SDO observation of an oscillating coronal upflow yields a Strouhal number consistent with MHD vortex shedding, suggesting the phenomenon occurs in the solar corona.
Marsch, in The Sun and the Heliosphere as an Inte- grated System , Astrophysics and Space Science Library, Vol
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Evidence for Vortex Shedding in the Sun's Hot Corona
SDO observation of an oscillating coronal upflow yields a Strouhal number consistent with MHD vortex shedding, suggesting the phenomenon occurs in the solar corona.