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Coronal electron density measurements using the near-ir [Fe XIII] emission lines

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Abstract

Observations made during the 1991 total solar eclipse and recent observations from NSO/Sac Peak are discussed. The ground-based density measurements will be complimentary to SOHO observations, particularly SOHO electron density measurements.

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References

  • Flower, D.R., Pineau des Forêts, G.: 1973,A&A 24, 181

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  • Penn, M.J., Arnaud, J., Mickey, D.L., LaBonte, B.J.: 1993,preprint

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Authors and Affiliations

  1. National Solar Observatory/Sacramento Peak, National Optical Astronomy Observatories, P.O. Box 62, 88349, Sunspot, NM, USA

    M. J. Penn & J. R. Kuhn

  2. Observatoire Midi-Pyrenees, 14 Avenue Edouard Belin, 31400, Toulouse, France

    J. Arnaud

  3. University of Hawaii, 2680 Woodlawn Drive, 96822, Honolulu, HI, USA

    D. L. Mickey & B. J. Labonte

Authors
  1. M. J. Penn
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  2. J. R. Kuhn
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  3. J. Arnaud
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  4. D. L. Mickey
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  5. B. J. Labonte
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Operated by the Association of Universities for Research in Astronomy, Inc. (AURA) under cooperative agreement with the National Science Foundation

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Penn, M.J., Kuhn, J.R., Arnaud, J. et al. Coronal electron density measurements using the near-ir [Fe XIII] emission lines. Space Sci Rev 70, 185–188 (1994). https://doi.org/10.1007/BF00777865

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  • DOI: https://doi.org/10.1007/BF00777865

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