Field Lines Twisting in a Noisy Corona: Implications for Energy Storage and Release, and Initiation of Solar Eruptions. Rappazzo, A., Velli, M., & Einaudi, G. \apj, 771:76, July, 2013. doi bibtex @ARTICLE{2013ApJ...771...76R,
author = {{Rappazzo}, A.~F. and {Velli}, M. and {Einaudi}, G.},
title = "{Field Lines Twisting in a Noisy Corona: Implications for Energy Storage and Release, and Initiation of Solar Eruptions}",
journal = {\apj},
archivePrefix = "arXiv",
eprint = {1301.7678},
primaryClass = "astro-ph.SR",
keywords = {magnetohydrodynamics: MHD, Sun: corona, Sun: coronal mass ejections: CMEs, Sun: magnetic topology, turbulence },
year = 2013,
month = jul,
volume = 771,
eid = {76},
pages = {76},
doi = {10.1088/0004-637X/771/2/76},
adsurl = {http://adsabs.harvard.edu/abs/2013ApJ...771...76R},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
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