Abstract
The small regions in the photosphere where many absorption lines weaken have been investigated by several authors. Sheeley attempted to explain the weakening of neutral lines in terms of a temperature increase on the basis of a simple theoretical model. It is shown that this model is not applicable but that a modified theory is able to interpret the observed behaviour of both neutral and ionized lines in terms of a temperature increase of a few percent.
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References
Chapman, G. A. and Sheeley, N. R.: 1968, Solar Phys. 5, 442.
Engvold, O. and Sheeley, N. R.: 1970, Solar Phys. 12, 69.
Sheeley, N. R.: 1967, Solar Phys. 1, 171.
Sheeley, N.R.: 1969, Solar Phys. 9, 347.
Unsöld, A.: 1955, Physik der Sternatmosphären, Springer, Berlin.
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Mitteilungen aus dem Fraunhofer Institut, Nr. 98.
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Grossmann-Doerth, U. On temperature in line-gap regions. Sol Phys 13, 287–291 (1970). https://doi.org/10.1007/BF00153549
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DOI: https://doi.org/10.1007/BF00153549