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dc.contributor.authorVan Hemelrijck, E.
dc.date1988
dc.date.accessioned2017-06-08T12:20:54Z
dc.date.available2017-06-08T12:20:54Z
dc.identifier.urihttps://orfeo.belnet.be/handle/internal/5770
dc.descriptionThe latitudinal and seasonal variation of the direct solar radiation incident at the top of the atmosphere of Uranus and Neptune has been recalculated by use of updated values for the period of axial rotation and the oblateness. Values for the solar radiation are given in Watt per square meter instead of the unit used in earlier papers (calories per square centimeter per planetary day). The solar radiation averaged over a season and a year as a function of planetocentric latitude has also been reviewed. In addition, attention is made to the ratio of the solar radiation incident on an oblate planet to that incident on a spherical planet.
dc.languageeng
dc.titleThe solar radiation incident at the top of the atmospheres of Uranus and Neptune
dc.typeArticle
dc.subject.frascatiPhysical sciences
dc.audienceScientific
dc.source.titleEarth, Moon and Planets
dc.source.volume40
dc.source.issue2
dc.source.page149-164
Orfeo.peerreviewedYes
dc.identifier.doi10.1007/BF00056022
dc.identifier.scopus2-s2.0-34250096481


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