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Dynamics of Coronal-Hole Boundaries
A. K. Higginson, S. K. Antiochos, C. R. DeVore +2
Remote and in-situ observations strongly imply that the slow solar wind consists of plasma from the hot, closed-field corona that is released onto open magnetic field lines. The Se…
The Role of Magnetic Helicity in Structuring the Solar Corona
Kalman J. Knizhnik, Spiro K. Antiochos, C. Richard DeVore
Two of the most widely observed and yet most puzzling features of the Sun's magnetic field are coronal loops that are smooth and laminar and prominences/filaments that are strongly…
Reconnection-Driven Magnetohydrodynamic Turbulence in a Simulated Coronal-Hole Jet
Vadim M. Uritsky, Merrill A. Roberts, C. Richard DeVore +1
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-ligh…
Reconnection-Driven Coronal-Hole Jets with Gravity and Solar Wind
J. T. Karpen, C. R. DeVore, S. K. Antiochos +1
Coronal-hole jets occur ubiquitously in solar coronal holes, at EUV and X-ray bright points associated with intrusions of minority magnetic polarity. The embedded-bipole model for…