Light scattering by small particles and models of interplanetary matter derived from the zodiacal light

1963 ◽  
Vol 1 (3) ◽  
Author(s):  
R.H. Giese
1964 ◽  
Vol 69 ◽  
pp. 550
Author(s):  
S. Little ◽  
B. J. O'Mara ◽  
L. H. Aller

1985 ◽  
Vol 85 ◽  
pp. 223-226
Author(s):  
K. Weiss-Wrana ◽  
R.H. Giese ◽  
R.H. Zerull

AbstractThe investigations of light scattering by larger meteoritic and terrestrial single grains (size range 20 μm to 120 μm ) demonstrate that the scattering properties of irregularly shaped dark opaque particles with very rough surfaces resemble the characteristic features of the empirical scattering function as derived from measurements of the zodiacal light. Purely transparent or translucent irregularly shaped particles show a quite different scattering behaviour. Furthermore irregular and multicomponent fluffy particles in the size range of a few microns were modelled by microwave analog measurements in order to explain positive and negative polarization of the light scattered by cometary dust grains.


Author(s):  
Ivan Kassamakov ◽  
Tuomas Puranen ◽  
Göran Maconi ◽  
Maria Gritsevich ◽  
Antti Penttilä ◽  
...  

1991 ◽  
Vol 126 ◽  
pp. 163-170 ◽  
Author(s):  
P.L. Lamy ◽  
J.M. Perrin

AbstractAfter briefly evaluating the observations of the Zodiacal Light and F-corona, we review the laboratory results on the light scattering by dust particles and the various theories which have been recently proposed. We then discuss the optical properties of the dust with emphasis on the phase function, the polarization, the color, the albedo and the local enhancement in the Gegenschein.


1965 ◽  
Vol 70 ◽  
pp. 346 ◽  
Author(s):  
S. J. Little ◽  
B. J. O'Mara ◽  
L. H. Aller

2012 ◽  
Vol 97 (4) ◽  
pp. 44005 ◽  
Author(s):  
M. I. Tribelsky ◽  
A. E. Miroshnichenko ◽  
Y. S. Kivshar

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