1. Shodhganga@INFLIBNET
  2. University of Mumbai
  3. Physics, Tata Institute of Fundamental Research
Please use this identifier to cite or link to this item: http://hdl.handle.net/10603/506625
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DC FieldValueLanguage
dc.coverage.spatial
dc.date.accessioned2023-08-11T04:50:33Z-
dc.date.available2023-08-11T04:50:33Z-
dc.identifier.urihttp://hdl.handle.net/10603/506625-
dc.description.abstractnewline No
dc.format.extentxii, 136p
dc.languageEnglish
dc.relation
dc.rightsuniversity
dc.titleAn optimum deconvolution method for lunar occulations and commological studies using angular sizes of radio sources
dc.title.alternative
dc.creator.researcherSubrahmanya, C R
dc.subject.keywordAngular Sizes
dc.subject.keywordCosmology
dc.subject.keywordLunar Occulations
dc.subject.keywordPhysical Sciences
dc.subject.keywordPhysics
dc.subject.keywordPhysics Particles and Fields
dc.subject.keywordRadio Sources
dc.description.note
dc.contributor.guideSwarup, Govind
dc.publisher.placeMumbai
dc.publisher.universityUniversity of Mumbai
dc.publisher.institutionPhysics, Tata Institute of Fundamental Research
dc.date.registered
dc.date.completed1977
dc.date.awarded
dc.format.dimensions
dc.format.accompanyingmaterialDVD
dc.source.universityUniversity
dc.type.degreePh.D.
Appears in Departments:Physics, Tata Institute of Fundamental Research

Files in This Item:
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01_title.pdfAttached File284.22 kBAdobe PDFView/Open
02_prelim pages.pdf1.46 MBAdobe PDFView/Open
03_contents.pdf1.87 MBAdobe PDFView/Open
04_chapter 1.pdf10.81 MBAdobe PDFView/Open
05_chapter 2.pdf8.58 MBAdobe PDFView/Open
06_chapter 3.pdf21.46 MBAdobe PDFView/Open
07_chapter 4.pdf18.9 MBAdobe PDFView/Open
08_chapter 5.pdf2.8 MBAdobe PDFView/Open
09_annexures.pdf2.16 MBAdobe PDFView/Open
80_recommendation.pdf3.08 MBAdobe PDFView/Open
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