Chromospheric network spicules have spacings of 0.4-1.5 Mm, aspect ratios of 6-40, and counts of 40-100, which the authors argue can explain the medium scale of Parker Solar Probe switchbacks through random-walk redistribution inside supergranule funnels.
D., Goetz, K., Harvey, P
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Solar Chromospheric Network as a Source for Solar Wind Switchbacks
Chromospheric network spicules have spacings of 0.4-1.5 Mm, aspect ratios of 6-40, and counts of 40-100, which the authors argue can explain the medium scale of Parker Solar Probe switchbacks through random-walk redistribution inside supergranule funnels.