Radiation Balance of Jupiter and Saturn
[Auszug] Trafton3 has pointed out that the pressure-induced dipole absorption of H2 may produce significant absorption in the case of Jupiter. He finds that temperatures of the order of 147 K are not difficult to maintain by an atmospheric greenhouse effect depending only on this absorber. Owen4 has...
Ausführliche Beschreibung
Autor*in: |
OWEN, TOBIAS [verfasserIn] WALSH, THOMAS E. [verfasserIn] |
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Format: |
E-Artikel |
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Sprache: |
Englisch |
Erschienen: |
s.l.: Nature Publishing Group ; 1965 |
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Umfang: |
2 |
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Reproduktion: |
Nature Archives 1869 - 2009 |
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Übergeordnetes Werk: |
In: Nature |
Übergeordnetes Werk: |
volume:208 ; year:1965 ; number:5009 ; month:03 ; pages:476-477 ; extent:2 |
Links: |
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DOI / URN: |
10.1038/208476b0 |
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10.1038/208476b0 doi (DE-627)NLEJ234544988 DE-627 ger DE-627 rakwb eng OWEN, TOBIAS verfasserin aut Radiation Balance of Jupiter and Saturn [s.l.] Nature Publishing Group 1965 2 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier [Auszug] Trafton3 has pointed out that the pressure-induced dipole absorption of H2 may produce significant absorption in the case of Jupiter. He finds that temperatures of the order of 147 K are not difficult to maintain by an atmospheric greenhouse effect depending only on this absorber. Owen4 has ... Nature Archives 1869 - 2009 WALSH, THOMAS E. verfasserin aut In Nature <London> London [u.a.] : Nature Publising Group, 1869 208(1965), 5009 vom: März, Seite 476-477 (DE-627)NLEJ227682335 (DE-600)1413423-8 1476-4687 nnns volume:208 year:1965 number:5009 month:03 pages:476-477 extent:2 http://dx.doi.org/10.1038/208476b0 application/pdf Deutschlandweit zugänglich GBV_USEFLAG_U ZDB-1-NTA GBV_NL_ARTICLE AR 208 1965 5009 3 476-477 2 |
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10.1038/208476b0 doi (DE-627)NLEJ234544988 DE-627 ger DE-627 rakwb eng OWEN, TOBIAS verfasserin aut Radiation Balance of Jupiter and Saturn [s.l.] Nature Publishing Group 1965 2 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier [Auszug] Trafton3 has pointed out that the pressure-induced dipole absorption of H2 may produce significant absorption in the case of Jupiter. He finds that temperatures of the order of 147 K are not difficult to maintain by an atmospheric greenhouse effect depending only on this absorber. Owen4 has ... Nature Archives 1869 - 2009 WALSH, THOMAS E. verfasserin aut In Nature <London> London [u.a.] : Nature Publising Group, 1869 208(1965), 5009 vom: März, Seite 476-477 (DE-627)NLEJ227682335 (DE-600)1413423-8 1476-4687 nnns volume:208 year:1965 number:5009 month:03 pages:476-477 extent:2 http://dx.doi.org/10.1038/208476b0 application/pdf Deutschlandweit zugänglich GBV_USEFLAG_U ZDB-1-NTA GBV_NL_ARTICLE AR 208 1965 5009 3 476-477 2 |
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10.1038/208476b0 doi (DE-627)NLEJ234544988 DE-627 ger DE-627 rakwb eng OWEN, TOBIAS verfasserin aut Radiation Balance of Jupiter and Saturn [s.l.] Nature Publishing Group 1965 2 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier [Auszug] Trafton3 has pointed out that the pressure-induced dipole absorption of H2 may produce significant absorption in the case of Jupiter. He finds that temperatures of the order of 147 K are not difficult to maintain by an atmospheric greenhouse effect depending only on this absorber. Owen4 has ... Nature Archives 1869 - 2009 WALSH, THOMAS E. verfasserin aut In Nature <London> London [u.a.] : Nature Publising Group, 1869 208(1965), 5009 vom: März, Seite 476-477 (DE-627)NLEJ227682335 (DE-600)1413423-8 1476-4687 nnns volume:208 year:1965 number:5009 month:03 pages:476-477 extent:2 http://dx.doi.org/10.1038/208476b0 application/pdf Deutschlandweit zugänglich GBV_USEFLAG_U ZDB-1-NTA GBV_NL_ARTICLE AR 208 1965 5009 3 476-477 2 |
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10.1038/208476b0 doi (DE-627)NLEJ234544988 DE-627 ger DE-627 rakwb eng OWEN, TOBIAS verfasserin aut Radiation Balance of Jupiter and Saturn [s.l.] Nature Publishing Group 1965 2 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier [Auszug] Trafton3 has pointed out that the pressure-induced dipole absorption of H2 may produce significant absorption in the case of Jupiter. He finds that temperatures of the order of 147 K are not difficult to maintain by an atmospheric greenhouse effect depending only on this absorber. Owen4 has ... Nature Archives 1869 - 2009 WALSH, THOMAS E. verfasserin aut In Nature <London> London [u.a.] : Nature Publising Group, 1869 208(1965), 5009 vom: März, Seite 476-477 (DE-627)NLEJ227682335 (DE-600)1413423-8 1476-4687 nnns volume:208 year:1965 number:5009 month:03 pages:476-477 extent:2 http://dx.doi.org/10.1038/208476b0 application/pdf Deutschlandweit zugänglich GBV_USEFLAG_U ZDB-1-NTA GBV_NL_ARTICLE AR 208 1965 5009 3 476-477 2 |
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10.1038/208476b0 doi (DE-627)NLEJ234544988 DE-627 ger DE-627 rakwb eng OWEN, TOBIAS verfasserin aut Radiation Balance of Jupiter and Saturn [s.l.] Nature Publishing Group 1965 2 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier [Auszug] Trafton3 has pointed out that the pressure-induced dipole absorption of H2 may produce significant absorption in the case of Jupiter. He finds that temperatures of the order of 147 K are not difficult to maintain by an atmospheric greenhouse effect depending only on this absorber. Owen4 has ... Nature Archives 1869 - 2009 WALSH, THOMAS E. verfasserin aut In Nature <London> London [u.a.] : Nature Publising Group, 1869 208(1965), 5009 vom: März, Seite 476-477 (DE-627)NLEJ227682335 (DE-600)1413423-8 1476-4687 nnns volume:208 year:1965 number:5009 month:03 pages:476-477 extent:2 http://dx.doi.org/10.1038/208476b0 application/pdf Deutschlandweit zugänglich GBV_USEFLAG_U ZDB-1-NTA GBV_NL_ARTICLE AR 208 1965 5009 3 476-477 2 |
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[Auszug] Trafton3 has pointed out that the pressure-induced dipole absorption of H2 may produce significant absorption in the case of Jupiter. He finds that temperatures of the order of 147 K are not difficult to maintain by an atmospheric greenhouse effect depending only on this absorber. Owen4 has ... |
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[Auszug] Trafton3 has pointed out that the pressure-induced dipole absorption of H2 may produce significant absorption in the case of Jupiter. He finds that temperatures of the order of 147 K are not difficult to maintain by an atmospheric greenhouse effect depending only on this absorber. Owen4 has ... |
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