Analysis of high resolution stellar line profiles

  • David F. Gray
2. Observed Properties of Stellar Turbulence
Part of the Lecture Notes in Physics book series (LNP, volume 114)


Fourier Domain Solar Flux Noise Filter Spectral Line Shape Wavelength Domain 
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.


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Copyright information

© Springer-Verlag 1980

Authors and Affiliations

  • David F. Gray
    • 1
  1. 1.Department of AstronomyUniversity of Western OntarioLondonCanada

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