Solar Wind MME (Multi-Model Ensemble) at target: Jupiter

The multi-model ensemble (MME) resulting from running the Multi-Model Ensemble System for the outer Heliosphere (MMESH) at Jupiter, using in-situ solar wind data from the Ulysses and Juno spacecraft and the HUXt, MSWIM2D, and Tao et al. (2005) solar wind propagation models where available. The MMESH framework is described in Rutala et al. (2024) and Rutala et al. (2025). Two .csv files are provided for each date range: one including constituent models and one with only the ensemble average. Within each file, solar wind parameters are reported as following a skew-normal distribution, with a central value (_loc), a spread (_scale), and a skew (_a). Using all three of these distribution parameters to describe the ensemble output will yield the most accurate uncertainty estimates. Header contents, reproduced for convenience:Multi-Model Ensemble System for the outer Heliosphere (MMESH) Output MME for target: Jupiter Spanning: 1991/11/23 - 2025/07/01 (with gaps)Run by: M. J. Rutala, 2026/03/25 First row (if present) indicates the source of the parameter (whether consituent model or the ensemble itself) Second row indicates the parameter Units are as follows: B_mag (magnitude of the IMF): nT n_tot (total number density of solar wind, assumed to be all protons): cm^-3 p_dyn (solar wind dynamic pressure): nPa u_mag (magnitude of the solar wind flow speed): km/s