Multifractal properties of evolving active regions
Magnetohydrodynamic turbulence is thought to be responsible for producing complex, multiscale magnetic field distributions in solar active regions. Here we explore the multiscale properties of a number of evolving active regions using magnetograms from the Michelson Doppler Imager (MDI) on the Solar...
| Main Authors: | , , , , , , , |
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| Format: | Journal article |
| Published: |
2008
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