Simulation Models for Exploring Magnetic Reconnection
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| Titel: | Simulation Models for Exploring Magnetic Reconnection |
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| Autoren: | Shay, Michael, Adhikari, Subash, Beesho, Naoki, Birn, Joachim, Büchner, Jörg, Cassak, Paul, Chen, Li-Jen, Chen, Yuxi, Cozzani, Giulia, Drake, James, Guo, Fan, Hesse, Michael, Jain, Neeraj, Pfau-Kempf, Yann, Lin, Yu, Liu, Yi-Hsin, Oka, Mitsuo, Omelchenko, Yuri, Palmroth, Minna, Pezzi, Oreste, Reiff, Patricia H., Swisdak, Marc, Toffoletto, Frank, Toth, Gabor, Wolf, Richard A. |
| Weitere Verfasser: | Shay, Michael, Adhikari, Subash, Beesho, Naoki, Birn, Joachim, Büchner, Jörg, Cassak, Paul, Chen, Li-Jen, Chen, Yuxi, Cozzani, Giulia, Drake, James, Guo, Fan, Hesse, Michael, Jain, Neeraj, Pfau-Kempf, Yann, Lin, Yu, Liu, Yi-Hsin, Oka, Mitsuo, Omelchenko, Yuri, Palmroth, Minna, Pezzi, Oreste, Wolf, Richard A., POTHIER, Nathalie |
| Quelle: | Space Science Reviews. 221 |
| Publication Status: | Preprint |
| Verlagsinformationen: | Springer Science and Business Media LLC, 2025. |
| Publikationsjahr: | 2025 |
| Schlagwörter: | FOS: Physical sciences, Solar corona, 7. Clean energy, Physics - Plasma Physics, Space Physics (physics.space-ph), Plasma physics, Turbulence, [SDU] Sciences of the Universe [physics], Plasma Physics (physics.plasm-ph), Astrophysics - Solar and Stellar Astrophysics, Physics - Space Physics, Magnetosphere, Magnetic reconnection, Plasma simulation, Numerical methods, Solar and Stellar Astrophysics (astro-ph.SR) |
| Beschreibung: | 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 article 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). |
| Publikationsart: | Article |
| Dateibeschreibung: | application/pdf |
| Sprache: | English |
| ISSN: | 1572-9672 0038-6308 |
| DOI: | 10.1007/s11214-025-01210-5 |
| DOI: | 10.48550/arxiv.2406.05901 |
| Zugangs-URL: | http://arxiv.org/abs/2406.05901 https://resolver.sub.uni-goettingen.de/purl?gro-2/151811 https://insu.hal.science/insu-05281020v1/document https://insu.hal.science/insu-05281020v1 https://doi.org/10.1007/s11214-025-01210-5 |
| Rights: | CC BY arXiv Non-Exclusive Distribution |
| Dokumentencode: | edsair.doi.dedup.....5a184fdd86596b1142df236a29abc6fa |
| Datenbank: | OpenAIRE |
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Nájsť tento článok vo Web of Science | Abstract: | 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 article 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). |
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| ISSN: | 15729672 00386308 |
| DOI: | 10.1007/s11214-025-01210-5 |