The angle-dependent redistribution functionsRIII andRIV: Line absorption probability distribution functions and reemission coefficients
Abstract The line absorption probability distribution functions and the reemission coefficients are derived for the non-coherent scattering functionsRIII andRIV. The appropriate line profile function forRIII is shown to be a simple Voigt function, while forRIV, the line absorption probability distri...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
McKenna, Sean J. [verfasserIn] |
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| Format: |
Artikel |
|---|---|
| Sprache: |
Englisch |
| Erschienen: |
1984 |
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| Schlagwörter: |
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| Anmerkung: |
© D. Reidel Publishing Company 1984 |
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| Übergeordnetes Werk: |
Enthalten in: Astrophysics and space science - Kluwer Academic Publishers, 1968, 106(1984), 2 vom: Nov., Seite 299-307 |
|---|---|
| Übergeordnetes Werk: |
volume:106 ; year:1984 ; number:2 ; month:11 ; pages:299-307 |
| Links: |
|---|
| DOI / URN: |
10.1007/BF00650357 |
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| 520 | |a Abstract The line absorption probability distribution functions and the reemission coefficients are derived for the non-coherent scattering functionsRIII andRIV. The appropriate line profile function forRIII is shown to be a simple Voigt function, while forRIV, the line absorption probability distribution function is more complex involving a linear combination of two Voigt functions and another more complex probability distribution. The structure of the reemission coefficients forRIII andRIV is then discussed. | ||
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10.1007/BF00650357 doi (DE-627)OLC206615427X (DE-He213)BF00650357-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn McKenna, Sean J. verfasserin aut The angle-dependent redistribution functionsRIII andRIV: Line absorption probability distribution functions and reemission coefficients 1984 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © D. Reidel Publishing Company 1984 Abstract The line absorption probability distribution functions and the reemission coefficients are derived for the non-coherent scattering functionsRIII andRIV. The appropriate line profile function forRIII is shown to be a simple Voigt function, while forRIV, the line absorption probability distribution function is more complex involving a linear combination of two Voigt functions and another more complex probability distribution. The structure of the reemission coefficients forRIII andRIV is then discussed. Distribution Function Probability Distribution Linear Combination Line Absorption Probability Distribution Function Enthalten in Astrophysics and space science Kluwer Academic Publishers, 1968 106(1984), 2 vom: Nov., Seite 299-307 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:106 year:1984 number:2 month:11 pages:299-307 https://doi.org/10.1007/BF00650357 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_22 GBV_ILN_24 GBV_ILN_31 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2002 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 GBV_ILN_4046 GBV_ILN_4082 GBV_ILN_4103 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4700 AR 106 1984 2 11 299-307 |
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10.1007/BF00650357 doi (DE-627)OLC206615427X (DE-He213)BF00650357-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn McKenna, Sean J. verfasserin aut The angle-dependent redistribution functionsRIII andRIV: Line absorption probability distribution functions and reemission coefficients 1984 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © D. Reidel Publishing Company 1984 Abstract The line absorption probability distribution functions and the reemission coefficients are derived for the non-coherent scattering functionsRIII andRIV. The appropriate line profile function forRIII is shown to be a simple Voigt function, while forRIV, the line absorption probability distribution function is more complex involving a linear combination of two Voigt functions and another more complex probability distribution. The structure of the reemission coefficients forRIII andRIV is then discussed. Distribution Function Probability Distribution Linear Combination Line Absorption Probability Distribution Function Enthalten in Astrophysics and space science Kluwer Academic Publishers, 1968 106(1984), 2 vom: Nov., Seite 299-307 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:106 year:1984 number:2 month:11 pages:299-307 https://doi.org/10.1007/BF00650357 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_22 GBV_ILN_24 GBV_ILN_31 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2002 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 GBV_ILN_4046 GBV_ILN_4082 GBV_ILN_4103 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4700 AR 106 1984 2 11 299-307 |
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10.1007/BF00650357 doi (DE-627)OLC206615427X (DE-He213)BF00650357-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn McKenna, Sean J. verfasserin aut The angle-dependent redistribution functionsRIII andRIV: Line absorption probability distribution functions and reemission coefficients 1984 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © D. Reidel Publishing Company 1984 Abstract The line absorption probability distribution functions and the reemission coefficients are derived for the non-coherent scattering functionsRIII andRIV. The appropriate line profile function forRIII is shown to be a simple Voigt function, while forRIV, the line absorption probability distribution function is more complex involving a linear combination of two Voigt functions and another more complex probability distribution. The structure of the reemission coefficients forRIII andRIV is then discussed. Distribution Function Probability Distribution Linear Combination Line Absorption Probability Distribution Function Enthalten in Astrophysics and space science Kluwer Academic Publishers, 1968 106(1984), 2 vom: Nov., Seite 299-307 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:106 year:1984 number:2 month:11 pages:299-307 https://doi.org/10.1007/BF00650357 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_22 GBV_ILN_24 GBV_ILN_31 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2002 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 GBV_ILN_4046 GBV_ILN_4082 GBV_ILN_4103 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4700 AR 106 1984 2 11 299-307 |
