On Solar and Stellar Coronal Models

  • B. C. Monsignori Fossi
  • M. Landini
Conference paper
Part of the Astrophysics and Space Science Library book series (ASSL, volume 143)


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.


Type Star Differential Emission Measure Late Type Star Solar Type Star Large Activity Region 
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  2. Landini M. and Monsignori Fossi B.C. 1987,in preparationGoogle Scholar
  3. Oranje B.J. 1986, Astr. Astrophys. 154, 185.ADSGoogle Scholar
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  5. Schrijvert C.J. 1986, Astr.Astrophys. in pressGoogle Scholar

Copyright information

© Kluwer Academic Publishers 1988

Authors and Affiliations

  • B. C. Monsignori Fossi
    • 1
  • M. Landini
    • 2
  1. 1.Arcetri ObservatoryFirenzeItaly
  2. 2.Dipartimento di FisicaNapoliItaly

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