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Are electric currents in solar active regions neutralized? View all abstracts by submitter

Mike Wheatland   Submitted: 1999-11-17 03:03

Models for energy storage in the solar corona due to the twisting of coronal magnetic fields by subphotospheric flows imply that coronal currents should be neutralized (i.e. observed currents over a given polarity of the magnetic field should sum to zero). The neutralized current hypothesis is quantitatively tested by examining vector magnetic field data from 21 active regions observed by the Solar Magnetic Field Telescope of the Huariou Solar Observing Station of Beijing Astronomical Observatory. For each active region the current over the positive polarity of the field, I_+, is estimated, as well as the current over the negative polarity, I_-, and the total current over both polarities, I_tot. In no case is the total current I_tot significantly different from zero. The currents I_+ and I_- are found to be significantly different from zero (at the 3 sigma level) in more than half of the active regions studied, implying that large scale currents in active regions are typically unneutralized. The implications of this result and the relationship of this study to related studies (e.g. of current helicity) are discussed.

Authors: Wheatland, M.S.
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Publication Status: ApJ (in press)
Last Modified: 1999-11-17 03:03
Go to main E-Print page  Frequency-energy distributions of flares and active region transient brightenings
  Flare frequency-size distributions for individual active regions
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