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Ehret M, Kochetkov Y, Abe Y, Law KFF, Bukharskii N, Stepanischev V, Fujioka S, d'Humières E, Zielbauer B, Bagnoud V, Schaumann G, Somekawa T, Roth M, Tikhonchuk V, Santos JJ, Korneev P. Kilotesla plasmoid formation by a trapped relativistic laser beam. Phys Rev E 2022; 106:045211. [PMID: 36397600 DOI: 10.1103/physreve.106.045211] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 09/17/2019] [Accepted: 10/04/2022] [Indexed: 06/16/2023]
Abstract
A strong quasistationary magnetic field is generated in hollow targets with curved internal surface under the action of a relativistically intense picosecond laser pulse. Experimental data evidence the formation of quasistationary strongly magnetized plasma structures decaying on a hundred picoseconds timescale, with the magnetic field strength of the kilotesla scale. Numerical simulations unravel the importance of transient processes during the magnetic field generation and suggest the existence of fast and slow regimes of plasmoid evolution depending on the interaction parameters. The proposed setup is suited for perspective highly magnetized plasma application and fundamental studies.
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Affiliation(s)
- M Ehret
- Université de Bordeaux, CNRS, CEA, Centre Lasers Intenses et Applications (CELIA), UMR 5107, Talence, France
- Institut für Kernphysik, Technische Universität Darmstadt, Darmstadt, Germany
| | - Yu Kochetkov
- National Research Nuclear University MEPhI, Moscow, Russian Federation
| | - Y Abe
- Graduate School of Engineering, Osaka University, Japan
- Institute of Laser Engineering, Osaka University, Japan
| | - K F F Law
- Institute of Laser Engineering, Osaka University, Japan
| | - N Bukharskii
- National Research Nuclear University MEPhI, Moscow, Russian Federation
| | - V Stepanischev
- National Research Nuclear University MEPhI, Moscow, Russian Federation
| | - S Fujioka
- Institute of Laser Engineering, Osaka University, Japan
| | - E d'Humières
- Université de Bordeaux, CNRS, CEA, Centre Lasers Intenses et Applications (CELIA), UMR 5107, Talence, France
| | - B Zielbauer
- Plasma Physik/PHELIX, GSI Helmholtzzentrum für Schwerionenforschung GmbH, Darmstadt, Germany
| | - V Bagnoud
- Plasma Physik/PHELIX, GSI Helmholtzzentrum für Schwerionenforschung GmbH, Darmstadt, Germany
| | - G Schaumann
- Institut für Kernphysik, Technische Universität Darmstadt, Darmstadt, Germany
| | - T Somekawa
- Institute of Laser Engineering, Osaka University, Japan
- Institute for Laser Technology, 1-8-4 Utsubohonmachi, Osaka 550-0004, Japan
| | - M Roth
- Institut für Kernphysik, Technische Universität Darmstadt, Darmstadt, Germany
| | - V Tikhonchuk
- Université de Bordeaux, CNRS, CEA, Centre Lasers Intenses et Applications (CELIA), UMR 5107, Talence, France
- ELI-Beamlines, Institute of Physics Academy of Sciences of the Czech Republic, Dolní Břežany, Czech Republic
| | - J J Santos
- Université de Bordeaux, CNRS, CEA, Centre Lasers Intenses et Applications (CELIA), UMR 5107, Talence, France
| | - Ph Korneev
- National Research Nuclear University MEPhI, Moscow, Russian Federation
- P. N. Lebedev Physical Institute of RAS, Moscow, Russian Federation
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Observation of an evolving magnetic flux rope before and during a solar eruption. Nat Commun 2012; 3:747. [PMID: 22434190 DOI: 10.1038/ncomms1753] [Citation(s) in RCA: 209] [Impact Index Per Article: 16.1] [Reference Citation Analysis] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 10/31/2011] [Accepted: 02/16/2012] [Indexed: 11/08/2022] Open
Abstract
Explosive energy release is a common phenomenon occurring in magnetized plasma systems ranging from laboratories, Earth's magnetosphere, the solar corona and astrophysical environments. Its physical explanation is usually attributed to magnetic reconnection in a thin current sheet. Here we report the important role of magnetic flux rope structure, a volumetric current channel, in producing explosive events. The flux rope is observed as a hot channel before and during a solar eruption from the Atmospheric Imaging Assembly telescope on board the Solar Dynamic Observatory. It initially appears as a twisted and writhed sigmoidal structure with a temperature as high as 10 MK, and then transforms toward a semi-circular shape during a slow-rise phase, which is followed by fast acceleration and onset of a flare. The observations suggest that the instability of the magnetic flux rope triggers the eruption, thus making a major addition to the traditional magnetic-reconnection paradigm.
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Binderbauer MW, Guo HY, Tuszewski M, Putvinski S, Sevier L, Barnes D, Rostoker N, Anderson MG, Andow R, Bonelli L, Brandi F, Brown R, Bui DQ, Bystritskii V, Ceccherini F, Clary R, Cheung AH, Conroy KD, Deng BH, Dettrick SA, Douglass JD, Feng P, Galeotti L, Garate E, Giammanco F, Glass FJ, Gornostaeva O, Gota H, Gupta D, Gupta S, Kinley JS, Knapp K, Korepanov S, Hollins M, Isakov I, Jose VA, Li XL, Luo Y, Marsili P, Mendoza R, Meekins M, Mok Y, Necas A, Paganini E, Pegoraro F, Pousa-Hijos R, Primavera S, Ruskov E, Qerushi A, Schmitz L, Schroeder JH, Sibley A, Smirnov A, Song Y, Sun X, Thompson MC, Van Drie AD, Walters JK, Wyman MD. Dynamic formation of a hot field reversed configuration with improved confinement by supersonic merging of two colliding high-β compact toroids. PHYSICAL REVIEW LETTERS 2010; 105:045003. [PMID: 20867853 DOI: 10.1103/physrevlett.105.045003] [Citation(s) in RCA: 12] [Impact Index Per Article: 0.8] [Reference Citation Analysis] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 01/25/2010] [Indexed: 05/29/2023]
Abstract
A hot stable field-reversed configuration (FRC) has been produced in the C-2 experiment by colliding and merging two high-β plasmoids preformed by the dynamic version of field-reversed θ-pinch technology. The merging process exhibits the highest poloidal flux amplification obtained in a magnetic confinement system (over tenfold increase). Most of the kinetic energy is converted into thermal energy with total temperature (T{i}+T{e}) exceeding 0.5 keV. The final FRC state exhibits a record FRC lifetime with flux confinement approaching classical values. These findings should have significant implications for fusion research and the physics of magnetic reconnection.
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Affiliation(s)
- M W Binderbauer
- Tri Alpha Energy, Inc., Post Office Box 7010, Rancho Santa Margarita, California 92688, USA
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