Infrared thermal models for Saturn's ring
Infrared (10 and 20 μm) thermal emission data for Saturn's rings are discussed in terms of simple isothermal radiative transfer models of finite optical thickness. Recent brightness temperature measurements, corresponding to essentially maximum ring tilt, indicate that optical single scattering...
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| Autor*in: |
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| Format: |
E-Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
1976 |
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| Reproduktion: |
Elsevier Journal Backfiles on ScienceDirect 1907 - 2002 |
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| Übergeordnetes Werk: |
in: Icarus - Amsterdam : Elsevier, 27(1976), 4, Seite 537-544 |
| Übergeordnetes Werk: |
volume:27 ; year:1976 ; number:4 ; pages:537-544 |
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| 520 | |a Infrared (10 and 20 μm) thermal emission data for Saturn's rings are discussed in terms of simple isothermal radiative transfer models of finite optical thickness. Recent brightness temperature measurements, corresponding to essentially maximum ring tilt, indicate that optical single scattering albedos less than 0.75 are required to provide sufficient heating of the ring material. Reconciliation with analyses of the optical scattering properties of the ring requires the back-scattering efficiency to be even higher than for a macroscopic sphere. Historical brightness temperature measurements are used to show that no unique isothermal ring model exists. Instead, a temperature gradient perpendicular to the ring plane appears to be present. | ||
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(DE-627)NLEJ180400169 (DE-599)GBVNLZ180400169 DE-627 ger DE-627 rakwb eng Infrared thermal models for Saturn's ring 1976 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier Infrared (10 and 20 μm) thermal emission data for Saturn's rings are discussed in terms of simple isothermal radiative transfer models of finite optical thickness. Recent brightness temperature measurements, corresponding to essentially maximum ring tilt, indicate that optical single scattering albedos less than 0.75 are required to provide sufficient heating of the ring material. Reconciliation with analyses of the optical scattering properties of the ring requires the back-scattering efficiency to be even higher than for a macroscopic sphere. Historical brightness temperature measurements are used to show that no unique isothermal ring model exists. Instead, a temperature gradient perpendicular to the ring plane appears to be present. Elsevier Journal Backfiles on ScienceDirect 1907 - 2002 Price, M.J. oth in Icarus Amsterdam : Elsevier 27(1976), 4, Seite 537-544 (DE-627)NLEJ176861017 (DE-600)1467991-7 0019-1035 nnns volume:27 year:1976 number:4 pages:537-544 http://dx.doi.org/10.1016/0019-1035(76)90169-X GBV_USEFLAG_H ZDB-1-SDJ GBV_NL_ARTICLE AR 27 1976 4 537-544 |
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(DE-627)NLEJ180400169 (DE-599)GBVNLZ180400169 DE-627 ger DE-627 rakwb eng Infrared thermal models for Saturn's ring 1976 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier Infrared (10 and 20 μm) thermal emission data for Saturn's rings are discussed in terms of simple isothermal radiative transfer models of finite optical thickness. Recent brightness temperature measurements, corresponding to essentially maximum ring tilt, indicate that optical single scattering albedos less than 0.75 are required to provide sufficient heating of the ring material. Reconciliation with analyses of the optical scattering properties of the ring requires the back-scattering efficiency to be even higher than for a macroscopic sphere. Historical brightness temperature measurements are used to show that no unique isothermal ring model exists. Instead, a temperature gradient perpendicular to the ring plane appears to be present. Elsevier Journal Backfiles on ScienceDirect 1907 - 2002 Price, M.J. oth in Icarus Amsterdam : Elsevier 27(1976), 4, Seite 537-544 (DE-627)NLEJ176861017 (DE-600)1467991-7 0019-1035 nnns volume:27 year:1976 number:4 pages:537-544 http://dx.doi.org/10.1016/0019-1035(76)90169-X GBV_USEFLAG_H ZDB-1-SDJ GBV_NL_ARTICLE AR 27 1976 4 537-544 |
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(DE-627)NLEJ180400169 (DE-599)GBVNLZ180400169 DE-627 ger DE-627 rakwb eng Infrared thermal models for Saturn's ring 1976 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier Infrared (10 and 20 μm) thermal emission data for Saturn's rings are discussed in terms of simple isothermal radiative transfer models of finite optical thickness. Recent brightness temperature measurements, corresponding to essentially maximum ring tilt, indicate that optical single scattering albedos less than 0.75 are required to provide sufficient heating of the ring material. Reconciliation with analyses of the optical scattering properties of the ring requires the back-scattering efficiency to be even higher than for a macroscopic sphere. Historical brightness temperature measurements are used to show that no unique isothermal ring model exists. Instead, a temperature gradient perpendicular to the ring plane appears to be present. Elsevier Journal Backfiles on ScienceDirect 1907 - 2002 Price, M.J. oth in Icarus Amsterdam : Elsevier 27(1976), 4, Seite 537-544 (DE-627)NLEJ176861017 (DE-600)1467991-7 0019-1035 nnns volume:27 year:1976 number:4 pages:537-544 http://dx.doi.org/10.1016/0019-1035(76)90169-X GBV_USEFLAG_H ZDB-1-SDJ GBV_NL_ARTICLE AR 27 1976 4 537-544 |