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10.1007/BF00650357 doi (DE-627)OLC206615427X (DE-He213)BF00650357-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn McKenna, Sean J. verfasserin aut The angle-dependent redistribution functionsRIII andRIV: Line absorption probability distribution functions and reemission coefficients 1984 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © D. Reidel Publishing Company 1984 Abstract The line absorption probability distribution functions and the reemission coefficients are derived for the non-coherent scattering functionsRIII andRIV. The appropriate line profile function forRIII is shown to be a simple Voigt function, while forRIV, the line absorption probability distribution function is more complex involving a linear combination of two Voigt functions and another more complex probability distribution. The structure of the reemission coefficients forRIII andRIV is then discussed. Distribution Function Probability Distribution Linear Combination Line Absorption Probability Distribution Function Enthalten in Astrophysics and space science Kluwer Academic Publishers, 1968 106(1984), 2 vom: Nov., Seite 299-307 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:106 year:1984 number:2 month:11 pages:299-307 https://doi.org/10.1007/BF00650357 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_22 GBV_ILN_24 GBV_ILN_31 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2002 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 GBV_ILN_4046 GBV_ILN_4082 GBV_ILN_4103 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4700 AR 106 1984 2 11 299-307 |
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10.1007/BF00650357 doi (DE-627)OLC206615427X (DE-He213)BF00650357-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn McKenna, Sean J. verfasserin aut The angle-dependent redistribution functionsRIII andRIV: Line absorption probability distribution functions and reemission coefficients 1984 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © D. Reidel Publishing Company 1984 Abstract The line absorption probability distribution functions and the reemission coefficients are derived for the non-coherent scattering functionsRIII andRIV. The appropriate line profile function forRIII is shown to be a simple Voigt function, while forRIV, the line absorption probability distribution function is more complex involving a linear combination of two Voigt functions and another more complex probability distribution. The structure of the reemission coefficients forRIII andRIV is then discussed. Distribution Function Probability Distribution Linear Combination Line Absorption Probability Distribution Function Enthalten in Astrophysics and space science Kluwer Academic Publishers, 1968 106(1984), 2 vom: Nov., Seite 299-307 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:106 year:1984 number:2 month:11 pages:299-307 https://doi.org/10.1007/BF00650357 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_22 GBV_ILN_24 GBV_ILN_31 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2002 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 GBV_ILN_4046 GBV_ILN_4082 GBV_ILN_4103 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4700 AR 106 1984 2 11 299-307 |
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the angle-dependent redistribution functionsriii andriv: line absorption probability distribution functions and reemission coefficients |
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The angle-dependent redistribution functionsRIII andRIV: Line absorption probability distribution functions and reemission coefficients |
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Abstract The line absorption probability distribution functions and the reemission coefficients are derived for the non-coherent scattering functionsRIII andRIV. The appropriate line profile function forRIII is shown to be a simple Voigt function, while forRIV, the line absorption probability distribution function is more complex involving a linear combination of two Voigt functions and another more complex probability distribution. The structure of the reemission coefficients forRIII andRIV is then discussed. © D. Reidel Publishing Company 1984 |
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Abstract The line absorption probability distribution functions and the reemission coefficients are derived for the non-coherent scattering functionsRIII andRIV. The appropriate line profile function forRIII is shown to be a simple Voigt function, while forRIV, the line absorption probability distribution function is more complex involving a linear combination of two Voigt functions and another more complex probability distribution. The structure of the reemission coefficients forRIII andRIV is then discussed. © D. Reidel Publishing Company 1984 |
| abstract_unstemmed |
Abstract The line absorption probability distribution functions and the reemission coefficients are derived for the non-coherent scattering functionsRIII andRIV. The appropriate line profile function forRIII is shown to be a simple Voigt function, while forRIV, the line absorption probability distribution function is more complex involving a linear combination of two Voigt functions and another more complex probability distribution. The structure of the reemission coefficients forRIII andRIV is then discussed. © D. Reidel Publishing Company 1984 |
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The angle-dependent redistribution functionsRIII andRIV: Line absorption probability distribution functions and reemission coefficients |
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