THE PRESENCE OF $C_2$ LINES IN SUNSPOTS

  • Yun, Hong-Sik (Department of Astronomy, Seoul National University) ;
  • Beebe, H.A. (Department of Astronomy, New Mexico State University) ;
  • Baggett, W.E. (Department of Astronomy, New Mexico State University)
  • 발행 : 1982.08.31

초록

High spatial and spectral resolution observations have been made over a sunspot (SPO 6403) with the Echelle Spectrograph at the Vacuum Tower Telescope, Sacramento Peak Observatory. Our observed spectra, scanned with SPO's fast microdensitometer, clearly show strengthening of $C_2$ lines in the penumbra relative to the photosphere and much weakening in the umbra in agreement with the predictions made by our molecular equilibrium calculations (Lee et al. 1981).

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