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ISBN-10: 087590081X

ISBN-13: 9780875900810

ISBN-10: 111866437X

ISBN-13: 9781118664377

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Published by means of the yank Geophysical Union as a part of the Geophysical Monograph Series.


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Submitted, 1996. Gosling, J. , D. J. McComas, J. L. Phillips, and S. J. Bame, Geomagnetic activity associated with E a r t h pas­ sage of interplanetary shock disturbances and coronal mass ejections, J. Geophys. , 9 6 , 7831-7839, 1991. Gosling, J. , Corotating and transient solar wind flows in three dimensions, Annu. Rev. Astron. , 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.

8 x 10 K and appears to trace the lowlying magnetic field. Schwenn et al. [1997] have presented s o m e initial observations from C I . In Figure 7 the green line structure during February 1996 is shown. 07 nm spectral band at the core of the Fe XIV green line. , 1997]. These small loops are quite stable, but s h o w continual small-scale motions. T h e impression is that the motions are outward, but no loops are actually seen at these latitudes at higher heights. T h i s may be an observational problem, due to the emission line moving out of the narrow passband of the Fabry-Perot interferometer.

W. Leibacher, Chromospheric evaporation in a well-observed compact flare, Ap. , 2 6 3 , 409-422, 1982. Acton, L. , S. T s u n e t a , Y. Ogawara, R. Bentley, M. Bruner, R. Canfield, L. Culhane, G. Doschek, E. Hiei, and T . Hirayama, T h e Yohkoh mission for high-energy solar physics, Science, 2 5 8 , 618-621, 1992. , H. S. Hudson, G. Slater, A. McAllister, and K. Harvey, T h e large-scale coronal eruptive event of April 14, 1994, in Solar Dynamic Phenomena and Solar Wind Consequences: Proceedings of the Third SOHO Workshop, ESA SP-373, 187-190, 1994.

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Coronal Mass Ejections

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