• DocumentCode
    976333
  • Title

    Red shift of spectral lines in the Sun´s chromosphere

  • Author

    Marmet, Paul

  • Author_Institution
    Herzberg Inst. of Astrophys., Nat. Res. Council of Canada, Ottawa, Ont., Canada
  • Volume
    17
  • Issue
    2
  • fYear
    1989
  • fDate
    4/1/1989 12:00:00 AM
  • Firstpage
    238
  • Lastpage
    244
  • Abstract
    An unexplained center-to-limb variation (CLV) of solar wavelengths has been known for 75 years. A theory is described which not only explains this variation but also predicts its amplitude without the use of any adjustable parameter. The model considered is based on the fact that the momentum transfer of the solar photons to the electrons of the atoms of the solar atmosphere produces secondary radiation due to bremsstrahlung. The energy of this bremsstrahlung radiation is taken away from the energy of the initial photons and leads to a red shift. No ad hoc parameters are used, and all constants are either fundamental physical constants or well-known solar parameters. The model can explain the variation of the CLV as a function of its position on the disk and near the limb, and even the change in the lineshapes especially near the limb
  • Keywords
    bremsstrahlung; chromosphere; red shift; solar spectra; Sun; amplitude; bremsstrahlung; chromosphere; momentum transfer; red shift; secondary radiation; solar atmosphere; solar photons; spectral lines; Displacement measurement; Documentation; Doppler shift; Earth; Helium; Instruments; Iron; Motion detection; Plasmas; Sun;
  • fLanguage
    English
  • Journal_Title
    Plasma Science, IEEE Transactions on
  • Publisher
    ieee
  • ISSN
    0093-3813
  • Type

    jour

  • DOI
    10.1109/27.24630
  • Filename
    24630