3 papers
astro-ph.SR2011
Morphology, dynamics and plasma parameters of plumes and inter-plume regions in solar coronal holes
K. Wilhelm, L. Abbo, F. Auchere +12
Coronal plumes, which extend from solar coronal holes (CH) into the high corona and - possibly - into the solar wind (SW), can now continuously be studied with modern telescopes an…
astro-ph.SR2010
Ultraviolet Coronagraph Spectroscopy: A Key Capability for Understanding the Physics of Solar Wind Acceleration
S. R. Cranmer, J. L. Kohl, D. Alexander +21
Understanding the physical processes responsible for accelerating the solar wind requires detailed measurements of the collisionless plasma in the extended solar corona. Some key c…
astro-ph.SR2009
Morphology and density of post-CME current sheets
B. Vršnak, G. Poletto, E. Vujić +11
Eruption of a coronal mass ejection (CME) drags and "opens" the coronal magnetic field, presumably leading to the formation of a large-scale current sheet and the field relaxation…