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Distribution of the Spectropolarimetric Parameter of the Moon in the Northern Part of Ocean Procellarum for a Large Phase Angle

机译:大相位角月球在大洋北部北部的光谱极化参数分布

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Polarimetric observations of the moon have been carried out at λ_(eff) = 0.48 and 0.63 μm using the 50 cm telescope of the Maidanak (Middle Asia) observatory. Imaging has been performed using a Canon-350D camera with a CMOS array and rotating polaroid. The investigation covered the north-western part of the lunar disk comprising the northern part of Ocean Procellarum and obtained the images representing the albedo, polarization degree, color index, and polarimetric color ratio at a phase angle of 96°. It is the first time that the latter parameter has been imaged with a resolution of approximately 1 km. Its pattern has proved to resemble that of the color index, although some impor-tant differences can be seen. This shows that spectropolarimetric observations of the moon can give new information on the composition and optical properties of the lunar regolith.
机译:使用迈达纳克(中亚)天文台的50厘米望远镜在λ_(eff)= 0.48和0.63μm处进行了月球的偏振观测。使用具有CMOS阵列和旋转宝丽来的Canon-350D相机进行了成像。研究覆盖了月球的西北部分,包括海洋Procellarum的北部,并获得了代表反照率,偏振度,色指数和偏振色比的图像,相位角为96°。这是第一次以大约1 km的分辨率对后一个参数成像。尽管可以看到一些重要的差异,但事实证明,它的图案类似于颜色指数。这表明对月球的光谱极化观测可以提供有关月球巨石的组成和光学性质的新信息。

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