By Wing-Huen Ip, Anil Bhardwaj
Advances in Geosciences is the results of a concerted attempt in bringing the newest effects and making plans actions relating to earth and house technology in Asia and the overseas enviornment. the quantity editors are all major scientists of their examine fields masking six sections: Hydrological technology (HS), Planetary technology (PS), sunlight Terrestrial (ST), reliable Earth (SE), Ocean technological know-how (OS) and Atmospheric technological know-how (AS). the most objective is to focus on the medical concerns necessary to the learn of earthquakes, tsunamis, atmospheric airborne dirt and dust storms, weather switch, drought, flood, typhoons, monsoons, area climate, and planetary exploration.
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Extra info for Advances in Geosciences: Planetary Science (PS) (Advances in Geosciences)
Brunini, Icarus 138 (1999) 129. 7. K. Muinonen, J. Piironen, Yu. Shkuratov, A. Ovcharenko and B. E. Clark, in Asteroids III, eds. W. F. Bottke, A. Cellino, P. Paolicchi and R. P. Binzel (University of Arizona Press, Tucson, 2002), pp. 123–138. 8. Yu. G. Shkuratov, A. Ovcharenko, E. Zubko, D. Stankevich, O. Miloslavskaya, K. Muinonen, J. Piironen, R. Nelson, W. Smythe, V. Rosenbush and P. Helfenstein, Icarus 159 (2002) 396. 9. A. C. Levasseur-Regourd, E. Hadamcik and J. Lasue, Adv. Space Res. 37 (2006) 161.
2 shows that in a plot of Pmin vs. polarimetric inversion angle, not only there is a clear separation between low (F , B, C, G, D) intermediate (S, M ) and highalbedo (E) objects, but also there is a fairly clear separation even among objects of similar albedo. As a matter of fact, a recent analysis12 has convincingly shown that the availability of a good coverage of the phase– polarization curve for a sample of objects is suﬃcient to derive a taxonomic classiﬁcation in very good agreement with that produced by spectroscopic data.
At the Paris-Meudon Observatory, and subsequently by other researchers in diﬀerent countries. 2 The observations allow the observers to directly measure the degree of polarization of light coming from an asteroid. The state of polarization of a light beam is described by the Stokes parameters Q and U (giving the degree of linear polarization), V (related to circular polarization), and I (the total intensity of the received light). In asteroid polarimetry, the V parameter is usually negligible, and the light is in a state of partial linear polarization described by the Stokes parameters Q and U .