Simulation Models for Exploring Magnetic Reconnection
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arXiv
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| Auteurs principaux: | , , , , , , , , , , , , , , , , , , , , , , , , |
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| Format: | Preprint |
| Publié: |
2024
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| _version_ | 1866916281480904704 |
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| author | Shay, Michael Adhikari, Subash Beesho, Naoki Birn, Joachim Buechner, Jorg Cassak, Paul Chen, Li-Jen Chen, Yuxi Cozzani, Giulia Drake, Jim Guo, Fan Hesse, Michael Jain, Neeraj Pfau-Kempf, Yann Lin, Yu Liu, Yi-Hsin Oka, Mitsuo Omelchenko, Yuri A. Palmroth, Minna Pezzi, Oreste Reiff, Patricia H. Swisdak, Marc Toffoletto, Frank Toth, Gabor Wolf, Richard A. |
| author_facet | Shay, Michael Adhikari, Subash Beesho, Naoki Birn, Joachim Buechner, Jorg Cassak, Paul Chen, Li-Jen Chen, Yuxi Cozzani, Giulia Drake, Jim Guo, Fan Hesse, Michael Jain, Neeraj Pfau-Kempf, Yann Lin, Yu Liu, Yi-Hsin Oka, Mitsuo Omelchenko, Yuri A. Palmroth, Minna Pezzi, Oreste Reiff, Patricia H. Swisdak, Marc Toffoletto, Frank Toth, Gabor Wolf, Richard A. |
| contents | Simulations have played a critical role in the advancement of our knowledge of magnetic reconnection. However, due to the inherently multiscale nature of reconnection, it is impossible to simulate all physics at all scales. For this reason, a wide range of simulation methods have been crafted to study particular aspects and consequences of magnetic reconnection. This chapter reviews many of these methods, laying out critical assumptions, numerical techniques, and giving examples of scientific results. Plasma models described include magnetohydrodynamics (MHD), Hall MHD, Hybrid, kinetic particle-in-cell (PIC), kinetic Vlasov, Fluid models with embedded PIC, Fluid models with direct feedback from energetic populations, and the Rice Convection Model (RCM). |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2406_05901 |
| institution | arXiv |
| publishDate | 2024 |
| record_format | arxiv |
| spellingShingle | Simulation Models for Exploring Magnetic Reconnection Shay, Michael Adhikari, Subash Beesho, Naoki Birn, Joachim Buechner, Jorg Cassak, Paul Chen, Li-Jen Chen, Yuxi Cozzani, Giulia Drake, Jim Guo, Fan Hesse, Michael Jain, Neeraj Pfau-Kempf, Yann Lin, Yu Liu, Yi-Hsin Oka, Mitsuo Omelchenko, Yuri A. Palmroth, Minna Pezzi, Oreste Reiff, Patricia H. Swisdak, Marc Toffoletto, Frank Toth, Gabor Wolf, Richard A. Plasma Physics Solar and Stellar Astrophysics Space Physics Simulations have played a critical role in the advancement of our knowledge of magnetic reconnection. However, due to the inherently multiscale nature of reconnection, it is impossible to simulate all physics at all scales. For this reason, a wide range of simulation methods have been crafted to study particular aspects and consequences of magnetic reconnection. This chapter reviews many of these methods, laying out critical assumptions, numerical techniques, and giving examples of scientific results. Plasma models described include magnetohydrodynamics (MHD), Hall MHD, Hybrid, kinetic particle-in-cell (PIC), kinetic Vlasov, Fluid models with embedded PIC, Fluid models with direct feedback from energetic populations, and the Rice Convection Model (RCM). |
| title | Simulation Models for Exploring Magnetic Reconnection |
| topic | Plasma Physics Solar and Stellar Astrophysics Space Physics |
| url | https://arxiv.org/abs/2406.05901 |