Abstract
Using a parametrized profile of conductive flux, XUV data from coronal active regions on the sun and from late type stars are analyzed. A best χ2 fit is used to deduce the parameters by comparison with experimental data.
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References
Landini M. and Monsignori Fossi B.C. 1984, Physica Scripta T7, 53.
Landini M. and Monsignori Fossi B.C. 1987,in preparation
Oranje B.J. 1986, Astr. Astrophys. 154, 185.
Schrijvert C.J., Zwann C., Maxson V.V., Noyes R.W. 1985, Astr. Astrophys. 149, 123.
Schrijvert C.J. 1986, Astr.Astrophys. in press
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© 1988 Kluwer Academic Publishers
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Fossi, B.C.M., Landini, M. (1988). On Solar and Stellar Coronal Models. In: Havnes, O., Pettersen, B.R., Schmitt, J.H.M.M., Solheim, J.E. (eds) Activity in Cool Star Envelopes. Astrophysics and Space Science Library, vol 143. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-2951-7_37
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DOI: https://doi.org/10.1007/978-94-009-2951-7_37
Publisher Name: Springer, Dordrecht
Print ISBN: 978-94-010-7827-6
Online ISBN: 978-94-009-2951-7
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