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Spectral Analysis of a White Light Flare

Published online by Cambridge University Press:  27 September 2017

Boyer R.  and
Sotirovski P.
Boyer R.
Affiliation:
Observatoire de Meudon, F - 92195 MEUDON
Sotirovski P.
Affiliation:
Observatoire de Meudon, F - 92195 MEUDON

Abstract

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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

References

Boyer, R., Machado, M.E., Rust, D.M. and Sotirovski, P. : 1905. Solar Phys. 98, 255.Google Scholar
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Svestka, Z. : 1965. Adv. Astron. Astrophys. 3, 119.Google Scholar