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The Current-Free Electric Double Layer in a Coronal Magnetic Funnel
Author(s) -
R. W. Boswell,
E. Marsch,
Christine Charles
Publication year - 2006
Publication title -
the astrophysical journal
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.376
H-Index - 489
eISSN - 1538-4357
pISSN - 0004-637X
DOI - 10.1086/503155
Subject(s) - physics , funnel , magnetic field , plasma , corona (planetary geology) , nanoflares , coronal hole , astrophysics , computational physics , solar wind , coronal mass ejection , nuclear physics , astrobiology , chemistry , organic chemistry , quantum mechanics , venus
Current-free double layers (CFDLs) have been recently discovered in a number of laboratory devices, when a low collisional plasma is forced to expand from a high magnetic field source region to a low magnetic field diffusion region. This experimental setup bears a striking resemblance to the natural conditions prevailing in the magnetic funnels of the solar corona. It was commonly thought that magnetic-field-aligned potential disruptions were driven by electron currents, although the theoretical possibility of a CDFL has been known of for some time. Given its recent experimental verification, we make here a contribution to solar plasma physics by inves- tigating the possibility of CFDLs in coronal funnels, which have much in common with the laboratory experiments. Therefore, CFDLs may play an important role in supplying and accelerating plasma in coronal funnels.

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