A CME Model for the 1992 July 15 Flare on AU Mic Observed by EUVE

S. L. Cully (1), G.H. Fisher (1), Oswald H.W. Siegmund (1), and M. J. Abbott (2),

1) Space Sciences Laboratory, University of California, Berkeley, CA 94720
2) Center for EUV Astrophysics, 2150 Kittredge Street, University of California, Berkeley, CA 94720

ASP Conference Series, 64, pp. 32-34, 1994.

Abstract

We present a simplemodel for the decay phase of a large flare on AU Mic seen by EUVE. The model assume s a cooling, isothermal plasma expanding with a constant velocity reminiiscent of a solar coronal mass ejection (CME).

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