Mildly relativistic magnetized shocks in electron–ion plasmas – I. Electromagnetic shock structure
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- Arianna Ligorini
- Institute of Nuclear Physics, Polish Academy of Sciences, PL-31342 Krakow, Poland
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- Jacek Niemiec
- Institute of Nuclear Physics, Polish Academy of Sciences, PL-31342 Krakow, Poland
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- Oleh Kobzar
- Astronomical Observatory of the Jagiellonian University, PL-30244 Krakow, Poland
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- Masanori Iwamoto
- Faculty of Engineering Sciences, Kyushu University, Kasuga, Fukuoka 816-8580, Japan
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- Artem Bohdan
- DESY, D-15738 Zeuthen, Germany
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- Martin Pohl
- DESY, D-15738 Zeuthen, Germany
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- Yosuke Matsumoto
- Department of Physics, Chiba University, 1-33 Yayoi, Inage-ku, Chiba 263-8522, Japan
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- Takanobu Amano
- Department of Earth and Planetary Science, University of Tokyo, 7-3-1 Hongo, Bunkyo-ku, Tokyo 113-0033, Japan
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- Shuichi Matsukiyo
- Faculty of Engineering Sciences, Kyushu University, Kasuga, Fukuoka 816-8580, Japan
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- Yodai Esaki
- Interdisciplinary Graduate School of Engineering Sciences, Kyushu University, Kasuga, Fukuoka 816-8580, Japan
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- Masahiro Hoshino
- Department of Earth and Planetary Science, University of Tokyo, 7-3-1 Hongo, Bunkyo-ku, Tokyo 113-0033, Japan
抄録
<jats:title>ABSTRACT</jats:title> <jats:p>Mildly relativistic shocks in magnetized electron–ion plasmas are investigated with 2D kinetic particle-in-cell simulations of unprecedentedly high resolution and large scale for conditions that may be found at internal shocks in blazar cores. Ion-scale effects cause corrugations along the shock surface whose properties somewhat depend on the configuration of the mean perpendicular magnetic field, that is either in or out of the simulation plane. We show that the synchrotron maser instability persists to operate in mildly relativistic shocks in agreement with theoretical predictions and produces coherent emission of upstream-propagating electromagnetic waves. Shock front ripples are excited in both mean-field configurations and they engender effective wave amplification. The interaction of these waves with upstream plasma generates electrostatic wakefields.</jats:p>
収録刊行物
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- Monthly Notices of the Royal Astronomical Society
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Monthly Notices of the Royal Astronomical Society 501 (4), 4837-4849, 2020-12-21
Oxford University Press (OUP)
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詳細情報 詳細情報について
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- CRID
- 1360290617823863168
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- ISSN
- 13652966
- 00358711
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- データソース種別
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- Crossref
- KAKEN