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 along a given trajectory.
Current Output Resolution: 1 hour
Available Dates: 1995.01.01 - 2019.05.31
Developed by Timothy Keebler and Gabor Toth
In case of session timeout, use smaller data range.