Coronal Magnetic Field Topology from Total Solar Eclipse Observations

Measuring the global magnetic field of the solar corona remains exceptionally challenging. The fine-scale density structures observed in white-light images taken during total solar eclipses are currently the best proxies for inferring the magnetic field direction in the corona from the solar limb ou...

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Veröffentlicht in:	The Astrophysical journal 2020-06, Vol.895 (2), p.123
Hauptverfasser:	Boe, Benjamin, Habbal, Shadia, Druckmüller, Miloslav
Format:	Artikel
Sprache:	eng
Schlagworte:	Astrophysics Corona Coronal holes Coronal magnetic fields Hough transformation Magnetic fields Photosphere Solar corona Solar coronal holes Solar coronal plumes Solar coronal streamers Solar cycle Solar eclipses Solar limb Solar magnetic field Solar magnetic fields Solar optical telescopes Solar physics Solar surface Solar wind Topology White light Wind measurement
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