29 citations · 83 across the 8 of their papers we have counts for
8 papers
Filament Mass Losses Forced by Magnetic Reconnection in the Solar Corona
Craig D. Johnston, Lars K. S. Daldorff, Peter W. Schuck +4
Recent observations of the solar atmosphere in cool extreme ultraviolet (EUV) lines have reported the prevalence of coronal rain falling from coronal cloud filaments that are assoc…
Synthetic Remote-sensing and In-situ Observations of Fine-scale Structure in a Pseudostreamer Coronal Mass Ejection through the Solar Corona
B. J. Lynch, P. F. Wyper, E. Palmerio +11
Coronal pseudostreamer flux systems have a specific magnetic configuration that influences the morphology and evolution of coronal mass ejections (CMEs) from these regions. Here we…
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…
The Thickness of Electric Current Sheets and Implications for Coronal Heating
James A. Klimchuk, James E. Leake, Lars K. S. Daldorff +1
The thickness of current sheets is extremely important, especially as it relates to the onset of fast magnetic reconnection. Onset determines how much magnetic free energy can buil…
Impact of 3D Structure on Magnetic Reconnection
Lars K. S. Daldorff, James E. Leake, James A. Klimchuk
Results from 2.5D and 3D studies of the onset and development of the tearing instability are presented, using high fidelity resistive MHD simulations. A limited parameter study of…
The Onset of 3D Magnetic Reconnection and Heating in the Solar Corona
James Leake, Lars Daldorff, James Klimchuk
Magnetic reconnection, a fundamentally important process in many aspects of astrophysics, is believed to be initiated by the tearing instability of an electric current sheet, a reg…