Pasachoff, Jay M. and Zirin, Harold (1971) On K-line central reversals. Solar Physics, 18 (1). pp. 27-28. ISSN 0038-0938. doi:10.1007/bf00146028. https://resolver.caltech.edu/CaltechAUTHORS:20200630-152052528
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Abstract
The double reversal at the center of the spatially-averaged profiles of the H and K resonance lines in the solar atmosphere has been used as a probe to give the distribution of temperature and density with height. Details of the interpretations depend on the mechanism assumed for the formation of the central reversals. The non-LTE theory of stellar atmospheres has succeeded in explaining a symmetric double reversal; the history of this effort has recently been reviewed by Linsky and Avrett (1970).
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| Additional Information: | © 1971 Kluwer Academic Publishers. Provided by the NASA Astrophysics Data System. Received 11 February 1971; Issue Date May 1971. This work was partially supported by NASA Grant NGR 05-002-034 and by NSF Grant No. GA 24015. | |||||||||
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| Issue or Number: | 1 | |||||||||
| DOI: | 10.1007/bf00146028 | |||||||||
| Record Number: | CaltechAUTHORS:20200630-152052528 | |||||||||
| Persistent URL: | https://resolver.caltech.edu/CaltechAUTHORS:20200630-152052528 | |||||||||
| Official Citation: | Pasachoff, J.M., Zirin, H. On K-line central reversals. Sol Phys 18, 27–28 (1971). https://doi.org/10.1007/BF00146028 | |||||||||
| Usage Policy: | No commercial reproduction, distribution, display or performance rights in this work are provided. | |||||||||
| ID Code: | 104171 | |||||||||
| Collection: | CaltechAUTHORS | |||||||||
| Deposited By: | Tony Diaz | |||||||||
| Deposited On: | 30 Jun 2020 22:46 | |||||||||
| Last Modified: | 16 Nov 2021 18:29 |
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