{"title":"实现逼真的太阳耀斑模型:DISPATCH 框架中的显式粒子单元求解器","authors":"Michael Haahr, Boris V. Gudiksen, Åke Nordlund","doi":"arxiv-2409.02493","DOIUrl":null,"url":null,"abstract":"Context. Simulating solar flares, which involve large-scale dynamics and\nsmall-scale magnetic reconnection, poses significant computational challenges.\nAims. This study aims to develop an explicit Particle-In-Cell (PIC) solver\nwithin the DISPATCH framework to model the small-scale kinetic processes in\nsolar corona setting. This study in the first in a series with the ultimate\ngoal to develop a hybrid PIC-MHD solver, to simulate solar flares. Methods. The\nPIC solver, inspired by the PhotonPlasma code, solves the Vlasov-Maxwell\nequations in a collisionless regime using explicit time-staggering and\nspatial-staggering techniques. Validation included unit tests, plasma frequency\nrecovery, two-stream instability, and current sheet dynamics. Results.\nValidation tests confirmed the solver's accuracy and robustness in modeling\nplasma dynamics and electromagnetic fields. Conclusions. The integration of the\nexplicit PIC solver into the DISPATCH framework is the first step towards\nbridging the gap between large and small scale dynamics, providing a robust\nplatform for future solar physics research.","PeriodicalId":501423,"journal":{"name":"arXiv - PHYS - Space Physics","volume":"17 1","pages":""},"PeriodicalIF":0.0000,"publicationDate":"2024-09-04","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"Toward Realistic Solar Flare Models: An explicit Particle-In-Cell solver in the DISPATCH framework\",\"authors\":\"Michael Haahr, Boris V. Gudiksen, Åke Nordlund\",\"doi\":\"arxiv-2409.02493\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"Context. Simulating solar flares, which involve large-scale dynamics and\\nsmall-scale magnetic reconnection, poses significant computational challenges.\\nAims. This study aims to develop an explicit Particle-In-Cell (PIC) solver\\nwithin the DISPATCH framework to model the small-scale kinetic processes in\\nsolar corona setting. This study in the first in a series with the ultimate\\ngoal to develop a hybrid PIC-MHD solver, to simulate solar flares. Methods. The\\nPIC solver, inspired by the PhotonPlasma code, solves the Vlasov-Maxwell\\nequations in a collisionless regime using explicit time-staggering and\\nspatial-staggering techniques. Validation included unit tests, plasma frequency\\nrecovery, two-stream instability, and current sheet dynamics. Results.\\nValidation tests confirmed the solver's accuracy and robustness in modeling\\nplasma dynamics and electromagnetic fields. Conclusions. The integration of the\\nexplicit PIC solver into the DISPATCH framework is the first step towards\\nbridging the gap between large and small scale dynamics, providing a robust\\nplatform for future solar physics research.\",\"PeriodicalId\":501423,\"journal\":{\"name\":\"arXiv - PHYS - Space Physics\",\"volume\":\"17 1\",\"pages\":\"\"},\"PeriodicalIF\":0.0000,\"publicationDate\":\"2024-09-04\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"arXiv - PHYS - Space Physics\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://doi.org/arxiv-2409.02493\",\"RegionNum\":0,\"RegionCategory\":null,\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"\",\"JCRName\":\"\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"arXiv - PHYS - Space Physics","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/arxiv-2409.02493","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
Toward Realistic Solar Flare Models: An explicit Particle-In-Cell solver in the DISPATCH framework
Context. Simulating solar flares, which involve large-scale dynamics and
small-scale magnetic reconnection, poses significant computational challenges.
Aims. This study aims to develop an explicit Particle-In-Cell (PIC) solver
within the DISPATCH framework to model the small-scale kinetic processes in
solar corona setting. This study in the first in a series with the ultimate
goal to develop a hybrid PIC-MHD solver, to simulate solar flares. Methods. The
PIC solver, inspired by the PhotonPlasma code, solves the Vlasov-Maxwell
equations in a collisionless regime using explicit time-staggering and
spatial-staggering techniques. Validation included unit tests, plasma frequency
recovery, two-stream instability, and current sheet dynamics. Results.
Validation tests confirmed the solver's accuracy and robustness in modeling
plasma dynamics and electromagnetic fields. Conclusions. The integration of the
explicit PIC solver into the DISPATCH framework is the first step towards
bridging the gap between large and small scale dynamics, providing a robust
platform for future solar physics research.