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
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
- 828 KB
- Volume
- 35
- Category
- Article
- ISSN
- 0038-0938
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โฆ Synopsis
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 is consistent with our previous CN(0, 0) 23883 spectra. We derive a solar carbon abundance of logAe = 8.30-t-0.10 compared to the HSRA value of logAe = 8.55 โข 0.10. In addition we specify the regions of formation for the CN(0, 0) 23883.35 and CN(1, 1) 23871.38 bandheads at disc center and limb.
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