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Solar Vector Magnetograms of the Okayama Astrophysical Observatory

  • Mitsugu Makita
  • Shigeo Hamana
  • Keizo Nishi
  • Minoru Shimizu
  • Takashi Sakurai
  • Kiyoto Shibasaki

Abstract

The title instrument is mounted on the 65 cm solar Coudé telescope at the Okayama observatory. Observation is usually of the FeI 5250 Å line. The data obtained are briefly described.

Keywords

Stokes Parameter Line Wing Wollaston Prism White Light Flare Minute Oscillation 
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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References

  1. Makita, M., Hamana, S., and Nishi, K.: 1985, in M. J. Hagyard (ed.), Measurements of Solar Vector Magnetic Fields, NASA CP 2374, p. 173.Google Scholar
  2. Makita, M., Hamana, S., Kawakami, H., and Nishi, K.: 1982, Ann. Tokyo Astron. Obs. 19, 24.ADSGoogle Scholar
  3. Makita, M., Hamana, S., Nishi, K., Shimizu, M., Koyano, H., Sakurai, T., and Komatsu, H.: Publ. Astron. Soc. Japan 37 (in press).Google Scholar
  4. Makita, M., Nishi, K., Shimizu, M., Hamana, S., Sakurai, T., Grigoryev, V. M., Kuklin, G. V., and Selivanov, V. L.: 1985, in M. J. Hagyard (ed.), Measurements of Solar Vector Magnetic Fields, NASA CP 2374, p. 399.Google Scholar
  5. Sakurai, T.: 1982, Solar Phys. 76, 301.ADSCrossRefGoogle Scholar
  6. Sakurai, T. and Makita, M.: 1984, Vector Magnetograms of Solar Active Regions, December 1982-December 1983, Okayama Astrophys. Obs., Tokyo Astron. Obs.Google Scholar

Copyright information

© D. Reidel Publishing Company 1986

Authors and Affiliations

  • Mitsugu Makita
    • 1
  • Shigeo Hamana
    • 1
  • Keizo Nishi
    • 1
  • Minoru Shimizu
    • 1
  • Takashi Sakurai
    • 2
  • Kiyoto Shibasaki
    • 3
  1. 1.Tokyo Astronomical ObservatoryUniversity of TokyoMitaka, TokyoJapan
  2. 2.Department of AstronomyUniversity of TokyoBunkyo-ku, TokyoJapan
  3. 3.Research Institute of AtmosphericsNagoya UniversityHonohara, ToyokawaJapan

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