Axial Flux Evolution of Small-scale Magnetic Flux Ropes from 0.06 to 10 au
Small-scale magnetic flux ropes (SMFRs) fill much of the solar wind, but their origin and evolution are debated. We apply our recently developed, improved Grad–Shafranov algorithm for the detection and reconstruction of SMFRs to data from Parker Solar Probe, Solar Orbiter, Wind, and Voyager 1 and 2...
| Main Authors: | , , , , |
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| 格式: | 文件 |
| 语言: | English |
| 出版: |
IOP Publishing
2024-01-01
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| 丛编: | The Astrophysical Journal Letters |
| 主题: | |
| 在线阅读: | https://doi.org/10.3847/2041-8213/ad3964 |