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The Soft X-Ray and EUV Spectra of Solar Flares

Published online by Cambridge University Press:  12 April 2016

K. Nishi  and
K. Tanaka
K. Nishi
Affiliation:
Tokyo Astronomical Observatory, University of Tokyo Mitaka Tokyo, Japan
K. Tanaka
Affiliation:
Tokyo Astronomical Observatory, University of Tokyo Mitaka Tokyo, Japan

Extract

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The Japanese solar maximum satellite HINOTORI was launched on 21 February 1981, and so far 720 Solar flares were detected including many large flares; the largest observed was a X12 class flare occurred on June 6, 1982. Unfortunately, the data recorder malfunctioned in June, 1982, since then the real time basis observation has been possible to continue. The general introductory explanation and some important results were already published in some proceedings (1, 2, 3 ), therefore we would like to focus on presenting some new results of the Soft X-ray spectra obtained by the spectrometers rather than on talking a review.

Type
Session 1. Solar Astrophysics
Information
International Astronomical Union Colloquium , Volume 86: Eighth International Colloquium on Ultraviolet and X-ray Spectroscopy of Astrophysical and Laboratory Plasmas , 1984 , pp. 1 - 8
Copyright
Copyright © Naval Research Laboratory 1984. Publication courtesy of the Naval Research Laboratory, Washington, DC.

References

(1) Proceedings of HINOTORI symposium on Solar Flares; (Tokyo, 27-29 January, 1982) published by ISAS, May(982)Google Scholar
(2) Proceedings of US-Japan Seminor on Recent Advance in Understanding of Solar Flares, Solar Phys., 86, Nos. 1,2(1983)Google Scholar
(3) Proceedings of the Japan-France Seminor on Active Phenomena in the Outer Atmosphere of the Sun and Stars, (Paris, 3-7 Octover 1983) publiched by CNRS, (1984)Google Scholar
Akita, K., Tanaka, K. and Watanabe, T. 1983, ‘Solar Phys.’ 86, 101.CrossRefGoogle Scholar
Akita, K., 1984, private communication.Google Scholar
Bely-Dubau, F., Dubau, J., Faucher, P., and Gabriel, A.H. 1932a, M. N. R. A. S. 198, 239.CrossRefGoogle Scholar
Bely-Dubau, F. et al. 1982b, M. N. R. A. S., 201, 1155.CrossRefGoogle Scholar
Doschek, G.A., Feldmann, U., Kreplin, R.W., and Cohen, L., 1980 Astrophys. J., 239, 725 CrossRefGoogle Scholar
Dubau, J. et al. 1981, M. N. R. A. S. 195, 705.CrossRefGoogle Scholar
Gabriel, A.H. 1972, M. N. R. A. S., 160, 99.CrossRefGoogle Scholar
Hirayama, T., et al., 1984; submitted to Solar Phys.Google Scholar
Moriyama, F., 1984; private communication.Google Scholar
Nishi, K., 1973, Solar Phys., 33, 23.CrossRefGoogle Scholar
Nishi, K., 1975, Solar Phys., 42, 37.CrossRefGoogle Scholar
Shull, J.M., and Van Steenberg, M., 1982, Astrophys. J., Sup. Ser., 48, 95.CrossRefGoogle Scholar
Tanaka, K. and Nishi, K., 1978, Jap. J. Applied Phys. 17, Suppl. 17-2, 461.CrossRefGoogle Scholar
Tanaka, K., Watanabe, T., Nishi, K. and Akita, K., 1982, Astrophys. J. Letters, 254, L59.CrossRefGoogle Scholar
Tanaka, K., Nitta, N., Akita, K., and Watanabe, T., 1983, Solar Phys., 86, 91.CrossRefGoogle Scholar
Tanaka, et al., 1984, Astrophys. J. July 15 issue.Google Scholar
Tanaka, Y., 1983, ISAS Research Note No. 240.Google Scholar
Tsuneta, S., Takakura, T., Nitta, N., Ohki, K., Tanaka, K., Makishima., K., Murakami, T., Oda, M., Ogawara, Y., Kondo, I., 1984, Astrophys. J., 280, 887.CrossRefGoogle Scholar
Watanabe, T., Tanaka, K., and Matsuoka, M., 1982, p. 14; HINITORI Syrap. on Solar Flares; published by ISAS.Google Scholar
Watanabe, T., Tanaka, K., Akita, K., and Nitta, N., 1983, Solar Phys., 86, 107.CrossRefGoogle Scholar