The Effect of Spatial Resolution on the Wang–Sheeley–Arge Model Unsigned Open Flux Prediction
The open solar magnetic field refers to field lines that are magnetically connected to the surface of the Sun at one end and continue through the corona into the heliosphere. The open magnetic flux problem is the discrepancy between the total unsigned open magnetic flux determined using in situ meas...
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| Autori principali: | , , , , , |
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| Natura: | Artigo |
| Lingua: | Inglês |
| Pubblicazione: |
IOP Publishing
2026-01-01
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| Serie: | The Astrophysical Journal |
| Soggetti: | |
| Accesso online: | https://doi.org/10.3847/1538-4357/ae45a0 |
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