By Steven Tomczyk, Jie Zhang, Timothy Bastian
Captures advances being made within the box of coronal magnetism, from idea to observations and instrumentation.
This quantity is a set of analysis articles just about the sunlight corona, and especially, coronal magnetism. The e-book was once stimulated by means of the Workshop on Coronal Magnetism: Connecting versions to info and the Corona to the Earth, which was once held 21 - 23 may perhaps 2012 in Boulder, Colorado, united states. This workshop used to be attended via nearly 60 researchers. Articles from this assembly are contained during this topical factor, however the topical factor additionally comprises contributions from researchers no longer current on the workshop.
This quantity is aimed toward researchers and graduate scholars lively in sun physics.
Originally released in Solar Physics, Vol. 288, factor 2, 2013 and Vol. 289, factor eight, 2014.
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303, 927. : 1996, Solar Phys. 168, 115. 1007/BF00145829. : 2008, Solar Phys. 251, 613. 1007/s11207008-9122-y. : 2009, Astrophys. J. 700, 559. 1088/0004-637X/ 700/1/559. : 1994, Astrophys. J. 422, 899. 1086/173781. : 2008, Solar Phys. 247, 269. 1007/s11207-007-9110-7. : 2012, Solar Phys. 278, 149. 1007/s11207011-9924-1. : 2011, Solar Phys. 272, 29. 1007/ s11207-011-9809-3.
In this modelling, the magnetic field in the quiet Sun has been decomposed into two components: i) closed field lines, which characterise the complexity of the magnetic field (below several hundreds of kilometre according to Régnier, Parnell, and Haynes, 2008) and are linked to granule’s boundary and part of supergranular field, ii) open field lines (“open” meaning leaving the box of computation), which is often considered as the source of the solar wind. The amount of open flux has been measured at different height showing that a small amount of the photospheric magnetic flux is open above few megameters.
2010, Astron. Astrophys. 522, 52. 1051/0004-6361/200913058. : 2006, Astron. Astrophys. 446, 691. 1051/0004-6361: 20054076. : 1998, Astron. Astrophys. 339, 252. : 1999, Astron. Astrophys. 350, 1051. : 1997, Solar Phys. 174, 129. : 1987, Astrophys. J. 312, 886. 1086/164935. : 2006, Astron. Astrophys. 454, 957. 1051/0004-6361:20064953. : 2005, Solar Phys. 228, 339. 1007/s11207-005-2788-5. : 2012a, Solar Phys. 1007/s11207-012-0069-7. : 2012b, Solar Phys. 1007/s11207-012-0203-6. : 2013, Astrophys.