Long time evolution of collisionless shocks in laser produced counterstreaming plasmas
| Autor: | Nigel Woolsey, H. Takabe, Youichi Sakawa, Christopher D. Gregory, M. Koenig, J. N. Waugh, Taichi Morita, Yasuhiro Kuramitsu |
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| Rok vydání: | 2013 |
| Předmět: |
Physics
Nuclear and High Energy Physics Radiation Astrophysics::High Energy Astrophysical Phenomena Time evolution Astrophysics Plasma Laser Computational physics law.invention symbols.namesake Mach number Physics::Plasma Physics law Physics::Space Physics symbols Merge (version control) Astrophysics::Galaxy Astrophysics |
| Zdroj: | High Energy Density Physics. 9:222-225 |
| ISSN: | 1574-1818 |
| DOI: | 10.1016/j.hedp.2013.01.001 |
| Popis: | Long time evolution of collisionless shocks in laser-produced plasmas is discussed. By irradiating a double plane target a high Mach number collisionless shock has been observed in laser produced counterstreaming plasmas [Kuramitsu et al., Phys. Rev. Lett., 106, 175002 (2011)]. While in early time we observe the shock in front of one plane, which is irradiated with the laser, we observe another shock in front of the other plane in much later time than the first shock formation. These two shocks coexist and collide or merge with each other as time passes. This means that the upstream plasmas for the first and second shocks have to be provided from the second and first shock sides, respectively, i.e., both the first and second shock have to be collisionless. There are two major candidates to account for the long time evolution of the collisionless shocks. One is that the secondary plasmas at the planes can be continuously created by the plasmas from the other planes. Another is that the actual shock thickness is much thiner than the detection limit, as indicated by numerical simulations. |
| Databáze: | OpenAIRE |
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