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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...

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Bibliografiske detaljer
Udgivet i:Astrophys J
Main Authors: Uritsky, Vadim M., Roberts, Merrill A., DeVore, C. Richard, Karpen, Judith T.
Format: Artigo
Sprog:Inglês
Udgivet: 2017
Fag:
Online adgang: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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