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Investigation of Thickness and Electrical Resistivity of the Current Sheets in Solar EruptionsA discussion of the thickness of current sheets in solar eruptions led Lin et al. in 2007 to estimate very large values for the effective resistivity. This paper addresses some questions raised by that paper. The limb synoptic map technique is applied to find the current sheet thickness to be between 5.OE4 and 4.6E5 km, increasing with both time and altitude. The possibility that large apparent values result from projection effects is examined and rejected. Theoretical scaling laws corroborate this conclusion.
Document ID
20090042334
Acquisition Source
Goddard Space Flight Center
Document Type
Reprint (Version printed in journal)
Authors
Lin, J.
(Harvard-Smithsonian Center for Astrophysics Cambridge, MA, United States)
Li, J.
(Harvard-Smithsonian Center for Astrophysics Cambridge, MA, United States)
Ko, Y.-K.
(Harvard-Smithsonian Center for Astrophysics Cambridge, MA, United States)
Raymond, J. C.
(Harvard-Smithsonian Center for Astrophysics Cambridge, MA, United States)
Date Acquired
August 24, 2013
Publication Date
January 1, 2009
Publication Information
Publication: The Astrophysical Journal
Volume: 693
Subject Category
Solar Physics
Funding Number(s)
CONTRACT_GRANT: NNX08AQ96G
Distribution Limits
Public
Copyright
Other

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