In the inner heliosphere, solar-wind turbulence amplitude, wave-like character, and energy transfer rate rise with solar activity, and high-turbulence streams trace to unipolar coronal holes while low-turbulence streams trace to multipolar active-region fields.
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Solar-Cycle Modulation and Photospheric Magnetic Control of Turbulence in the Young Solar Wind
In the inner heliosphere, solar-wind turbulence amplitude, wave-like character, and energy transfer rate rise with solar activity, and high-turbulence streams trace to unipolar coronal holes while low-turbulence streams trace to multipolar active-region fields.