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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.

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