Short-term Variability of Atmospheric Extinction During the Night, Under Clear-Sky Conditions, Investigated by Broadband Stellar Photometry

dc.contributor.advisorEllingson, Robert G.en_US
dc.contributor.authorMusat, Ileana Cristinaen_US
dc.contributor.departmentMeteorologyen_US
dc.contributor.publisherDigital Repository at the University of Marylanden_US
dc.contributor.publisherUniversity of Maryland (College Park, Md.)en_US
dc.date.accessioned2004-10-09T05:21:17Z
dc.date.available2004-10-09T05:21:17Z
dc.date.issued2004-09-02en_US
dc.description.abstractThis is a study about the possibility of determining the aerosol optical depth by using star broadband observations from a whole sky imager. The main difficulty in such measurements consists of accurately separating the star flux value from the non-stellar diffuse light, which is overwhelmingly present in the whole sky imagery. A correction method to solve this problem is found and the monochromatic extinction at the ground due to aerosols is extracted from heterochromatic measurements. A form of closure is achieved by comparison with simultaneous or temporally close measurements with other instruments. The accuracy and precision of the method are assessed: the total error is a combination of random error of measurements and systematic error of calibration and model and is between 2.6 and 3% rms.en_US
dc.format.extent6111620 bytes
dc.format.mimetypeapplication/pdf
dc.identifier.urihttp://hdl.handle.net/1903/1897
dc.language.isoen_US
dc.subject.pqcontrolledPhysics, Atmospheric Scienceen_US
dc.titleShort-term Variability of Atmospheric Extinction During the Night, Under Clear-Sky Conditions, Investigated by Broadband Stellar Photometryen_US
dc.typeDissertationen_US

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