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(DE-627)NLEJ180400169 (DE-599)GBVNLZ180400169 DE-627 ger DE-627 rakwb eng Infrared thermal models for Saturn's ring 1976 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier Infrared (10 and 20 μm) thermal emission data for Saturn's rings are discussed in terms of simple isothermal radiative transfer models of finite optical thickness. Recent brightness temperature measurements, corresponding to essentially maximum ring tilt, indicate that optical single scattering albedos less than 0.75 are required to provide sufficient heating of the ring material. Reconciliation with analyses of the optical scattering properties of the ring requires the back-scattering efficiency to be even higher than for a macroscopic sphere. Historical brightness temperature measurements are used to show that no unique isothermal ring model exists. Instead, a temperature gradient perpendicular to the ring plane appears to be present. Elsevier Journal Backfiles on ScienceDirect 1907 - 2002 Price, M.J. oth in Icarus Amsterdam : Elsevier 27(1976), 4, Seite 537-544 (DE-627)NLEJ176861017 (DE-600)1467991-7 0019-1035 nnns volume:27 year:1976 number:4 pages:537-544 http://dx.doi.org/10.1016/0019-1035(76)90169-X GBV_USEFLAG_H ZDB-1-SDJ GBV_NL_ARTICLE AR 27 1976 4 537-544 |
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(DE-627)NLEJ180400169 (DE-599)GBVNLZ180400169 DE-627 ger DE-627 rakwb eng Infrared thermal models for Saturn's ring 1976 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier Infrared (10 and 20 μm) thermal emission data for Saturn's rings are discussed in terms of simple isothermal radiative transfer models of finite optical thickness. Recent brightness temperature measurements, corresponding to essentially maximum ring tilt, indicate that optical single scattering albedos less than 0.75 are required to provide sufficient heating of the ring material. Reconciliation with analyses of the optical scattering properties of the ring requires the back-scattering efficiency to be even higher than for a macroscopic sphere. Historical brightness temperature measurements are used to show that no unique isothermal ring model exists. Instead, a temperature gradient perpendicular to the ring plane appears to be present. Elsevier Journal Backfiles on ScienceDirect 1907 - 2002 Price, M.J. oth in Icarus Amsterdam : Elsevier 27(1976), 4, Seite 537-544 (DE-627)NLEJ176861017 (DE-600)1467991-7 0019-1035 nnns volume:27 year:1976 number:4 pages:537-544 http://dx.doi.org/10.1016/0019-1035(76)90169-X GBV_USEFLAG_H ZDB-1-SDJ GBV_NL_ARTICLE AR 27 1976 4 537-544 |
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Infrared thermal models for Saturn's ring |
| abstract |
Infrared (10 and 20 μm) thermal emission data for Saturn's rings are discussed in terms of simple isothermal radiative transfer models of finite optical thickness. Recent brightness temperature measurements, corresponding to essentially maximum ring tilt, indicate that optical single scattering albedos less than 0.75 are required to provide sufficient heating of the ring material. Reconciliation with analyses of the optical scattering properties of the ring requires the back-scattering efficiency to be even higher than for a macroscopic sphere. Historical brightness temperature measurements are used to show that no unique isothermal ring model exists. Instead, a temperature gradient perpendicular to the ring plane appears to be present. |
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Infrared (10 and 20 μm) thermal emission data for Saturn's rings are discussed in terms of simple isothermal radiative transfer models of finite optical thickness. Recent brightness temperature measurements, corresponding to essentially maximum ring tilt, indicate that optical single scattering albedos less than 0.75 are required to provide sufficient heating of the ring material. Reconciliation with analyses of the optical scattering properties of the ring requires the back-scattering efficiency to be even higher than for a macroscopic sphere. Historical brightness temperature measurements are used to show that no unique isothermal ring model exists. Instead, a temperature gradient perpendicular to the ring plane appears to be present. |
| abstract_unstemmed |
Infrared (10 and 20 μm) thermal emission data for Saturn's rings are discussed in terms of simple isothermal radiative transfer models of finite optical thickness. Recent brightness temperature measurements, corresponding to essentially maximum ring tilt, indicate that optical single scattering albedos less than 0.75 are required to provide sufficient heating of the ring material. Reconciliation with analyses of the optical scattering properties of the ring requires the back-scattering efficiency to be even higher than for a macroscopic sphere. Historical brightness temperature measurements are used to show that no unique isothermal ring model exists. Instead, a temperature gradient perpendicular to the ring plane appears to be present. |
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