scholarly journals Application of the monte carlo test particle method to calсulate transport coefficiens in diluted gases

Author(s):  
Finnikov Konstantin ◽  
2020 ◽  
Author(s):  
Anita Linnéa Elisabeth Werner ◽  
François Leblanc ◽  
Jean-Yves Chaufray ◽  
Ronan Modolo

<div>The Mercury plasma environment is enriched in heavy ions (mass-per-charge ratio m/q > 4) from photo-ionization of the tenuous exosphere. The MErcury Surface, Space ENvironment, GEochemistry, and Ranging (MESSENGER) time-of-flight spectrometer Fast Imaging Plasma Spectrometer (FIPS) has detected many planetary ion species of which He<sup>+</sup>, the Na<sup>+</sup>-group (including Na<sup>+</sup>, Mg<sup>+</sup> and Si<sup>+</sup>) and the O<sup>+</sup>-group (including O<sup>+</sup> and several water group ions) are the most abundant. The Mercury Atmospheric and Surface Composition Spectrometer (MASCS) UltraViolet and Visible Spectrometer (UVVS) has also detected Ca<sup>+</sup> ions in the nightside plasma sheet. Models of the planetary ion distribution inside Mercury's magnetosphere have mostly concentrated on the abundant Na<sup>+</sup> and H<sup>+</sup> ion populations. Comparison with FIPS data has been limited to the first two MESSENGER flybys and no comparison has been made with MASCS/UVVS observations.</div><div> </div><div>We have developed a Monte Carlo test-particle model which describes the ion density distribution produced from photo-ionization of several neutral species in Mercury's exosphere. The global ion density and energy distribution of Ca<sup>+</sup>, Mg<sup>+</sup>, Na<sup>+</sup>, O<sup>+</sup> and He<sup>+</sup> will be presented here. We will review the influence of the interplanetary magnetic field (IMF) B<sub>x</sub> and B<sub>y</sub> components on the global structure of the ion density distribution, the composition of the nightside plasma sheet and the evolution of the Na<sup>+</sup> ion density along the Mercury year.</div>


2016 ◽  
Vol 69 (3) ◽  
pp. 620-627 ◽  
Author(s):  
Simpp Äkäslompolo ◽  
Tain Kurki-Suonio ◽  
Sepp Sipilä ◽  
ASCO Group

1991 ◽  
Vol 1 (1) ◽  
pp. 37-60 ◽  
Author(s):  
Wolfgang Paul ◽  
Kurt Binder ◽  
Dieter W. Heermann ◽  
Kurt Kremer

1995 ◽  
Vol 85 (4) ◽  
pp. 781-792 ◽  
Author(s):  
Jadran Vrabec ◽  
Johann Fischer

1999 ◽  
Vol 32 (5) ◽  
pp. 917-923 ◽  
Author(s):  
Bo Sjöberg

Computer simulations using Monte Carlo methods are used to investigate the effects of interparticle correlations on small-angle X-ray and neutron scattering from moderate or highly concentrated systems of ellipsoids of revolution. Both oblate and prolate ellipsoids, of varying eccentricities and concentrations, are considered. The advantage with Monte Carlo simulation is that completely general models, both regarding particle shapes and interaction potentials, can be considered. Equations are also given that relate the nonideal part of the chemical potential, βμni, with the scattering at zero angle,I(0), and the compressibility factor,z. The quantity βμnican be obtained during the Monte Carlo simulations by using Widom's test-particle method. For spherical particles, the simulations are compared with approximation formulas based on the Percus–Yevick equation. A method is also suggested for the calculation of both βμniandzfrom experimental values ofI(0) recorded as a function of concentration.


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