Fractal dust grains around R Coronae Borealis stars

1989 ◽  
Vol 346 ◽  
pp. L89 ◽  
Author(s):  
Edward L. Wright
2008 ◽  
Vol 36 (1) ◽  
pp. 310-314 ◽  
Author(s):  
Lorin S. Matthews ◽  
Truell W. Hyde
Keyword(s):  

1989 ◽  
pp. 337-342 ◽  
Author(s):  
Edward L. Wright
Keyword(s):  

2012 ◽  
Vol 19 (9) ◽  
pp. 093708 ◽  
Author(s):  
F. Huang ◽  
R. D. Peng ◽  
Y. H. Liu ◽  
Z. Y. Chen ◽  
M. F. Ye ◽  
...  
Keyword(s):  

1998 ◽  
Vol 498 (2) ◽  
pp. 757-762 ◽  
Author(s):  
B. R. Ragot
Keyword(s):  

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.


Sign in / Sign up

Export Citation Format

Share Document