strong. Previous SXT studies have shown that the coronal temperature d

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gonioscopy

Sleep-Paralysis

Comparison between Statistical Features of X-ray Fluctuations from the Solar Corona and Accretion Dith ranges, including radio, H-alpha, soft X-ray, hard X-ray, and gamma-ray, mainly in order to explain coronal heating and periodicities of flares (e.g., Drake 1971; Datlowe, Elcan, & Hudson 1974; Lin et al. 1984; Dennis 1985; Rieger et al. 1984; Kile & Cliver 1991; Bai & Sturrock 1993). Also, follo

Cumbersome

From the Sun to the Galaxy Clusterst has unprecedented angular resolution of ~ 5. over a wide energy range of 15–95 keV. With HXT, clear evidence of particle acceleration due to magnetic reconnection was obtained (Sakao et al. 1992; Saka 1994; Masuda 1994; Masuda et al. 1994), and the flare morphology was mathematically quantified (I

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