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Vertical Scales of Turbulence at the Mt. Wilson Observatory

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dc.contributor.author Treuhaft, Robert N. en_US
dc.date.accessioned 2004-10-03T03:38:18Z
dc.date.available 2004-10-03T03:38:18Z
dc.date.issued 1995
dc.identifier.citation Astrophysical Journal en_US
dc.identifier.clearanceno 95-0733
dc.identifier.uri http://hdl.handle.net/2014/30868
dc.description.abstract The vertical scales of turbulence at the Mt. Wilson observatory are inferred from data from the University of California at Berkeley Infrared Spatial Interferometer (ISI), by modeling path length fluctuations observed in the interferometric paths to celestial objects and those in instrumental ground- based paths. The correlations between the stellar and ground-based path length fluctuations and the temporal statistic of those fluctuations are modeled on various time scales to constrain the vertical scales. en_US
dc.format.extent 417579 bytes
dc.format.mimetype application/pdf
dc.language.iso en_US
dc.subject.other Mt. Wilson Observatory en_US
dc.title Vertical Scales of Turbulence at the Mt. Wilson Observatory en_US


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