2017
DOI: 10.1063/1.4975310
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Formation of collisionless shocks in magnetized plasma interaction with kinetic-scale obstacles

Abstract: This version is available at https://strathprints.strath.ac.uk/60508/ Strathprints is designed to allow users to access the research output of the University of Strathclyde. Unless otherwise explicitly stated on the manuscript, Copyright © and Moral Rights for the papers on this site are retained by the individual authors and/or other copyright owners. Please check the manuscript for details of any other licences that may have been applied. You may not engage in further distribution of the material for any pro… Show more

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Cited by 18 publications
(18 citation statements)
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“…OSIRIS simulation results indicate, in agreement with our previous FLASH simulations, that as the plasma impacts the sphere (of typical size larger than the ion Larmor radius), a bow shock develops [23]. The counterpropagating ion flow is unstable and excites plasma waves in the lower-hybrid range ahead of the shock front (see Figure 4).…”
Section: Fig 2 Optical Data and Radiation-hydrodynamicsupporting
confidence: 88%
“…OSIRIS simulation results indicate, in agreement with our previous FLASH simulations, that as the plasma impacts the sphere (of typical size larger than the ion Larmor radius), a bow shock develops [23]. The counterpropagating ion flow is unstable and excites plasma waves in the lower-hybrid range ahead of the shock front (see Figure 4).…”
Section: Fig 2 Optical Data and Radiation-hydrodynamicsupporting
confidence: 88%
“…Future work will utilize thousands of shots to correlate fluctuations in the magnetic and electric fields and determine the instability growth rate [28] . Kinetic-scale magnetospheres are also possible to explore by coupling the laser plasma with an ion-scale ( ) magnetic dipole field [29] . Of particular interest is the dynamics and 3D structure of the interaction between a super-Alfvénic flow and the dipole field, which can be mapped out at high resolution over thousands of shots.…”
Section: Discussionmentioning
confidence: 99%
“…The computational investigation into mini-magnetospheres has become an area of considerable interest. A number of papers on hybrid (Bamford et al 2008;Gargaté et al 2008;Kallio et al 2012;Poppe et al 2012) and particle-in-cell (PIC) (Kallio et al 2012;Bamford et al 2013aBamford et al , 2013bBamford et al , 2015Deca et al 2014Deca et al , 2015Jarvinen et al 2014;Cruz et al 2015Cruz et al , 2016Dyadechkin et al 2015;Fatemi et al 2015) simulations have been authored, following from previous magnetohydrodynamic (MHD) simulations (Harnett & Winglee 2002Kurata et al 2005). Here we perform fully self-consistent PIC simulations in 2D and 3D, with a realistic proton-to-electron mass ratio.…”
Section: Introductionmentioning
confidence: 99%