Astronomy and Astrophysics – Astrophysics
Scientific paper
Dec 2003
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003agufmsm31c1121l&link_type=abstract
American Geophysical Union, Fall Meeting 2003, abstract #SM31C-1121
Astronomy and Astrophysics
Astrophysics
2780 Solar Wind Interactions With Unmagnetized Bodies, 6218 Jovian Satellites, 7843 Numerical Simulation Studies
Scientific paper
The comets play important role as a simulation laboratory for multiscale kinetic plasma processes which are key-role processes in space and laboratory plasmas. A development of multiscale combined numerical methods allows us to use more realistic cometary plasma models (see, e.g. [Häberli et al., 1997; Delamere et al., 1999; Bagdonat and Motschmann, 2002; Lipatov et al., 2002]). In this report, we develop a Particle-Ion--Fluid-Ion--Fluid--Electron method of kinetic ion-neutral simulation (see, e.g. [Lipatov, 2002]), which is based on a multiscale adaptive mesh, particle and algorithm refinement. This method takes into account charge-exchange and photoionization processes. The first results of such simulation of the dynamics of ions near comet Borrelly are discussed in this report. ~
R Häberli, M R Combi, T I Gombosi, D L De Zeeuw, K G Powell, Icarus, 130, 373, 1997.
P A Delamere, D W Swift, H C Stenbaek-Nielsen, Geophys. Res. Lett., 26(18), 2837, 1999.
T Bagdonat, U Motschmann, Earth, Moon and Planets, 90, 305, 2002.
A S Lipatov, The Hybrid Multiscale Simulation Technology. An Introduction with Application to Astrophysical and Laboratory Plasmas, Springer-Verlag, Berlin, Heidelberg, New York, 2002, p.p. 1-403.
A S Lipatov, U Motschmann, T Bagdonat, Planet. Space Sci., 50, 403, 2002.
Combi Michael R.
Lipatov Alexander S.
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