Book contents
- Half title page
- Title page
- Copyright page
- Dedication
- Contents
- Contributors
- I Introduction
- II Theory, instrumentation, and laboratory studies
- III Stars and their environment
- IV Solar system
- 16 The Sun
- 17 Terrestrial planets
- 18 The Moon
- 19 Gas giant planets, Saturn’s rings, and Titan
- 20 Icy moons of the outer planets
- 21 Asteroids
- 22 Comets
- 23 Transneptunian objects and Centaurs
- 24 Interplanetary dust
- V Exoplanets and exobiology
- Book part
- Index
- References
18 - The Moon
from IV - Solar system
Published online by Cambridge University Press: 05 May 2015
Book contents
- Half title page
- Title page
- Copyright page
- Dedication
- Contents
- Contributors
- I Introduction
- II Theory, instrumentation, and laboratory studies
- III Stars and their environment
- IV Solar system
- 16 The Sun
- 17 Terrestrial planets
- 18 The Moon
- 19 Gas giant planets, Saturn’s rings, and Titan
- 20 Icy moons of the outer planets
- 21 Asteroids
- 22 Comets
- 23 Transneptunian objects and Centaurs
- 24 Interplanetary dust
- V Exoplanets and exobiology
- Book part
- Index
- References
Summary
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- Chapter
- Information
- Polarimetry of Stars and Planetary Systems , pp. 303 - 319Publisher: Cambridge University PressPrint publication year: 2015
References
Akimov, L. A. and Shkuratov, Yu. G. (1983). Optical research on lunar soil samples of different degrees of maturity. Solar System Research, 17, 152–158.Google Scholar
Bandermann, L. W., Kemp, L. C., and Wolstencroft, R. D. (1972). Circular polarization of light scattered from rough surfaces. Monthly Notices of the Royal Astronomical Society, 158, 291–304.CrossRefGoogle Scholar
Bohren, C. F. and Huffman, D. R. (2004). Absorption and Scattering of Light by Small Particles. WILEY-VCH Verlag GmbH & Co.Google Scholar
Bowell, E. and Zellner, B. (1974). Polarizations of asteroids and satellites. In Gehrels, T., ed., Planets, Stars, and Nebulae Studied with Photopolarimetry. Tucson: University of Arizona Press, pp. 381–404.Google Scholar
Bowell, E., Dollfus, A., and Geake, J. (1972). Polarimetric properties of the Lunar surface and its interpretation. Part 5: Apollo 14 and Luna 16 lunar samples. Proceedings of the 3rd Lunar Science Conference. Houston, USA: LPI, pp. 3103–3126.Google Scholar
Burns, R. (1993). Mineralogical Applications of Crystal Field Theory. Cambridge University Press.CrossRefGoogle Scholar
Degtyarev, V. and Kolokolova, L. (1992). Possible application of circular polarization for remote sensing of cosmic bodies. Earth, Moon, and Planets, 57, 213–223.CrossRefGoogle Scholar
Dollfus, A. (1962). The polarization of moonlight. Chapter 18. In Kopal, Z., ed., Physics and Astronomy of the Moon. Academic Press Inc., pp. 131–139.Google Scholar
Dollfus, A. (1998). Lunar surface imaging polarimetry: I. Roughness and grain size. Icarus, 136, 69–103.CrossRefGoogle Scholar
Dollfus, A. (1999). Lunar surface imaging polarimetry: II. Mare Fecunditatis and Messier. Icarus, 140, 313–327.CrossRefGoogle Scholar
Dollfus, A. (2000). Lunar surface imaging polarimetry. III. Langrenus. Icarus, 146, 420–429.CrossRefGoogle Scholar
Dollfus, A. and Bowell, E. (1971). Polarimetric properties of the lunar surface and interpretation. I. Telescope observation. Astronomy and Astrophysics, 10, 29–53.Google Scholar
