The scattering mean free path in the Uranian atmosphere
New measurements of the equivalent widths of the 4-0 S(0) and S(1) H"2 quadrupole lines in the Uranian spectrum have been obtained using high dispersion (4.12 Å/mm) image-tube spectrography. The measured equivalent widths are 62 +/- 19mÅ and 58 +/- 13 mÅ for the S(0) and S(1) lines, respectivel...
Ausführliche Beschreibung
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| Autor*in: |
|---|
| Format: |
E-Artikel |
|---|---|
| Sprache: |
Englisch |
| Erschienen: |
1973 |
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| Reproduktion: |
Elsevier Journal Backfiles on ScienceDirect 1907 - 2002 |
|---|---|
| Übergeordnetes Werk: |
in: Icarus - Amsterdam : Elsevier, 20(1973), 4, Seite 455-464 |
| Übergeordnetes Werk: |
volume:20 ; year:1973 ; number:4 ; pages:455-464 |
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NLEJ180428780 |
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| 520 | |a New measurements of the equivalent widths of the 4-0 S(0) and S(1) H"2 quadrupole lines in the Uranian spectrum have been obtained using high dispersion (4.12 Å/mm) image-tube spectrography. The measured equivalent widths are 62 +/- 19mÅ and 58 +/- 13 mÅ for the S(0) and S(1) lines, respectively. Curve-of-growth analysis in terms of a reflecting layer model yields an H"2 column-density of 780"-"3"3"0^+^9^4^0km amagat and a temperature of 78"-"2"4^+^8^0^oK. Interpretation using a semi-infinite, homogeneous, isotropically scattering model for line formation yields a scattering mean free path at λ6400 Å of 550 +/- 250 km amagat. Quoted errors for both the H"2 column-density and the scattering mean free path include the effect of uncertainty in the choice of atmospheric temperature. The results are discussed in terms of current models for the Uranian atmosphere. | ||
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(DE-627)NLEJ180428780 (DE-599)GBVNLZ180428780 DE-627 ger DE-627 rakwb eng The scattering mean free path in the Uranian atmosphere 1973 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier New measurements of the equivalent widths of the 4-0 S(0) and S(1) H"2 quadrupole lines in the Uranian spectrum have been obtained using high dispersion (4.12 Å/mm) image-tube spectrography. The measured equivalent widths are 62 +/- 19mÅ and 58 +/- 13 mÅ for the S(0) and S(1) lines, respectively. Curve-of-growth analysis in terms of a reflecting layer model yields an H"2 column-density of 780"-"3"3"0^+^9^4^0km amagat and a temperature of 78"-"2"4^+^8^0^oK. Interpretation using a semi-infinite, homogeneous, isotropically scattering model for line formation yields a scattering mean free path at λ6400 Å of 550 +/- 250 km amagat. Quoted errors for both the H"2 column-density and the scattering mean free path include the effect of uncertainty in the choice of atmospheric temperature. The results are discussed in terms of current models for the Uranian atmosphere. Elsevier Journal Backfiles on ScienceDirect 1907 - 2002 Price, M.J. oth in Icarus Amsterdam : Elsevier 20(1973), 4, Seite 455-464 (DE-627)NLEJ176861017 (DE-600)1467991-7 0019-1035 nnns volume:20 year:1973 number:4 pages:455-464 http://linkinghub.elsevier.com/retrieve/pii/0019-1035(73)90018-3 GBV_USEFLAG_H ZDB-1-SDJ GBV_NL_ARTICLE AR 20 1973 4 455-464 |
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(DE-627)NLEJ180428780 (DE-599)GBVNLZ180428780 DE-627 ger DE-627 rakwb eng The scattering mean free path in the Uranian atmosphere 1973 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier New measurements of the equivalent widths of the 4-0 S(0) and S(1) H"2 quadrupole lines in the Uranian spectrum have been obtained using high dispersion (4.12 Å/mm) image-tube spectrography. The measured equivalent widths are 62 +/- 19mÅ and 58 +/- 13 mÅ for the S(0) and S(1) lines, respectively. Curve-of-growth analysis in terms of a reflecting layer model yields an H"2 column-density of 780"-"3"3"0^+^9^4^0km amagat and