A multi‐model ensemble system for the Outer Heliosphere (MMESH): solar wind conditions near Jupiter

Rutala, M. J. ORCID: https://orcid.org/0000-0002-1837-4057, Jackman, C. M. ORCID: https://orcid.org/0000-0003-0635-7361, Owens, M. J. ORCID: https://orcid.org/0000-0003-2061-2453, Tao, C. ORCID: https://orcid.org/0000-0001-8817-0589, Fogg, A. R. ORCID: https://orcid.org/0000-0002-1139-5920, Murray, S. A. ORCID: https://orcid.org/0000-0002-9378-5315 and Barnard, L. ORCID: https://orcid.org/0000-0001-9876-4612 (2024) A multi‐model ensemble system for the Outer Heliosphere (MMESH): solar wind conditions near Jupiter. Journal of Geophysical Research: Space Physics, 129 (6). e2024JA032613. ISSN 2169-9402 doi: 10.1029/2024JA032613

Abstract/Summary

How the solar wind influences the magnetospheres of the outer planets is a fundamentally important question, but is difficult to answer in the absence of consistent, simultaneous monitoring of the upstream solar wind and the large-scale dynamics internal to the magnetosphere. To compensate for the relative lack of in-situ solar wind data, propagation models are often used to estimate the ambient solar wind conditions at the outer planets for comparison to remote observations or in-situ measurements. This introduces another complication: the propagation of near-Earth solar wind measurements introduces difficult-to-assess uncertainties. Here, we present the Multi-Model Ensemble System for the outer Heliosphere (MMESH) to begin to address these issues, along with the resultant multi-model ensemble (MME) of the solar wind conditions near Jupiter. MMESH accepts as input any number of solar wind models together with contemporaneous in-situ spacecraft data. From these, the system characterizes typical uncertainties in model timing, quantifies how these uncertainties vary under different conditions, attempts to correct for systematic biases in the input model timing, and composes a MME with uncertainties from the results. For the Juno-era (04/07/2016–04/07/2023) MME hindcast for Jupiter presented here, three solar wind propagation models were compared to in-situ measurements from the near-Jupiter spacecraft Ulysses and Juno spanning diverse geometries and phases of the solar cycle across >14,000 hr of data covering 2.5 decades. The MME gives the most-probable near-Jupiter solar wind conditions for times within the tested epoch, outperforming the input models and returning quantified estimates of uncertainty.

Item Type	Article
URI	https://reading-clone.eprints-hosting.org/id/eprint/116874
Item Type	Article
Refereed	Yes
Divisions	Science > School of Mathematical, Physical and Computational Sciences > Department of Meteorology
Publisher	American Geophysical Union
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