Models of quiescent stellar microwave emission

  • D. E. Gary
Session III: Small Scale Atmosphere Structures: Data
Part of the Lecture Notes in Physics book series (LNP, volume 254)


Models for gyrosynchrotron emission from thermal electrons in dMe stellar coronae are developed using the formula for electron emissivity given by Robinson and Melrose (1984). The most physically plausible model also closely fits VIA observations. A comparison of this model to the observations is presented.


Spectral Shape Rotational Modulation Thermal Electron Stellar Radius Right Hand 


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Copyright information

© Springer-Verlag 1986

Authors and Affiliations

  • D. E. Gary
    • 1
  1. 1.Solar AstronomyPasadena

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