Tracing switchbacks back to their solar source with three propagation models yields no robust hourly correlation with coronal jet rates, so jets are not established as the main switchback precursors.
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Tracing magnetic switchbacks to their source: An assessment of solar coronal jets as switchback precursors
Tracing switchbacks back to their solar source with three propagation models yields no robust hourly correlation with coronal jet rates, so jets are not established as the main switchback precursors.