Author:
Riley P.,Lionello R.,Linker J. A.,Mikic Z.,Luhmann J.,Wijaya J.
Publisher
Springer Science and Business Media LLC
Subject
Space and Planetary Science,Astronomy and Astrophysics
Reference57 articles.
1. Athay, R.G.: 1986, Radiation loss rates in Lyman-alpha for solar conditions. Astrophys. J. 308, 975 – 981. doi: 10.1086/164565 .
2. Buchlin, E., Velli, M.: 2007, Shell models of RMHD turbulence and the heating of solar coronal loops. Astrophys. J. 662, 701 – 714. doi: 10.1086/512765 .
3. Cranmer, S.R.: 2010, An efficient approximation of the coronal heating rate for use in global Sun-heliosphere simulations. Astrophys. J. Lett. 710, L676 – L688. doi: 10.1088/0004-637X/710/1/676 .
4. Cranmer, S.R., van Ballegooijen, A.A., Edgar, R.J.: 2007, Self-consistent coronal heating and solar wind acceleration from anisotropic magnetohydrodynamic turbulence. Astrophys. J. Suppl. Ser. 171, 520 – 551. doi: 10.1086/518001 .
5. Cranmer, S.R., Kohl, J.L., Miralles, M.P., van Ballegooijen, A.A.: 2010, Extended coronal heating and solar wind acceleration over the solar cycle. In: Cranmer, S.R., Hoeksema, J.T., Kohl, J.L. (eds.) SOHO-23: Understanding a Peculiar Solar Minimum CS-428, Astron. Soc. Pacific, San Francisco, 209.
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