Numéro |
J. Phys. IV France
Volume 133, June 2006
|
|
---|---|---|
Page(s) | 1025 - 1030 | |
DOI | https://doi.org/10.1051/jp4:2006133207 | |
Publié en ligne | 16 juin 2006 |
J.-C. Gauthier, et al.
J. Phys. IV France 133 (2006) 1025-1030
DOI: 10.1051/jp4:2006133207
Laboratory and PIC simulations of collisionless interaction between expanding space plasma clouds and magnetic field with and without ionised background
D. Mourenas1, F. Simonet1, Yu.P. Zakharov2, A.G. Ponomarenko2, V.M. Antonov2, E.L. Boyarintsev2, A.V. Melekhov2, V.G. Posukh2 and I.F. Shaikhislamov21 Département de Physique Théorique et Appliquée, CEA/DAM-Île-de-France, BP. 12, 91680 Bruyères-le-Châtel, France
2 Institute of Laser Physics (ILP), Russian Academy of Sciences, 630090 Novosibirsk, Russia
Abstract
Experiments on flute instability of plasma clouds at
Alfven Mach-number Ma 0 and 1, and with varying ion's magnetization
level have been realized at the KI-1 laser-plasma facility at the ILP of
Novosibirsk, with similarity parameters close to those of Barium releases in
Earth's magnetosphere. A number of diagnostics have allowed to characterize
the dynamics of the cloud-magnetic field interaction, as well as flutes
development, or suppression for Ma > 1. Hybrid simulations with HAWAI2D code
have reproduced the main observed features, such as the diamagnetic cavity
dynamics, and flutes growth. A mode-mixing phenomenon related to Larmor
rotation has been observed in simulations, which seems to lead to a
reduction of mode number at later times in agreement with experimental
results.
© EDP Sciences 2006