a temperature of 78"-"2"4^+^8^0^oK. Interpretation using a semi-infinite, homogeneous, isotropically scattering model for line formation yields a scattering mean free path at λ6400 Å of 550 +/- 250 km amagat. Quoted errors for both the H"2 column-density and the scattering mean free path include the effect of uncertainty in the choice of atmospheric temperature. The results are discussed in terms of current models for the Uranian atmosphere. Elsevier Journal Backfiles on ScienceDirect 1907 - 2002 Price, M.J. oth in Icarus Amsterdam : Elsevier 20(1973), 4, Seite 455-464 (DE-627)NLEJ176861017 (DE-600)1467991-7 0019-1035 nnns volume:20 year:1973 number:4 pages:455-464 http://linkinghub.elsevier.com/retrieve/pii/0019-1035(73)90018-3 GBV_USEFLAG_H ZDB-1-SDJ GBV_NL_ARTICLE AR 20 1973 4 455-464 |
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(DE-627)NLEJ180428780 (DE-599)GBVNLZ180428780 DE-627 ger DE-627 rakwb eng The scattering mean free path in the Uranian atmosphere 1973 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier New measurements of the equivalent widths of the 4-0 S(0) and S(1) H"2 quadrupole lines in the Uranian spectrum have been obtained using high dispersion (4.12 Å/mm) image-tube spectrography. The measured equivalent widths are 62 +/- 19mÅ and 58 +/- 13 mÅ for the S(0) and S(1) lines, respectively. Curve-of-growth analysis in terms of a reflecting layer model yields an H"2 column-density of 780"-"3"3"0^+^9^4^0km amagat and a temperature of 78"-"2"4^+^8^0^oK. Interpretation using a semi-infinite, homogeneous, isotropically scattering model for line formation yields a scattering mean free path at λ6400 Å of 550 +/- 250 km amagat. Quoted errors for both the H"2 column-density and the scattering mean free path include the effect of uncertainty in the choice of atmospheric temperature. The results are discussed in terms of current models for the Uranian atmosphere. Elsevier Journal Backfiles on ScienceDirect 1907 - 2002 Price, M.J. oth in Icarus Amsterdam : Elsevier 20(1973), 4, Seite 455-464 (DE-627)NLEJ176861017 (DE-600)1467991-7 0019-1035 nnns volume:20 year:1973 number:4 pages:455-464 http://linkinghub.elsevier.com/retrieve/pii/0019-1035(73)90018-3 GBV_USEFLAG_H ZDB-1-SDJ GBV_NL_ARTICLE AR 20 1973 4 455-464 |
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(DE-627)NLEJ180428780 (DE-599)GBVNLZ180428780 DE-627 ger DE-627 rakwb eng The scattering mean free path in the Uranian atmosphere 1973 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier New measurements of the equivalent widths of the 4-0 S(0) and S(1) H"2 quadrupole lines in the Uranian spectrum have been obtained using high dispersion (4.12 Å/mm) image-tube spectrography. The measured equivalent widths are 62 +/- 19mÅ and 58 +/- 13 mÅ for the S(0) and S(1) lines, respectively. Curve-of-growth analysis in terms of a reflecting layer model yields an H"2 column-density of 780"-"3"3"0^+^9^4^0km amagat and a temperature of 78"-"2"4^+^8^0^oK. Interpretation using a semi-infinite, homogeneous, isotropically scattering model for line formation yields a scattering mean free path at λ6400 Å of 550 +/- 250 km amagat. Quoted errors for both the H"2 column-density and the scattering mean free path include the effect of uncertainty in the choice of atmospheric temperature. The results are discussed in terms of current models for the Uranian atmosphere. Elsevier Journal Backfiles on ScienceDirect 1907 - 2002 Price, M.J. oth in Icarus Amsterdam : Elsevier 20(1973), 4, Seite 455-464 (DE-627)NLEJ176861017 (DE-600)1467991-7 0019-1035 nnns volume:20 year:1973 number:4 pages:455-464 http://linkinghub.elsevier.com/retrieve/pii/0019-1035(73)90018-3 GBV_USEFLAG_H ZDB-1-SDJ GBV_NL_ARTICLE AR 20 1973 4 455-464 |
