Turbulence, Energy Transfers and Reconnection in Compressible Coronal Heating Field-line Tangling Models. Dahlburg, R., Rappazzo, A., & Velli, M. Twelfth International Solar Wind Conference, 1216:40-43, March, 2010. doi bibtex @ARTICLE{2010AIPC.1216...40D,
author = {{Dahlburg}, R.~B. and {Rappazzo}, A.~F. and {Velli}, M.},
title = "{Turbulence, Energy Transfers and Reconnection in Compressible Coronal Heating Field-line Tangling Models}",
journal = {Twelfth International Solar Wind Conference},
archivePrefix = "arXiv",
eprint = {0912.1063},
primaryClass = "astro-ph.SR",
keywords = {magnetohydrodynamics, turbulence, solar corona, magnetic fields, Magnetohydrodynamics and plasmas, Convection turbulence and diffusion, Coronal loops streamers, Interplanetary magnetic fields},
year = 2010,
month = mar,
volume = 1216,
pages = {40-43},
doi = {10.1063/1.3395890},
adsurl = {http://adsabs.harvard.edu/abs/2010AIPC.1216...40D},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
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