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dc.contributor.advisorPeter H. Stone.en_US
dc.contributor.authorLin, Charles Augustinen_US
dc.date.accessioned2010-04-28T15:08:08Z
dc.date.available2010-04-28T15:08:08Z
dc.date.issued1979en_US
dc.identifier.urihttp://hdl.handle.net/1721.1/54267
dc.descriptionThesis (Ph.D.)--Massachusetts Institute of Technology, Dept. of Meteorology, 1979.en_US
dc.descriptionMicrofiche copy available in Archives and Science.en_US
dc.descriptionVita.en_US
dc.descriptionBibliography: leaves 143-146.en_US
dc.description.statementofresponsibilityby Charles Augustin Lin.en_US
dc.format.extent147 leavesen_US
dc.language.isoengen_US
dc.publisherMassachusetts Institute of Technologyen_US
dc.relation.ispartofseriesMassachusetts Institute of Technology. Dept. of Meteorology.en_US
dc.rightsM.I.T. theses are protected by copyright. They may be viewed from this source for any purpose, but reproduction or distribution in any format is prohibited without written permission. See provided URL for inquiries about permission.en_US
dc.rights.urihttp://dspace.mit.edu/handle/1721.1/7582en_US
dc.subjectMeteorologyen_US
dc.subject.lcshRossby waves Mathematical modelsen_US
dc.subject.lcshEddy fluxen_US
dc.subject.lcshBaroclinicityen_US
dc.subject.lcshHeat budget (Geophysics)en_US
dc.titleEddy heat fluxes and stability of planetary wavesen_US
dc.typeThesisen_US
dc.description.degreePh.D.en_US
dc.contributor.departmentMassachusetts Institute of Technology. Department of Meteorologyen_US
dc.contributor.departmentMassachusetts Institute of Technology. Department of Earth, Atmospheric, and Planetary Sciences
dc.identifier.oclc07239724en_US


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