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Line Shifts and Asymmetries in the IR Solar Spectrum
Published online by Cambridge University Press: 03 August 2017
Abstract
Line shifts and asymmetries of spectral lines have been found in the ATMOS spectra. These are due to the granulation at the solar surface. A two-component model for the solar photosphere is used to calculate theoretical profiles which are compared to the observations. The ATMOS lines provide additional constraints on models for the solar photosphere.
- Type
- Part 6: The Infrared Spectrum
- Information
- Symposium - International Astronomical Union , Volume 154: Infrared Solar Physics , 1994 , pp. 533 - 537
- Copyright
- Copyright © Kluwer 1994