๐”– Bobbio Scriptorium
โœฆ   LIBER   โœฆ

Fine structure of convective motions in the solar photosphere: Observations and theory

โœ Scribed by R. I. Kostyk; N. G. Shchukina


Book ID
110139892
Publisher
Springer
Year
2004
Tongue
English
Weight
298 KB
Volume
48
Category
Article
ISSN
1063-7729

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Absolute wavelengths for Fraunhofer lines are compared with laboratory measurements for several atomic and molecular spectra. The wavelength differences are shown to be consistent with the proposal that the deeper layers of the photosphere are in convective motion: ve -~ 3 km/sec for log To> --1.0.

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