Solar Physics

, Volume 149, Issue 1, pp 143–148 | Cite as

Doppler shifts of metallic lines for a white-light flare

  • M. D. Ding
  • C. Fang
  • T. Okamoto
Article

Abstract

In this paper we investigate the Doppler shifts of the metallic lines for a 3B white-light flare on September 19, 1979. The results show that there is no systematic shift at the line center, while there may appear some asymmetry at the line wing. A possible heating process of this flare is proposed to interpret the observed spectral features.

Keywords

Flare Spectral Feature Line Center Doppler Shift Heating Process 

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Copyright information

© Kluwer Academic Publishers 1994

Authors and Affiliations

  • M. D. Ding
    • 1
  • C. Fang
    • 1
  • T. Okamoto
    • 2
  1. 1.Department of AstronomyNanjing UniversityNanjingChina
  2. 2.National Astronomical ObservatoryTokyoJapan

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