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EVIDENCE FOR THE MAGNETIC BREAKOUT MODEL IN AN EQUATORIAL CORONAL-HOLE JET

Small, impulsive jets commonly occur throughout the solar corona, but are especially visible in coronal holes. Evidence is mounting that jets are part of a continuum of eruptions that extends to much larger coronal mass ejections and eruptive flares. Because coronal-hole jets originate in relatively...

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Publicat a:Astrophys J
Autors principals: KUMAR, PANKAJ, KARPEN, JUDITH T., ANTIOCHOS, SPIRO K., WYPER, PETER F., DEVORE, C. RICHARD, DEFOREST, CRAIG E.
Format: Artigo
Idioma:Inglês
Publicat: 2018
Matèries:
Accés en línia:https://ncbi.nlm.nih.gov/pmc/articles/PMC8051205/
https://ncbi.nlm.nih.gov/pubmed/33867543
https://ncbi.nlm.nih.govhttp://dx.doi.org/10.3847/1538-4357/aaab4f
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