Vasilyev, Oleg B., Leyva, Amando, Muhila, Agustin, Valdes, Mauro, Peralta, Ricardo, Kovalenko, Anatoliy P., Welch, Ronald M., Berendes, Todd A., Isakov, Vladilen Yu., Kulikovskiy, Yuri P., Sokolov, Sergey S., Strepanov, Nikolay N., Gulidov, Sergey S., and Hoyningen-Huene, Wolfgang von
A spectroradiometer with wedge interference filters (SWIF) (the filters were produced by Carl Zeiss, Jena, Germany) and a CCD matrix (which was of Russian production) that functions as the sensor has been designed and built for use in ground-based optical sensing of the atmosphere and the Earth's surface in the spectral range of 0.35-1.15 [[micro]meter]. Absolute calibration of this instrument was performed through a series of observations of direct solar radiation at Mauna Loa Observatory (MLO) in Hawaii in May and June 1993. Spectral optical depth (SOD) measurements that were made during these field experiments provided detailed spectral information about both aerosol extinction (scattering plus absorption) and molecular absorption in the atmosphere above the site at MLO. The aerosol-SOD measurements were compared with narrow-band radiometer measurements at wavelengths of 380, 500, and 778 nm The SWIF and narrow-band radiometer measurements are in agreement to within the experimental error. At a wavelength of 500 nm, the aerosol SOD was found to be approximately 0.045. A description of the SWIF instrument, its absolute calibration, and the determination of atmospheric SOD's at MLO are presented. Key words: Spectroradiometer, atmospheric spectral optical depths, atmospheric transparency, light calibration.