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A Facula Model and Its Application to Facula Fine Structures

Published online by Cambridge University Press:  14 August 2015

E. Wiehr  and
G. Stellmacher
E. Wiehr
Affiliation:
Universitäts-Sternwarte, Göttingen, F.R.G.
G. Stellmacher
Affiliation:
Universitäts-Sternwarte, Göttingen, F.R.G.

Abstract

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In a recent paper Stellmacher and Wiehr (1973) discussed in detail the discrepancies between ‘continuum-’ and ‘line-profile facula models’. Their calculations show that continuum models (e.g. Kuz'minykh, 1962; Schmahl, 1967; Chapman 1970; Wilson, 1971) encounter the problem that the facula contrast increases towards the limb but decreases with wavelength λ. This discrepancy evidently cannot be due to NLTE effects since it concerns the continumm data.

Type
Part V: The Chromosphere in Active Regions
Information
Symposium - International Astronomical Union , Volume 56: Chromospheric Fine Structure , 1974 , pp. 179 - 181
Copyright
Copyright © Reidel 1974 

References

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