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Reconnection-Driven Magnetohydrodynamic Turbulence in a Simulated Coronal-Hole Jet
Extreme-ultraviolet and X-ray jets occur frequently in magnetically open coronal holes on the Sun, especially at high solar latitudes. Some of these jets are observed by white-light coronagraphs as they propagate through the outer corona toward the inner heliosphere, and it has been proposed that th...
שמור ב:
| הוצא לאור ב: | Astrophys J |
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| Main Authors: | , , , |
| פורמט: | Artigo |
| שפה: | Inglês |
| יצא לאור: |
2017
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| נושאים: | |
| גישה מקוונת: | https://ncbi.nlm.nih.gov/pmc/articles/PMC5799884/ https://ncbi.nlm.nih.gov/pubmed/29430025 https://ncbi.nlm.nih.govhttp://dx.doi.org/10.3847/1538-4357/aa5cb9 |
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