Kozlovsky, Ben-Zion and Zirin, Harold (1968) The O VI emission from the sun. Solar Physics, 5 (1). pp. 50-54. ISSN 0038-0938. doi:10.1007/bf00147119. https://resolver.caltech.edu/CaltechAUTHORS:20200702-125854922
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Abstract
The ionization equilibrium of oxygen is calculated for various temperatures. A peculiarity in the dielectronic recombination leads to a considerable fraction of O VI in the corona. Thus, the O VI lines may be emitted from the corona rather than the transition region.
| Item Type: | Article | |||||||||
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| Additional Information: | © 1968 Kluwer Academic Publishers. Provided by the NASA Astrophysics Data System. Received 17 March 1968; Published 01 September 1968; Issue Date September 1968. This work was supported by NASA and ONR (HZ) and by NSF and ONR (BZ). | |||||||||
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| Subject Keywords: | Oxygen; Recombination; Transition Region; Considerable Fraction; Ionization Equilibrium | |||||||||
| Issue or Number: | 1 | |||||||||
| DOI: | 10.1007/bf00147119 | |||||||||
| Record Number: | CaltechAUTHORS:20200702-125854922 | |||||||||
| Persistent URL: | https://resolver.caltech.edu/CaltechAUTHORS:20200702-125854922 | |||||||||
| Official Citation: | Kozlovsky, B., Zirin, H. The O VI emission from the sun. Sol Phys 5, 50–54 (1968). https://doi.org/10.1007/BF00147119 | |||||||||
| Usage Policy: | No commercial reproduction, distribution, display or performance rights in this work are provided. | |||||||||
| ID Code: | 104210 | |||||||||
| Collection: | CaltechAUTHORS | |||||||||
| Deposited By: | Tony Diaz | |||||||||
| Deposited On: | 02 Jul 2020 20:22 | |||||||||
| Last Modified: | 16 Nov 2021 18:29 |
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