Authors: CR. Gilly (Southwest Research Institute), Momchil Molnar(Southwest Research Institute)

In this work we look at new data from the Cryo-NIRSP instrument at the DKIST atop Haleakala in Maui, HI.  These spectropolarimetric observations provide insight into the state of the corona from about X to Y solar radii. We hope to uncover and characterize the waves and flows captured in these observations.