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24, 35, 1996. , H. Kurokawa, S. Enome, H. Nakajima, K. Shibasaki, M. Nishio, T . Takano, C, Torii, H. Sekiguchi, and S. Kawashima, Simultaneous observations of a promi­ nence eruption followed by a coronal arcade formation in radio, soft X-rays, and H a , Publ. Astr. Soc. Japan, 46, 205-216, 1994. Hansen, R. , C. G. , S. F . Hansen, and E. Yasukawa. Abrupt depletions of the inner corona, Publ. Astr. Soc. Pacific, 8 6 , 500-515, 1974. , T h e n a t u r e of solar flares associated with coro­ nal m a s s ejection, Astr.

In general the main arcade brightening follows the mass ejection and the impulsive phase of any associated flare ("impulsive" here means non-thermal energy release as detected in hard X-ray bremsstrahlung; Hudson et ai [1994] show that this occurs even in slowly-rising arcade events). In some of the cases that have been studied, the Yoh­ koh SXT observations show details of the origin of the ejected material. For example, the 13 November 1994 cloud event has the appearance of a large structure with approximately one full twist (~27r); the structure ap­ pears to be anchored at one end in a flaring active region [Hudson et ai, 1996b].

A. , p 3, D. Reidel, Hingham, MA, 1977. J. J. Michels, R. Tousey, CR. E. T. T. T. J. Garcia, and E. Yasukawa, Synoptic observa­ tions of the solar corona during carrington rotations 1580 - 1596 (11 October 1971 - 15 January 1973), World Data Center A, Report U A G 4 8 A , 1975. R. J. J. Michels, Coronal Mass Ejections 1979-1981, J. Geophys. , 90, 8173, 1985. R. J. J. G. Marsden, p 107, D. Reidel, Dordrecht, 1986. R. Jokipi, CP. S. Giampapa, in press, University of Arizona Press, Tucson, AZ, 1997.

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