Bak-Steslicka, U., Proceedings of the International Astronomical Union, 8, 395-396, doi:10.1017/S1743921313011253., , , B. Forland, and L. A. Rachmeler, 2014: The spatial relation between EUV cavities and linear polarization signatures.
|Title:||The spatial relation between EUV cavities and linear polarization signatures|
|Abstract:||Solar coronal cavities are regions of rarefied density and elliptical cross-section. The Coronal Multi-channel Polarimeter (CoMP) obtains daily full-Sun coronal observations in linear polarization, allowing a systematic analysis of the coronal magnetic field in polar-crown prominence cavities. These cavities commonly possess a characteristic “lagomorphic” signature in linear polarization that may be explained by a magnetic flux-rope model. We analyze the spatial relation between the EUV cavity and the CoMP linear polarization signature.|
|Copyright Information:||Copyright 2014 Cambridge University Press|
|OpenSky citable URL:||ark:/85065/d7ms3vhv|