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Phase Effects: Photometry & Polarimetry
AS3141 Benda Kecil dalam Tata SuryaProdi Astronomi 2007/2008
B. Dermawan
Observing Plane
• The plane Sun-Object-Observer is the plane of light scattering of the radiating reaching us from the Sun via the object.
• It is a symmetry-breaking plane, and because of this, makes the light from the object polarized
Karttunen et al. 1987
Photometry – Polarimetry vs Phase Angles
Photometric & Polarimetric Phase Curves
Phase Effect
• Photometric:Opposition effect (spike): A nonlinear increase in disk-integrated brightness at small solar phase angles
• Polarimetric:Negative polarization surge (polarization opposition effect): A peculiar degree of linear polarization for unpolarized incident sunlight
Muinonen et al. 2002 (Asteroids III)
Photometric & Polarimetric
Phase Effects
Physical Phenomena behind the Effects
(Classical) Shadowing Mechanism (SM)
First-order multiple scattering Coherent Backscattering Mechanism (CBM)
Higher-order (>2nd, inclusive) multiple scattering
Backscattering phenomena of atmosphereless solar system bodies (Muinonen 1994, Shkuratov et al. 1994)
Coherent Backscattering Mechanism
Photometry
Polarimetry
Muinonen et al. 2002
Spacecraft Photometry
Muinonen et al. 2002 (Asteroids III)
Hapke’s Photometric Model
Effect of shadowing
(and surface roughness)
)1(
)1)(0(
)tan(1))0(,,(
2
0
21
0
gw
gSB
BShB
h
w the single scattering albedo (efficiency of average particle to scatter and absorb light)h The width of the opposition peak (soil structure)S(0) the amplitude of the peakg the asymmetry factor of the particle phase function (the Henyey-Greenstein approx.)
the average topographic slope angle of surface roughness (does not directly obtained from the equation)
Degree of Linear Polarization
I and I are proper intensities
//
//
II
IIP
Lyot 1929
Laboratory Result
Muinonen et al. 2002 (Asteroids III)
Empirical Modeling (1)Photometric phase-effect:Shevchenko 1997, Belskaya & Shevchenko 2000:
ba
cV
1
1 ),(
Relation between parameter a and b
Shevchenko 1997
c is a parameter
Empirical Modeling (2)
Relation between the parameters (a & b) and albedo pv
b = 0.013(0.002) –
0.024(0.002) log pv
Relation between the parameters (a & b) and Pmin
b = 0.016(0.002) + 0.015(0.002) Pmin
Shevchenko 1997 Shevchenko 1997
Empirical Modeling (3)
Polarimetric phase-effect:Lumme & Muinonen 1993:
)sin(2
cos)(sin)( 021
ccbP
Describe polarization throughout the phase angle range [0, 2]
The values of the function are limited to the range [-1,1] when the parameter ranges are correctly defined
Penttilä et al. 2005
Juno
Halley
Empirical Modeling (4)
Photometric & Polarimetric phase-effects:Muinonen et al. 2002 (Mem. S. A. It., 73, 716-721), Kaasalainen et al. 2002 (Asteroids III):
kbd
af
exp)(
Photometry:
f() the relative intensity
a the height of the brightest peak
d the width of the brightest peak
b the background intensity
Polarimetry:
f() the degree of linear polarization
a an amplitude coefficient
d the angular scale
b the balancing amplitude coefficient
k the slope of linear part of the phase curve
Ceres
Empirical Models of Photometric & Polarimetric Phase-effects
Muinonen et al. 2002