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Please use this identifier to cite or link to this item: https://doi.org/10.1007/BF00928371
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dc.titleLight scattering by an inhomogeneous spherically symmetric cometary atmosphere: Solar flux impinging on the nucleus head
dc.contributor.authorWilson, S.J.
dc.contributor.authorWan, F.S.
dc.date.accessioned2014-10-28T02:37:52Z
dc.date.available2014-10-28T02:37:52Z
dc.date.issued1983-08
dc.identifier.citationWilson, S.J., Wan, F.S. (1983-08). Light scattering by an inhomogeneous spherically symmetric cometary atmosphere: Solar flux impinging on the nucleus head. The Moon and the Planets 29 (1) : 1-6. ScholarBank@NUS Repository. https://doi.org/10.1007/BF00928371
dc.identifier.issn01650807
dc.identifier.urihttp://scholarbank.nus.edu.sg/handle/10635/103489
dc.description.abstractThe generalized Eddington approximation, obtained by the three-stream division of the radiation field, is used to compute the intensity falling on the nucleus head of a spherically-symmetric comet illuminated by parallel solar radiation. © 1983 D. Reidel Publishing Company.
dc.description.urihttp://libproxy1.nus.edu.sg/login?url=http://dx.doi.org/10.1007/BF00928371
dc.sourceScopus
dc.typeArticle
dc.contributor.departmentMATHEMATICS
dc.description.doi10.1007/BF00928371
dc.description.sourcetitleThe Moon and the Planets
dc.description.volume29
dc.description.issue1
dc.description.page1-6
dc.identifier.isiutA1983RK30500001
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