Daytime Sky Brightness Modeling of Haleakala

Details Daytime Sky Brightness Modeling of Haleakala Daytime Sky Brightness Modeling of Haleakala

Sep 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011amos.confe..63j&link_type=abstract

Proceedings of the Advanced Maui Optical and Space Surveillance Technologies Conference, held in Wailea, Maui, Hawaii, September

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We model the brightness of the daytime sky as seen from Haleakala from 0.3 to 5 microns using MODTRAN®5. Our goal was to determine the sky background radiance and transmission as a function of wavelength for imaging applications during the daytime. The sky brightness varies through a modeled day, and this is shown using a set of look angles toward the geosynchronous belt. We compare our results using radiosonde and real weather data recorded at the summit with the default atmospheric model of MODTRAN.

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