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.

Input satellite and time range.

Created Trajectory: View Download


Upload a trajectory file for interpolation.

Sample Trajectory Format:  View Download
Note: Trajectory must be in HGI coordinates.

Upload desired trajectory file:

Interpolated Solar Wind: View Download