Michigan Solar WInd Model 2D (MSWIM2D)

Model input from OMNI dataset and STEREO spacecraft.

Output from SWMF/Outer Heliosphere domain run in stand-alone mode.

Interpolates modeled solar wind in the ecliptic plane between 1 AU and 75 AU to 1-hour resolution along a given trajectory.

Available Dates: 1995.01.01 - 2022.03.31

Developed by Timothy Keebler and Gabor Toth

Contact: tkeebler@umich.edu

Publication:  10.3847/1538-4365/ac67eb  (open access)

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