Advertisement

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)

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.

Keywords

Type Star Differential Emission Measure Late Type Star Solar Type Star Large Activity Region 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

Preview

Unable to display preview. Download preview PDF.

Unable to display preview. Download preview PDF.

References

  1. Landini M. and Monsignori Fossi B.C. 1984, Physica Scripta T7, 53.ADSCrossRefGoogle Scholar
  2. Landini M. and Monsignori Fossi B.C. 1987,in preparationGoogle Scholar
  3. Oranje B.J. 1986, Astr. Astrophys. 154, 185.ADSGoogle Scholar
  4. Schrijvert C.J., Zwann C., Maxson V.V., Noyes R.W. 1985, Astr. Astrophys. 149, 123.ADSGoogle Scholar
  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

Personalised recommendations