Coherent backscattering and opposition effects observed in some atmosphereless bodies of the solar system

The results of photometric and polarimetric observations carried out for some bright atmosphere-less bodies of the Solar system near the zero phase angle reveal the simultaneous existence of two spectacular optical phenomena, the so-called brightness and polarization opposition effects. In a number of studies, these phenomena were explained by the influence of coherent backscattering. However, in general, the interference concept of coherent backscattering can be used only in the case where the particles are in the far-field zones of each other, i.e., when the scattering medium is rather rarefied. Because of this, it is important to prove rigorously and to demonstrate that the coherent backscattering effect may also exist in densely packed scattering media like regolith surface layers of celestial bodies. From the results of the computer modeling performed with the use of numerically exact solutions of the macroscopic Maxwell equations for discrete random media with different packing densities of particles, we studied the origin and evolution of all the opposition phenomena predicted by the coherent backscattering theory for low-packing-density media. It has been shown that the predictions of this theory remain valid for rather high packing densities of particles that are typical, in particular, of regolith surfaces of the Solar system bodies. The results allow us to conclude that both opposition effects observed simultaneously in some high-albedo atmosphereless bodies of the Solar system are caused precisely by coherent backscattering of solar light in the regolith layers composed of microscopic particles.

[1]  M. Mishchenko On the nature of the polarization opposition effect exhibited by Saturn's rings , 1993 .

[2]  Michael I. Mishchenko,et al.  Azimuthal asymmetry of the coherent backscattering cone: Theoretical results , 2009 .

[3]  J. Gradie,et al.  Minor planets and related objects. XX - Polarimetric evidence for the albedos and compositions of 94 asteroids , 1976 .

[4]  M. Mishchenko,et al.  COHERENT BACKSCATTERING VERIFIED NUMERICALLY FOR A FINITE VOLUME OF SPHERICAL PARTICLES , 2012 .

[5]  K. Jockers,et al.  Polarization and brightness opposition effects for the E-type Asteroid 64 Angelina , 2005 .

[6]  M. Mishchenko Polarization characteristics of the coherent backscatter opposition effect , 1992 .

[7]  V. Rosenbush,et al.  Polarization opposition effect for the Galilean satellites of Jupiter , 2005 .

[8]  Lagendijk,et al.  Light scattering in strongly scattering media: Multiple scattering and weak localization. , 1988, Physical review. B, Condensed matter.

[9]  Michael I. Mishchenko,et al.  Numerically exact computer simulations of light scattering by densely packed, random particulate media , 2011 .

[10]  Richard P. Binzel,et al.  Phase relations of high albedo asteroids: The unusual opposition brightening of 44 Nysa and 64 Angelina☆ , 1989 .

[11]  V. L. Kuzmin,et al.  REVIEWS OF TOPICAL PROBLEMS: Coherent phenomena in light scattering from disordered systems , 1996 .

[12]  M. van der Mee,et al.  Transfer of Polarized Light in Planetary Atmospheres: Basic Concepts and Practical Methods , 2005 .

[13]  J. Piironen,et al.  The Opposition Effect and Negative Polarization of Structural Analogs for Planetary Regoliths , 2002 .

[14]  Nieuwenhuizen,et al.  Full angular profile of the coherent polarization opposition effect , 2000, Journal of the Optical Society of America. A, Optics, image science, and vision.

[15]  D. Campbell,et al.  Radar imaging of Saturn's rings , 2005 .

[16]  D. Mackowski A simplified model to predict the effects of aggregation on the absorption properties of soot particles , 2006 .

[17]  Brian Cairns,et al.  Multiple scattering by random particulate media: exact 3D results. , 2007, Optics express.

[18]  M. I. Mishchenko,et al.  Coherent backscatter and the opposition effect for E-type asteroids , 1993 .

[19]  A. Lacis,et al.  Multiple Scattering of Light by Particles: Radiative Transfer and Coherent Backscattering , 2006 .

[20]  Kenneth M. Watson,et al.  Multiple Scattering of Electromagnetic Waves in an Underdense Plasma , 1969 .

[21]  G. Pettengill,et al.  Radar observations of Saturn's rings at intermediate tilt angles , 1980 .

[22]  M. Mishchenko,et al.  Can weak localization of photons explain the opposition effect of Saturn's rings? , 1992 .

[23]  Michael I. Mishchenko,et al.  Weak localization of electromagnetic waves and radar polarimetry of Saturn's rings , 2008 .

[24]  Karri Muinonen,et al.  Light scattering by inhomogeneous media : backward enhancement and reversal of linear polarization , 1990 .

[25]  Paul E. Johnson,et al.  New results from optical polarimetry of Saturn's rings , 1980, Nature.

[26]  F. Franklin,et al.  Optical properties of Saturn's rings. II. Two-color phase curves of the 2 bright rings. , 1965 .

[27]  Andrew A. Lacis,et al.  Scattering, Absorption, and Emission of Light by Small Particles , 2002 .

[28]  Gorden Videen,et al.  Polarimetric detection, characterization, and remote sensing , 2011 .

[29]  Michael I. Mishchenko,et al.  Calculation of the T matrix and the scattering matrix for ensembles of spheres , 1996 .

[30]  Yu. A. Kravtsov,et al.  II Enhanced Backscattering in Optics , 1991 .

[31]  M. Mishchenko,et al.  A multiple sphere T-matrix Fortran code for use on parallel computer clusters , 2011 .

[32]  M. Mishchenko,et al.  Weak localization of electromagnetic waves and opposition phenomena exhibited by high-albedo atmosphereless solar system objects. , 2006, Applied optics.

[33]  E. V. Petrova,et al.  Modeling of opposition effects with ensembles of clusters: Interplay of various scattering mechanisms , 2007 .

[34]  E. V. Petrova,et al.  Light scattering by morphologically complex objects and opposition effects (a review) , 2011 .

[35]  G. Maret,et al.  Theoretical study of the coherent backscattering of light by disordered media , 1988 .

[36]  M. Mishchenko,et al.  DIRECT SOLUTIONS OF THE MAXWELL EQUATIONS EXPLAIN OPPOSITION PHENOMENA OBSERVED FOR HIGH-ALBEDO SOLAR SYSTEM OBJECTS , 2009 .

[37]  G. Lockwood,et al.  Photoelectric photometry of Europa and Callisto 1976–1991 , 1992 .

[38]  M. I. Mishchenko,et al.  Enhanced backscattering of polarized light from discrete random media : calculations in exactly the backscattering direction , 1992 .