Dollfus, A. and Titulaer, C. (1971). Polarimetric properties of the lunar surface and its interpretation. Part III. Astronomy and Astrophysics, 12, 199–209.Google Scholar
Dzhapiashvili, V. P. and Korol, A. N. (1982). Polarimetric Atlas of the Moon. Tbilisi: Metsniereba.Google Scholar
Engelhardt, W., Hurrle, H., and Luft, E. (1976). Microimpact-induced changes of textural parameters and modal composition of the lunar regolith. Proceedings of the 7th Lunar Planetary Science Conference. Houston, USA: LPI, pp. 373–392.Google Scholar
Evsyukov, N. N., and Shestopalov, D. I. (1976). Polarimetric mapping of the Moon. Soviet Astronomy, 19, 772–775.Google Scholar
Fox, G., Code, A., Anderson, C.et al. (1998). Solar system observations by the Wisconsin Ultraviolet Photopolarimeter Experiment – III. The first ultraviolet spectropolarimetry of the Moon. Monthly Notices of the Royal Astronomical Society, 298, 303–309.CrossRefGoogle Scholar
Grynko, E. and Shkuratov, Yu. (2003). Scattering matrix for semitransparent particles of different shapes in geometric optics approximation. Journal of Quantitative Spectroscopy and Radiative Transfer, 78, 319–340.CrossRefGoogle Scholar
Grynko, E. S. and Shkuratov, Yu. G. (2007). Ray tracing sumulation of light scattering by spherical clusters consisting of particles with different shapes. Journal of Quantitative Spectroscopy and Radiative Transfer, 106, 56–62.CrossRefGoogle Scholar
Hapke, B. (1971). Optical properties of the lunar surface. In Kopal, Z., ed., Physics and Astronomy of the Moon. New York: Academic Press, pp. 155–211.Google Scholar
Hapke, B. (2012). Theory of Reflectance and Emittance Spectroscopy. Cambridge University Press.CrossRefGoogle Scholar
Hapke, B. W., Nelson, R. M., and Smythe, W. D. (1974). The opposition effect of the moon: The contribution of coherent backscatter. Science, 260(5107), 509–511.CrossRefGoogle Scholar
Heiken, G. H., McKay, D. S., and Brown, R. W. (1974). Lunar deposits of possible pyroclastic origin. Geochimica et Cosmochimica Acta, 38, 1703–1718.CrossRefGoogle Scholar
Kaydash, V., Shkuratov, Y., and Videen, G. (2012). Phase-ratio imagery as a tool of lunar remote sensing. Journal of Quantitative Spectroscopy and Radiative Transfer, 113, 2601–2607.CrossRefGoogle Scholar
Kemp, J. C., Wolstencroft, R. D., and Swedlung, J. B. (1971). Circular polarization: Jupiter and other planets. Nature, 232, 165–168.CrossRefGoogle ScholarPubMed
Kornienko, Y. V., Shkuratov, Y. G., Bychinskii, V. I., and Stankevich, D. G. (1982). Correlation between albedo and polarization characteristics of the Moon – application of digital image processing. Soviet Astronomy, 26, 345–348.Google Scholar
Korokhin, V. V. and Velikodsky, Y. I. (2005). Parameters of the positive polarization maximum of the Moon: Mapping. Solar System Research, 39, 45–53.CrossRefGoogle Scholar
Kvaratskhelia, O. I. (1988). Spectropolarimetry of the lunar surface and samples of the lunar soil. Bulletin of Abastumari Astrophysical Observatory, 64, 1–312.Google Scholar
Lipsky, Y. N. and Pospergelis, M. M. (1967). Several results of measuring the complete Stokes vector for lunar surface features. Astronomicheskii Zhurnal, 44, 410–412.Google Scholar
Lyot, B. (1929). Recherches sur la polarisation de la lumière des planètes et de quelques substances terrestres. Annales de l’Observatoire de Paris, section de Meudon, 8, 1–161.Google Scholar
