Abstract
To gain a lunar absolute radiance and reflectance, the lunar images at 650nm had been observed with a cooling CCD camera mounted on telescope. The absolute radiance was derived through dark-field correction, flat-field correction, radiance calibration, atmospheric correction, and photometric correction. And the reflectance was calculated by being divided by the solar radiance estimated from the Plank's black body radiation Law. The 750nm reflectance of Apollo 16 WEST calibration site of Clementine UVVIS images was compared with our reflectances converted into those at 750 nm using a shape of Apollo 16 sample 62231 spectrum. As the result, our reflectance is 0.56 times that of Clementine UVVIS images. In this presentation the near-side images of the lunar absolute radiance and reflectance are shown.
