| タイトル | A Wavelength-Dependent Visible and Infrared Spectrophotometric Function for the Moon based on ROLO Data |
| 著者（英） | Boardman, J.; Stone, T. C.; Staid, M.; Pieters, C. M.; Sunshine, J.; Buratti, B. J.; Nettles, J.; Hicks, M. D. |
| 著者所属（英） | Jet Propulsion Lab., California Inst. of Tech. |
| 発行日 | 2011-04-05 |
| 言語 | eng |
| 内容記述 | The USGS's Robotic Lunar Observatory (ROLO) dedicated ground-based lunar calibration project obtained photometric observations of the Moon over the spectral range attainable from Earth (0.347-2.39 microns) and over solar phase angles of 1.55 deg -97 deg . From these observations, we derived empirical lunar surface solar phase functions for both the highlands and maria that can be used for a wide range of applications. The functions can be used to correct for the effects of viewing geometry to produce lunar mosaics, spectra, and quick-look products for future lunar missions and ground-based observations. Our methodology can be used for a wide range of objects for which multiply scattered radiation is not significant, including all but the very brightest asteroids and moons. |
| NASA分類 | Lunar and Planetary Science and Exploration |
| 権利 | Copyright |
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