Mishchenko, M., Dlugach, J., Liu, L. et al. (2009). Direct solutions of the Maxwell equations explain opposition phenomena observed for high-albedo solar system objects. The Astrophysical Journal Letters, 705, L118–L122.CrossRefGoogle Scholar
Muinonen, K. (1989). Electromagnetic scattering by two interacting dipoles. In Proceedings of the 1989 URSI International Symposium on Electromagnetic Theory. Stockholm: Royal Institute of Technology (Stockholm), pp. 428–430.Google Scholar
Novikov, V. V. (1980). Polarimetry as a tool of remote sensing selenochemistry. Trudy Shternberg Gosudarstvennogo Astronomicheskogo Instituta Moscow, 50, 135–149.Google Scholar
Opanasenko, N. V. and Shkuratov, Y. G. (1994). Results of simultaneous polarimetry and photometry of the Moon. Solar System Research, 28, 398–417.Google Scholar
Opanasenko, N. V., Dolukhanyan, A. A., Shkuratov, Y. G.et al. (1994). Polarization map of the Moon at the minimum of the negative branch. Solar System Research, 28, 98–105.Google Scholar
Opanasenko, N. V., Opanasenko, A. N., Shkuratov, Y. G.et al. (2009). The negative polarization parameters of the light scattered by the lunar surface: Mapping. Solar System Research, 43, 210–214.CrossRefGoogle Scholar
Opanasenko, N., Shkuratov, Y., Kaydash, V.et al. (2013). Preliminary mapping negative polarization of the lunar nearside. In Proceedings of the 44th Lunar and Planetary Science Conference. Houston: LPI, p. 1354.Google Scholar
Shestopalov, D. I., McFadden, L. A., Golubeva, L. F., Khomenko, V. M., and Gasanova, L. O. (2008). Vestoid surface composition from analysis of faint absorption bands in visible reflectance spectra. Icarus, 195, 649–662.CrossRefGoogle Scholar
Shkuratov, Y. G. (1981). Connection between the albedo and polarization properties of the Moon. Fresnel component of reflected light. Soviet Astronomy, 25(4), 490–494.Google Scholar
Shkuratov, Y. G. (1985). On the origin of the opposition effect and negative polarization for cosmic bodies with solid surface. In Astronomicheskii Circular, No. 1400. Moscow: Sternberg State Astronomy Institute, pp. 3–6.Google Scholar
Shkuratov, Y. G. (1987). Negative polarization of sunlight scattered from celestial bodies: Interpretation of the wavelength dependence. Soviet Astronomy Letters, 13, 182–183.Google Scholar
Shkuratov, Y. (1988). Diffraction model of the brightness surge of complex structure surfaces. Kinematics and Physics of Celestial Bodies, 4, 33–39.Google Scholar
Shkuratov, Y. G. and Basilevsky, A. T. (1981). An attempt at mapping the parameter of surface micro porosity of lunar regolith: Correlation between albedo and polarization properties of the Moon. In Proceedings of the 12th Lunar and Planetary Science Conference. Houston, USA: LPI, pp. 1981–1983.Google Scholar
Shkuratov, Y. and Grynko, Y. (2005). Scattering by semitransparent particles of different shapes and media consisting of these particles in geometric optics approximation: Consequences for photometry and spectroscopy of the planetary regoliths. Icarus, 173, 16–28.CrossRefGoogle Scholar
Shkuratov, Y. G. and Opanasenko, N. V. (1990). On the limb polarimetric effect in the Moon discovered by Lyot. Astronomicheskii Vestnik, 24(4), 333–336 [in Russian].Google Scholar
Shkuratov, Y. G. and Opanasenko, N. V. (1992). Polarimetric and photometric study of the Moon: Telescope observation and laboratory simulation. 2. The positive polarization. Icarus, 99, 468–484.CrossRefGoogle Scholar
