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Spectral Analysis of a White Light Flare
Published online by Cambridge University Press: 27 September 2017
Abstract
We discuss observations of a solar flare located close to the limb (N15, W75) at 07 00 UT on 26 September 1963 from the Crimean Astrophysical observatory.
Stark broadening and hence electron density have been obtained from measured time profile and half-width of the Baliner series lines from Hα to H M.
The emission mechanism has been deduced from a study of the continuum intensity as a function of wavelength.
- Type
- Session II: Solar Flares
- Information
- International Astronomical Union Colloquium , Volume 104 , Issue 2: Solar and Stellar Flares , 1989 , pp. 247 - 250
- Copyright
- Copyright © Kluwer 1989