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dc.contributor.advisorVictor P. Starr.en_US
dc.contributor.authorGilman, Peter A. (Peter Augustus)en_US
dc.date.accessioned2011-11-18T20:48:07Z
dc.date.available2011-11-18T20:48:07Z
dc.date.issued1966en_US
dc.identifier.urihttp://hdl.handle.net/1721.1/67115
dc.descriptionMassachusetts Institute of Technology. Dept. of Meteorology. Thesis. 1966. Ph.D.en_US
dc.descriptionBibliography: p. 197-202.en_US
dc.format.extent[11], 212 p.en_US
dc.language.isoengen_US
dc.publisherMassachusetts Institute of Technologyen_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.titleHydromagnetic model for the solar general circulation.en_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.oclc25776427en_US


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