Using Coronal Cells to Infer the Magnetic Field Structure and Chirality of Filament Channels. Sheeley, Martin, S., Panasenco, O., & Warren, H. \apj, 772:88, August, 2013. doi bibtex @ARTICLE{2013ApJ...772...88S,
author = {{Sheeley}, Jr., N.~R. and {Martin}, S.~F. and {Panasenco}, O. and
{Warren}, H.~P.},
title = "{Using Coronal Cells to Infer the Magnetic Field Structure and Chirality of Filament Channels}",
journal = {\apj},
archivePrefix = "arXiv",
eprint = {1306.2273},
primaryClass = "astro-ph.SR",
keywords = {magnetic fields, Sun: corona, Sun: filaments, prominences, Sun: UV radiation },
year = 2013,
month = aug,
volume = 772,
eid = {88},
pages = {88},
doi = {10.1088/0004-637X/772/2/88},
adsurl = {http://adsabs.harvard.edu/abs/2013ApJ...772...88S},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
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