Variations in the 13 cm opacity below the main cloud layer in the atmosphere of Venus inferred from Pioneer-Venus radio occultation studies 1978-1987
dc.contributor.author | Jenkins, Jon Michael | en_US |
dc.date.accessioned | 2007-06-22T11:34:15Z | |
dc.date.available | 2007-06-22T11:34:15Z | |
dc.date.issued | 1992-05 | en_US |
dc.identifier.uri | http://hdl.handle.net/1853/14843 | |
dc.publisher | Georgia Institute of Technology | en_US |
dc.rights | Access restricted to authorized Georgia Tech users only. | en_US |
dc.subject.lcsh | Venus (Planet) Atmosphere | en_US |
dc.subject.lcsh | Planets Atmospheres | en_US |
dc.subject.lcsh | Solar radio emission | en_US |
dc.title | Variations in the 13 cm opacity below the main cloud layer in the atmosphere of Venus inferred from Pioneer-Venus radio occultation studies 1978-1987 | en_US |
dc.type | Dissertation | en_US |
dc.description.degree | Ph.D. | en_US |
dc.contributor.department | Electric engineering | en_US |
dc.description.advisor | Paul G. Steffes | en_US |
dc.identifier.bibid | 353658 | en_US |
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Original work by students in the School of Electrical and Computer Engineering