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The origin of switchbacks in the solar wind is discussed in two classes of theory that differ in the location of the source being either near the transition region near the Sun or in the solar wind itself. The two classes of theory differ in their predictions of the switchback rate (the number of switchbacks observed per hour) as a function of distance from the Sun. To distinguish between these theories, one-hour averages of Parker Solar Probe data were averaged over five orbits to find the following: (1) The hourly averaged ...
Published by: \apj Published on: sep
YEAR: 2021   DOI: 10.3847/1538-4357/ac110d
Published by: \apjl Published on: 12/2021
YEAR: 2020   DOI: 10.3847/2041-8213/abce69