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Calculation of the escape probabilities of Fe
XVII resonance lines for the Voigt profile
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School of Science, Henan University of Science and Technology;
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Published |
05 Dec 2008 |
Issue Date |
05 Dec 2008 |
Using the Voigt profile we obtained, we calculate the escape probabilities of Fe XVII resonance lines at 15.02, 13.28, 12.12, 11.13, 11.02 and 10.12 Å for optically thick plasma, both for slab and cylindrical geometry. The oscillator strength, the number density of the absorbing atoms in the ground state, and the optical depth in the line center are discussed in this calculation. Results show that the escape probabilities for the slab geometry are larger than that for the cylindrical geometry. This calculation is useful for the study of the Fe XVII resonance lines.
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References
1. H. R.Rugge and D. L.McKenzie, Astrophys. J., 1985, 297: 338. doi: 10.1086/163532
2. A. K.Bhatia and J. L. R.Saba, Astrophys. J., 2001, 563: 434. doi: 10.1086/323688
3. A. A. M.Habib and Z.El-Gohary, J. Quant. Spectrosc.Radiat. Transfer., 2002, 72: 341. doi: 10.1016/S0022-4073(01)00128-5
4. H. W.Drawin, F.Emard, and F.Beiter, Plasma Physik, 1973,13: 143
5. F. E.Irons, J. Quant. Spectrosc. Radiat. Transfer., 1979, 22: 21. doi: 10.1016/0022-4073(79)90103-1
6. N.Barakat, M.Medhat, and Z.El-Gohary, J. Quant. Spectrosc. Radiat. Transfer., 1989, 42: 2. doi: 10.1016/0022-4073(89)90098-8
7. G. D.Rostn and F. S.Obaid, J. Quant. Spectrosc.Radiat. Transfer., 2005, 94:255. doi: 10.1016/j.jqsrt.2004.09.007
8. J.He and C. M.Zhang, J. Opt. A: Pure. andAppl. Opt., 2005, 7: 613. doi: 10.1088/1464-4258/7/10/014
9. J.He and Q. G.Zhang, J. Opt. A: Pure. andAppl. Opt., 2007, 9: 565. doi: 10.1088/1464-4258/9/7/003
10. J.He and Q. G.Zhang, Phys. Lett. A, 2006, 359: 256. doi: 10.1016/j.physleta.2006.06.041
11. D.A.Verner, E. M.Verner, and G. J.Ferland, Atomic Data and NuclearData Tables, 1996, 64: 1. doi: 10.1006/adnd.1996.0018
12. A. K.Bhatia and S. O.Kastner, Astrophys. J., 1999, 516: 482. doi: 10.1086/307085