3 papers
astro-ph.SR2018
Global Non-Potential Magnetic Models of the Solar Corona During the March 2015 Eclipse
A. R. Yeates, T. Amari, I. Contopoulos +17
Seven different models are applied to the same problem of simulating the Sun's coronal magnetic field during the solar eclipse on 2015 March 20. All of the models are non-potential…
astro-ph.SR2018
First Empirical Determination of the Fe 10+ and Fe 13+ Freeze-in Distances in the Solar Corona
Benjamin Boe, Shadia Habbal, Miloslav Druckmuller +5
Heavy ions are markers of the physical processes responsible for the density and temperature distribution throughout the fine scale magnetic structures that define the shape of the…
physics.space-ph2016
Erupting filaments with large enclosing flux tubes as sources of high-mass 3-part CMEs, and erupting filaments in the absence of enclosing flux tubes as sources of low-mass unstructured CMEs
Joe Hutton, Huw Morgan
The 3-part appearance of many CMEs arising from erupting filaments emerges from a large magnetic flux tube structure, consistent with the form of the erupting filament system. Othe…