Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
School of Mathematical and Computational Sciences, University of St. Andrews, St. Andrews, Fife KY16955, Scotland, UK
Erratum - Turbulent Coronal Heating
Formation of current layers in three-dimensional, inhomogeneous coronal magnetic fields by photospheric motions
Magnetic Null Points due to Multiple Sources of Solar Photospheric Flux
Turbulent coronal heating. I. Sheared arcade.
Turbulent coronal heating. II. Twisted flux tube.
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