Authors: Lidiya Y. Ahmed (Smithsonian Astrophysical Observatory, Harvard University), Michael L. Stevens (Smithsonian Astrophysical Observatory), Kristoff Paulson (Smithsonian Astrophysical Observatory), Sam Badman (Smithsonian Astrophysical Observatory), Yeimy Rivera (Smithsonian Astrophysical Observatory)

Three spacecraft, over five traversals, observed a solar wind stream traceable to a specific coronal hole that could be seen during the eclipse. In this project, DTW is used to map between traversal time series in order to understand the evolution of the solar wind.