2 papers
astro-ph.SR2020
CME Acceleration as a Probe of the Coronal Magnetic Field
James Paul Mason, Phillip C. Chamberlin, Thomas N. Woods +5
By 2050, we expect that CME models will accurately describe, and ideally predict, observed solar eruptions and the propagation of the CMEs through the corona. We describe some of t…
astro-ph.SR2019
Characteristics of ephemeral coronal holes
Andrew R. Inglis, Rachel E. O'Connor, W. Dean Pesnell +2
Small-scale ephemeral coronal holes may be a recurring feature on the solar disk, but have received comparatively little attention. These events are characterized by compact struct…