We have obtained center-to-limb photoelectric spectra of the CN(1, 1) B-X bandhead region 23868-3872/~ at Kitt Peak National Observatory. From these spectra and a detailed analysis of the formation of the CN(1, 1) spectrum we derive a best-fit upper photospheric model differing from the HSRA which i
One- and multi-component models of the upper photosphere based on molecular spectra
โ Scribed by George H. Mount; Jeffrey L. Linsky
- Publisher
- Springer
- Year
- 1974
- Tongue
- English
- Weight
- 513 KB
- Volume
- 36
- Category
- Article
- ISSN
- 0038-0938
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โฆ Synopsis
We have obtained accurate center-to-limb photoelectric spectra of the CH (0, 0)C-X bandhead region 23143-3148 ~ at Kitt Peak National Observatory. From these spectra and a detailed analysis of the formation of the CH(0, 0) spectrum we demonstrate that the best-fit upper photospheric model derived from our previous analyses of CN (0, 0) and CN (1, l) spectra adequately explains the CH C-X observations. In addition we derive a solar carbon abundance of logAc = 8.30 โข โข compared to the HSRA value of logAc = 8.55. This confirms our previous CN analyses which demonstrated that if the HSRA nitrogen abundance of logA.v --7.93 ~ 0. I0 is assumed, then logAc = 8.20 :t: 0.10. We also specify the regions of formation for the CH(0, 0) 23143.47 ,~ bandhead at disc center and limb.
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Spectroheliograms taken in the CN(0, 0) violet band near 23883 A, show very small scale network and cell structures with high contrast. The bandhead itself, which is a broad feature due to overlap of several CN lines, allows the diagnostic simplicity of a continuum since motions, magnetic fields, an
Non-LTE synthetic spectra derived from a detailed analysis of the formation o f the CN (0, 0) 23883 A spectrum are compared with center-limb photoelectric spectra taken at Kitt Peak National Observatory.\*\* Significant non-LTE effects are found and the Kurucz, Altrock-Cannon, Mount-Linsky lI, and H
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