Most fundamental radio emission from beam-generated turbulence in Type III sources is trapped Z-mode; the small escaping fraction is mainly O-mode, with X-mode only in weakly magnetized sources.
SMILEI: a collaborative, open-source, multi-purpose particle-in-cell code for plasma simulation
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abstract
SMILEI is a collaborative, open-source, object-oriented (C++) particle-in-cell code. To benefit from the latest advances in high-performance computing (HPC), SMILEI is co-developed by both physicists and HPC experts. The code's structures, capabilities, parallelization strategy and performances are discussed. Additional modules (e.g. to treat ionization or collisions), benchmarks and physics highlights are also presented. Multi-purpose and evolutive, SMILEI is applied today to a wide range of physics studies, from relativistic laser-plasma interaction to astrophysical plasmas.
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astro-ph.SR 1years
2025 1verdicts
CONDITIONAL 1representative citing papers
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Electromagnetic radiation by turbulent, magnetized and randomly inhomogeneous solar radio sources generated by electron beams
Most fundamental radio emission from beam-generated turbulence in Type III sources is trapped Z-mode; the small escaping fraction is mainly O-mode, with X-mode only in weakly magnetized sources.