@inproceedings{258f57ce759040b99cf398d63c0950b3,
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.",
keywords = "Prominences, Sun: corona, Sun: filaments, Sun: infrared, Sun: magnetic field",
author = "Urszula B{\c a}k-Stȩ{\'s}licka and Gibson, \{Sarah E.\} and Yuhong Fan and Christian Bethge and Blake Forland and Rachmeler, \{Laurel A.\}",
year = "2013",
month = jun,
doi = "10.1017/S1743921313011253",
language = "English",
isbn = "9781107045194",
series = "Proceedings of the International Astronomical Union",
publisher = "Cambridge University Press",
number = "S300",
pages = "395--396",
booktitle = "Nature of Prominences and their Role in Space Weather",
address = "United Kingdom",
edition = "S300",
}