Effect of multiple scattering on the accuracy of velocity profile reconstruction from the Monte-Carlo simulated OCDT signal in a model of biological tissues

2006 ◽  
Author(s):  
A. V. Bykov ◽  
M. Yu. Kirillin ◽  
A. V. Priezzhev ◽  
R. A. Myllylä
Keyword(s):  
Monte Carlo ◽  
Velocity Profile ◽  
Multiple Scattering ◽  
Biological Tissues ◽  
Profile Reconstruction

scholarly journals Monte Carlo simulation of halos in the crystal clouds

2021 ◽  
Vol 2099 (1) ◽  
pp. 012067
Author(s):  
Q Mu ◽  
E G Kablukova ◽  
B A Kargin ◽  
S M Prigarin
Keyword(s):  
Monte Carlo Simulation ◽  
Monte Carlo ◽  
Monte Carlo Method ◽  
Ray Tracing ◽  
Multiple Scattering ◽  
Radiation Transfer ◽  
Cirrus Clouds ◽  
Ice Crystals ◽  
The Sun ◽  
Different Shapes

Abstract In this paper, we try to answer the question: how the multiple scattering, the sun elevation, shape and orientation of ice crystals in the cirrus clouds affect a halo pattern. To study the radiation transfer in optically anisotropic clouds, we have developed the software based on Monte Carlo method and ray tracing. In addition to halos, this software enables one to simulate “anti-halos”, which above the cloud layer can be seen by observers. We present the visualization of halos and anti-halos generated by the cirrus clouds for different shapes and orientations of ice crystals.

Monte Carlo for multiple scattering and nonspherical particles

2004 ◽  
Author(s):  
Piero Bruscaglioni ◽  
Giovanni Zaccanti ◽  
Samuele del Bianco ◽  
G. Bazzini ◽  
Marco Gai
Keyword(s):  
Monte Carlo ◽  
Multiple Scattering ◽  
Nonspherical Particles

scholarly journals Polarization in Wolf-Rayet binaries: Monte Carlo simulations

1995 ◽  
Vol 163 ◽  
pp. 260-261
Author(s):  
Cláudia V. Rodrigues ◽  
Antonio Mário Magalhães
Keyword(s):  
Monte Carlo ◽  
Light Curve ◽  
Monte Carlo Simulations ◽  
Multiple Scattering ◽  
Linear Polarization ◽  
Monte Carlo Code ◽  
Circumstellar Envelopes ◽  
Analytical Approaches

We present some results on circumstellar envelopes using a Monte Carlo code we are developing. In contrast to analytical approaches, the effects of multiple scattering and the finite sizes of sources and envelope have been incorporated in the models. As an illustration, we fit the light-curve of V444 Cyg as well as the modulation of the linear polarization throughout its orbit.

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