Please use this identifier to cite or link to this item: http://hdl.handle.net/10603/529899
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dc.coverage.spatial
dc.date.accessioned2023-12-16T06:43:00Z-
dc.date.available2023-12-16T06:43:00Z-
dc.identifier.urihttp://hdl.handle.net/10603/529899-
dc.description.abstractnewline No
dc.format.extentxx, 203p
dc.languageEnglish
dc.relation
dc.rightsuniversity
dc.titleThe chemical composition of the primary cosmic ray nuclei of change Z greater than equal to 3
dc.title.alternative
dc.creator.researcherDurgaprasad, N
dc.subject.keywordCalibration
dc.subject.keywordChemistry
dc.subject.keywordChemistry Physical
dc.subject.keywordCosmic Ray
dc.subject.keywordFragmentation
dc.subject.keywordNuclei
dc.subject.keywordPhysical Sciences
dc.subject.keywordTexas Stacks
dc.description.note
dc.contributor.guideDaniel, R R
dc.publisher.placeMumbai
dc.publisher.universityUniversity of Mumbai
dc.publisher.institutionChemistry, Tata Institute of Fundamental Research
dc.date.registered
dc.date.completed1964
dc.date.awarded
dc.format.dimensions
dc.format.accompanyingmaterialDVD
dc.source.universityUniversity
dc.type.degreePh.D.
Appears in Departments:Chemistry, Tata Institute of Fundamental Research

Files in This Item:
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01_title.pdfAttached File236.13 kBAdobe PDFView/Open
02_prelim pages.pdf4.75 MBAdobe PDFView/Open
03_contents.pdf1.22 MBAdobe PDFView/Open
04_chapter 1.pdf4.45 MBAdobe PDFView/Open
05_chapter 2.pdf15.25 MBAdobe PDFView/Open
06_chapter 3.pdf5.65 MBAdobe PDFView/Open
07_chapter 4.pdf8.26 MBAdobe PDFView/Open
08_chapter 5.pdf12.88 MBAdobe PDFView/Open
09_chapter 6.pdf5.34 MBAdobe PDFView/Open
10_chapter 7.pdf9.67 MBAdobe PDFView/Open
11_annexures.pdf13.68 MBAdobe PDFView/Open
80_recommendation.pdf9.9 MBAdobe PDFView/Open


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