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X-ray temperature-emission measure modeling of the solar corona
Authors:G. G. Cohen  D. W. Keith
Affiliation:(1) Department of Physics and Astronomy, Vassar College, 12601 Poughkeepsie, N.Y., U.S.A.;(2) Present address: Department of Astronomy, Yale University, 06520 New Haven, Conn., U.S.A.
Abstract:Several problems related to the calculation of an emission measure differential in temperature are resolved using a new calculation technique. The analysis of a flare on 20 April, 1976, is used to evaluate the usefulness of this new approach and to estimate its future value.Amelia Earhart Fellow.
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