Abstract
The University of Hawaii (UH) Institute for Astronomy (IFA) has undergone a microthermal characterization exercise of the summit of Mt. Haleakala, Maui Hawaii. Instrumentation specific to this characterization has been developed jointly by the UH School for Ocean and Earth Science (SOEST) and the UH IFA. This paper details the instrumentation (development and characterization), discusses the specific data acquisition and reduction techniques, and gives the preliminary results of the survey.
© 1992 Optical Society of America
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