  Although recent research suggests a link in support of a model of switchback
formation in the solar corona via interchange reconnection that is propagated
outward with the solar wind and similarities in their ion composition to plasma
instability produced plasmoids, these plasma instabilities have yet to be
observationally linked to magnetic switchbacks. In this paper we aim to use the
theoretical framework of a twin coronal mass ejection event which is known to
include interchange reconnection processes and compare this model with
experimental observations using Parker Solar Probe FIELDS and $\isis$
instrumentationof an actual event containing two CMEs identified via the
associated solar proton event in order to further test and refine the
hypothesis of interchange reconnection as a possible physical origin for the
magnetic switchback phenomenon. We also intend to introduce a plasma model for
the formation of the switchbacks noted within the CME event.
