Observation of the 7320A O=(2P) Airglow Emission at Twilight

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dc.contributor.advisorWright, Wayne M., 1934-
dc.contributor.advisorSharp, William E.
dc.contributor.authorGoodwin, Robert W.
dc.date.accessioned2011-09-01T19:49:22Z
dc.date.available2011-09-01T19:49:22Z
dc.date.issued1987
dc.descriptionvi, 46 p.en_US
dc.description.abstractThis paper discusses the method of obtaining an altitude profile for atomic oxygen in the upper atmosphere by observing the sunlight-stimulated 7320A airglow emission of the 0+(2p) ion (whose abundance is directly proportional to that of 0) while the earth's shadow provides a natural "scan" of the atmosphere during twilight. Background on the emission and experiment is presented along with a detailed description of the instrument, data gathering procedure and analysis.en_US
dc.description.sponsorshipPhysics Research Laboratory. University of Michigan. Ann Arbor, Michigan.
dc.format.mimetypeapplication/pdf
dc.identifier.urihttp://hdl.handle.net/10920/23362
dc.language.isoen_USen_US
dc.relation.ispartofKalamazoo College Physics Senior Individualized Projects Collection
dc.relation.ispartofseriesSenior Individualized Projects. Physics.;
dc.rightsU.S. copyright laws protect this material. Commercial use or distribution of this material is not permitted without prior written permission of the copyright holder. All rights reserved.
dc.titleObservation of the 7320A O=(2P) Airglow Emission at Twilighten_US
dc.typeThesisen_US
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