Shkuratov, Y. G., Opanasenko, N. V., and Kreslavsky, M. A. (1992a). Polarimetric and photometric properties of the Moon: Telescope observation and laboratory simulation. 1. The negative polarization. Icarus, 95, 283–299.CrossRefGoogle Scholar
Shkuratov, Y. G., Kreslavsky, M. A., and Opanasenko, N. V. (1992b). Analysis of a mechanism of negative polarization of light scattered by the surfaces of atmosphereless celestial bodies. Solar System Research, 26, 33–38.Google Scholar
Shkuratov, Y., Muinonen, K., Bowell, E.et al. (1994). A critical review of theoretical models for the negative polarization of light scattered by atmosphereless solar system bodies. Earth, Moon, and Planets, 65, 201–246.CrossRefGoogle Scholar
Shkuratov, Y., Ovcharenko, A., Zubko, E. et al. (2002). The opposition effect and negative polarization of structurally simulated planetary regoliths. Icarus, 159, 396–416.CrossRefGoogle Scholar
Shkuratov, Yu., Ovcharenko, A., Zubko, E.et al. (2004). The negative polarization of light scattered from particulate surfaces and of independently scattering particles. Journal of Quantitative Spectroscopy and Radiative Transfer, 88, 267–284.CrossRefGoogle Scholar
Shkuratov, Y., Opanasenko, N., Zubko, E.et al. (2007). Multispectral polarimetry as a tool to investigate texture and chemistry of lunar regolith particles. Icarus, 187, 406–416.CrossRefGoogle Scholar
Shkuratov, Yu., Opanasenko, N., Opanasenko, A.et al. (2008). Polarimetric mapping of the Moon at a phase angle nearby minimum of polarization degree. Icarus, 198, 1–6.CrossRefGoogle Scholar
Shkuratov, Y., Kaydash, V., Korokhin, V.et al. (2011). Optical measurements of the Moon as a tool to study its surface. Planetary and Space Science, 59, 1326–1371.CrossRefGoogle Scholar
Stankevich, D., Istomina, L., Shkuratov, Yu., and Videen, G. (2007). The coherent backscattering effects in a random medium as calculated using a ray tracing technique for large non-transparent spheres. Journal of Quantitative Spectroscopy and Radiative Transfer, 106, 509–519.CrossRefGoogle Scholar
Sterzik, M. F., Bagnulo, S., and Palle, E. (2012). Biosignatures as revealed by spectropolarimetry of Earthshine. Nature, 483 (7387), 64–66, doi: 10.1038/nature10778.CrossRefGoogle ScholarPubMed
Takashi, J., Iton, Y., Akitaya, H. et al. (2013). Phase variation of Earthshine polarization spectra. Publications of the Astronomical Society of Japan, 65, 38–1–9.CrossRefGoogle Scholar
Umov, N. (1905). Chromatische depolarisation durch Lichtzerstreuung. Physikalische Zeitschrift, 6, 674–676.Google Scholar
Wolff, M. (1980). Theory and application of the polarization-albedo rules. Icarus, 44, 780–792.CrossRefGoogle Scholar
Zellner, B., Leake, M., Lebertre, T., Duseaux, M., and Dollfus, A. (1977). The asteroid albedo scale. I. Laboratory polarimetry of meteorites. Proceedings of the 8th Lunar Science Conference. Houston, USA: LPI, pp. 1091–1110.Google Scholar
Zubko, E., Kimura, H., Shkuratov, Y.et al. (2009). Effect of absorption on light scattering by agglomerated debris particles. Journal of Quantitative Spectroscopy and Radiative Transfer, 110, 1741–1749.CrossRefGoogle Scholar
Zubko, E., Videen, G., Shkuratov, Y., Muinonen, K., and Yamamoto, T. (2011). The Umov effect for single irregularly shaped particles with size comparable with wavelength. Icarus, 212, 403–415.CrossRefGoogle Scholar
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