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Coronal Holes and Open Magnetic Flux over Cycles 23 and 24
As the observational signature of the footprints of solar magnetic field lines open into the heliosphere, coronal holes provide a critical measure of the structure and evolution of these lines. Using a combination of Solar and Heliospheric Observatory/Extreme ultraviolet Imaging Telescope (SOHO/EIT)...
| Autores principales: | , , |
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| Formato: | Online Artículo Texto |
| Lenguaje: | English |
| Publicado: |
Springer Netherlands
2016
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| Acceso en línea: | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC7175679/ https://www.ncbi.nlm.nih.gov/pubmed/32355367 http://dx.doi.org/10.1007/s11207-016-1041-8 |