Magnetic Structures at the Boundary of the Closed Corona: Interpretation of S-Web Arcs

The topology of coronal magnetic fields near the open-closed magnetic flux boundary is important to the the process of interchange reconnection, whereby plasma is exchanged between open and closed flux domains. Maps of the magnetic squashing factor in coronal field models reveal the presence of the...

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Veröffentlicht in:	The Astrophysical journal 2018-12, Vol.869 (1), p.60
Hauptverfasser:	Scott, Roger B., Pontin, David I., Yeates, Anthony R., Wyper, Peter F., Higginson, Aleida K.
Format:	Artikel
Sprache:	eng
Schlagworte:	Acceleration Astrophysics Corona Coronal magnetic fields Current sheets Domains Energetic particles Fluctuations Heliosphere Heliospheric current sheet Magnetic fields Magnetic flux Magnetism Photosphere Protective equipment Solar energetic particles Solar wind Spine Sun: corona Topology Webs
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