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(DE-627)NLEJ180428780 (DE-599)GBVNLZ180428780 DE-627 ger DE-627 rakwb eng The scattering mean free path in the Uranian atmosphere 1973 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier New measurements of the equivalent widths of the 4-0 S(0) and S(1) H"2 quadrupole lines in the Uranian spectrum have been obtained using high dispersion (4.12 Å/mm) image-tube spectrography. The measured equivalent widths are 62 +/- 19mÅ and 58 +/- 13 mÅ for the S(0) and S(1) lines, respectively. Curve-of-growth analysis in terms of a reflecting layer model yields an H"2 column-density of 780"-"3"3"0^+^9^4^0km amagat and a temperature of 78"-"2"4^+^8^0^oK. Interpretation using a semi-infinite, homogeneous, isotropically scattering model for line formation yields a scattering mean free path at λ6400 Å of 550 +/- 250 km amagat. Quoted errors for both the H"2 column-density and the scattering mean free path include the effect of uncertainty in the choice of atmospheric temperature. The results are discussed in terms of current models for the Uranian atmosphere. Elsevier Journal Backfiles on ScienceDirect 1907 - 2002 Price, M.J. oth in Icarus Amsterdam : Elsevier 20(1973), 4, Seite 455-464 (DE-627)NLEJ176861017 (DE-600)1467991-7 0019-1035 nnns volume:20 year:1973 number:4 pages:455-464 http://linkinghub.elsevier.com/retrieve/pii/0019-1035(73)90018-3 GBV_USEFLAG_H ZDB-1-SDJ GBV_NL_ARTICLE AR 20 1973 4 455-464 |
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New measurements of the equivalent widths of the 4-0 S(0) and S(1) H"2 quadrupole lines in the Uranian spectrum have been obtained using high dispersion (4.12 Å/mm) image-tube spectrography. The measured equivalent widths are 62 +/- 19mÅ and 58 +/- 13 mÅ for the S(0) and S(1) lines, respectively. Curve-of-growth analysis in terms of a reflecting layer model yields an H"2 column-density of 780"-"3"3"0^+^9^4^0km amagat and a temperature of 78"-"2"4^+^8^0^oK. Interpretation using a semi-infinite, homogeneous, isotropically scattering model for line formation yields a scattering mean free path at λ6400 Å of 550 +/- 250 km amagat. Quoted errors for both the H"2 column-density and the scattering mean free path include the effect of uncertainty in the choice of atmospheric temperature. The results are discussed in terms of current models for the Uranian atmosphere. |
| abstractGer |
New measurements of the equivalent widths of the 4-0 S(0) and S(1) H"2 quadrupole lines in the Uranian spectrum have been obtained using high dispersion (4.12 Å/mm) image-tube spectrography. The measured equivalent widths are 62 +/- 19mÅ and 58 +/- 13 mÅ for the S(0) and S(1) lines, respectively. Curve-of-growth analysis in terms of a reflecting layer model yields an H"2 column-density of 780"-"3"3"0^+^9^4^0km amagat and a temperature of 78"-"2"4^+^8^0^oK. Interpretation using a semi-infinite, homogeneous, isotropically scattering model for line formation yields a scattering mean free path at λ6400 Å of 550 +/- 250 km amagat. Quoted errors for both the H"2 column-density and the scattering mean free path include the effect of uncertainty in the choice of atmospheric temperature. The results are discussed in terms of current models for the Uranian atmosphere. |
| abstract_unstemmed |
New measurements of the equivalent widths of the 4-0 S(0) and S(1) H"2 quadrupole lines in the Uranian spectrum have been obtained using high dispersion (4.12 Å/mm) image-tube spectrography. The measured equivalent widths are 62 +/- 19mÅ and 58 +/- 13 mÅ for the S(0) and S(1) lines, respectively. Curve-of-growth analysis in terms of a reflecting layer model yields an H"2 column-density of 780"-"3"3"0^+^9^4^0km amagat and a temperature of 78"-"2"4^+^8^0^oK. Interpretation using a semi-infinite, homogeneous, isotropically scattering model for line formation yields a scattering mean free path at λ6400 Å of 550 +/- 250 km amagat. Quoted errors for both the H"2 column-density and the scattering mean free path include the effect of uncertainty in the choice of atmospheric temperature. The results are discussed in terms of current models for the Uranian atmosphere. |
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