Self-generated Magnetic Fields in the Plasma Richtmyer-Meshkov Instability

V. Wheatley; Daryl Bond; Y. Li; Ravi Samtaney; D. I. Pullin

doi:10.1007/978-3-319-91020-8_77

Self-generated Magnetic Fields in the Plasma Richtmyer-Meshkov Instability

V. Wheatley, Daryl Bond, Y. Li, Ravi Samtaney, D. I. Pullin

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution

Abstract

Self-generated magnetic fields that arise in initially unmagnetized plasma during the ideal two-fluid plasma Richtmyer-Meshkov instability of a thermal interface are investigated computationally. These fields are of significant interest as they may adversely affect the coupling between the laser energy and the fuel in inertial confinement fusion implosions. We explore the mechanism by which these fields are generated and how their strength depends on the plasma parameters.

Original language	English (US)
Title of host publication	31st International Symposium on Shock Waves 1
Publisher	Springer Nature
Pages	653-660
Number of pages	8
ISBN (Print)	9783319910192
DOIs	https://doi.org/10.1007/978-3-319-91020-8_77
State	Published - Mar 22 2019

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title = "Self-generated Magnetic Fields in the Plasma Richtmyer-Meshkov Instability",

abstract = "Self-generated magnetic fields that arise in initially unmagnetized plasma during the ideal two-fluid plasma Richtmyer-Meshkov instability of a thermal interface are investigated computationally. These fields are of significant interest as they may adversely affect the coupling between the laser energy and the fuel in inertial confinement fusion implosions. We explore the mechanism by which these fields are generated and how their strength depends on the plasma parameters.",

author = "V. Wheatley and Daryl Bond and Y. Li and Ravi Samtaney and Pullin, {D. I.}",

note = "KAUST Repository Item: Exported on 2021-04-19 Acknowledged KAUST grant number(s): URF/1/2162-01 Acknowledgements: This research was supported by the KAUST Office of Sponsored Research under Award URF/1/2162-01. This work was supported by computational resources provided by the Australian Government under the National Computational Merit Allocation Scheme.",

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doi = "10.1007/978-3-319-91020-8_77",

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AU - Wheatley, V.

AU - Bond, Daryl

AU - Li, Y.

AU - Samtaney, Ravi

AU - Pullin, D. I.

N1 - KAUST Repository Item: Exported on 2021-04-19 Acknowledged KAUST grant number(s): URF/1/2162-01 Acknowledgements: This research was supported by the KAUST Office of Sponsored Research under Award URF/1/2162-01. This work was supported by computational resources provided by the Australian Government under the National Computational Merit Allocation Scheme.

PY - 2019/3/22

Y1 - 2019/3/22

N2 - Self-generated magnetic fields that arise in initially unmagnetized plasma during the ideal two-fluid plasma Richtmyer-Meshkov instability of a thermal interface are investigated computationally. These fields are of significant interest as they may adversely affect the coupling between the laser energy and the fuel in inertial confinement fusion implosions. We explore the mechanism by which these fields are generated and how their strength depends on the plasma parameters.

AB - Self-generated magnetic fields that arise in initially unmagnetized plasma during the ideal two-fluid plasma Richtmyer-Meshkov instability of a thermal interface are investigated computationally. These fields are of significant interest as they may adversely affect the coupling between the laser energy and the fuel in inertial confinement fusion implosions. We explore the mechanism by which these fields are generated and how their strength depends on the plasma parameters.

UR - http://hdl.handle.net/10754/668739

UR - http://link.springer.com/10.1007/978-3-319-91020-8_77

U2 - 10.1007/978-3-319-91020-8_77

DO - 10.1007/978-3-319-91020-8_77

M3 - Conference contribution

SN - 9783319910192

SP - 653

EP - 660

BT - 31st International Symposium on Shock Waves 1

PB - Springer Nature

ER -

Self-generated Magnetic Fields in the Plasma Richtmyer-Meshkov Instability

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