activity
19982024
most citedSolar Coronal Jets: Observations, Theory, and Modeling

361 citations · 514 across the 5 of their papers we have counts for

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Showing astro-ph.SRShow all

8 papers · 1 filter

astro-ph.SR2024

A Model for Flux Rope Formation and Disconnection in Pseudostreamer Coronal Mass Ejections

P. F. Wyper, B. J. Lynch, C. R. DeVore +3

Coronal mass ejections (CMEs) from pseudostreamers represent a significant fraction of large-scale eruptions from the Sun. In some cases, these CMEs take a narrow jet-like form rem…

astro-ph.SR202043 cited

Plumelets: Dynamic Filamentary Structures in Solar Coronal Plumes

V. M. Uritsky, C. E. DeForest, J. T. Karpen +4

Solar coronal plumes long seemed to possess a simple geometry supporting spatially coherent, stable outflow without significant fine structure. Recent high-resolution observations…

astro-ph.SR201945 cited

Escape of Flare-accelerated Particles in Solar Eruptive Events

S. Masson, S. K. Antiochos, C. R. DeVore

Impulsive solar energetic particle events are widely believed to be due to the prompt escape into the interplanetary medium of flare-accelerated particles produced by solar eruptiv…

astro-ph.SR2019

Numerical Simulation of Helical Jets at Active Region Peripheries

Peter F. Wyper, C. Richard DeVore, Spiro K. Antiochos

Coronal jets are observed above minority polarity intrusions throughout the solar corona. Some of the most energetic occur on the periphery of active regions where the magnetic fie…

astro-ph.SR2019

Modeling a Carrington-scale Stellar Superflare and Coronal Mass Ejection from

Benjamin J. Lynch, Vladimir S. Airapetian, C. Richard DeVore +5

Observations from the Kepler mission have revealed frequent superflares on young and active solar-like stars. Superflares result from the large-scale restructuring of stellar magne…

astro-ph.SR201965 cited

Multiwavelength Study of Equatorial Coronal-Hole Jets

Pankaj Kumar, Judith T. Karpen, Spiro K. Antiochos +3

Jets (transient/collimated plasma ejections) occur frequently throughout the solar corona and contribute mass/energy to the corona and solar wind. By combining numerical simulation…