Magnetic helicity peaks in the solar wind shift logarithmically to lower frequencies with heliocentric distance, indicating a persistent inverse cascade from the Sun out to about 0.4 AU.
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Evidence for an Inverse Cascade of Magnetic Helicity in the Inner Heliosphere
Magnetic helicity peaks in the solar wind shift logarithmically to lower frequencies with heliocentric distance, indicating a persistent inverse cascade from the Sun out to about 0.4 AU.