activity
20072026
most citedPhysics of Solar Prominences: II - Magnetic Structure and Dynamics

631 citations · 2.2k across the 44 of their papers we have counts for

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Showing 2016Show all

6 papers · 1 filter

astro-ph.SR2016★ 74 cited

A model for straight and helical solar jets: II. Parametric study of the plasma beta

E. Pariat, K. Dalmasse, C. R. DeVore +2

Jets are dynamic, impulsive, well-collimated plasma events that develop at many different scales and in different layers of the solar atmosphere. Jets are believed to be induced by…

astro-ph.SR2016★ 24 cited

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…

astro-ph.SR2016★ 10 cited

The effects of magnetic-field geometry on longitudinal oscillations of solar prominences: Cross-sectional area variation for thin tubes

M. Luna, A. J. Diaz, R. Oliver +2

Solar prominences are subject to both field-aligned (longitudinal) and transverse oscillatory motions, as evidenced by an increasing number of observations. Large-amplitude longitu…

astro-ph.SR2016★ 92 cited

Three-Dimensional Simulations of Tearing and Intermittency in Coronal Jets

P. F. Wyper, C. R. DeVore, J. T. Karpen +1

Observations of coronal jets increasingly suggest that local fragmentation and intermittency play an important role in the dynamics of these events. In this work we investigate thi…

astro-ph.SR2016★ 63 cited

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…

astro-ph.SR2016★ 72 cited

Magnetic-Island Contraction and Particle Acceleration in Simulated Eruptive Solar Flares

S. E. Guidoni, C. R. DeVore, J. T. Karpen +1

The mechanism that accelerates particles to the energies required to produce the observed high-energy impulsive emission in solar flares is not well understood. Drake et al. (2006)…