Post-processing Probabilistic Forecasts of the Solar Wind by Data Mining Similar Scenarios
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arXiv
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| Auteurs principaux: | , , , |
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| Format: | Preprint |
| Publié: |
2026
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| _version_ | 1866914386769084416 |
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| author | da Silva, Daniel E. Parlikar, Yash Jones, Shaela I. Arge, Charles N. |
| author_facet | da Silva, Daniel E. Parlikar, Yash Jones, Shaela I. Arge, Charles N. |
| contents | The solar wind speed at Earth is one of the most important parameters regarding the effects of space weather on society. Thus far, most approaches for predicting the solar wind speed produce a single-value time series without uncertainty, or utilize ensemble methods which require custom calibration development. In this study, a method is developed that produces calibrated probabilistic forecasts of the solar wind speed using skew normal distributions and a novel extension of analog ensembles. In our extension, the single-value predictions from a baseline model of the next $Δt$ days are used along with $Δwindow$ hours of recent observations and single-value predictions to create a forecasting scenario vector that is compared against a historical database for outcomes. The baseline model used is the combined Air Force Data Assimilative Photospheric Flux Transport-Wang Sheeley Arge (ADAPT-WSA) model and the WSA point parcel simulation, but the method is directly applicable to other deterministic models including components such as Enlil or the Heliospheric Upwind Extrapolation with time dependence model (HUXt). The approach works notably well on the benchmark of whether observations fall within the $p^{th}$ percentile $p\%$ of the time (for $p$ between 0 and 100). Falling back on the mean or median of the predicted distribution as a non-probabilistic prediction yields a direct improvement in root-mean-square error (RMSE) over the original WSA point parcel simulation, and is shown to beat $\approx$ 1 solar rotation recurrence for 1-5 day ahead forecasts. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2603_11284 |
| institution | arXiv |
| publishDate | 2026 |
| record_format | arxiv |
| spellingShingle | Post-processing Probabilistic Forecasts of the Solar Wind by Data Mining Similar Scenarios da Silva, Daniel E. Parlikar, Yash Jones, Shaela I. Arge, Charles N. Solar and Stellar Astrophysics Space Physics The solar wind speed at Earth is one of the most important parameters regarding the effects of space weather on society. Thus far, most approaches for predicting the solar wind speed produce a single-value time series without uncertainty, or utilize ensemble methods which require custom calibration development. In this study, a method is developed that produces calibrated probabilistic forecasts of the solar wind speed using skew normal distributions and a novel extension of analog ensembles. In our extension, the single-value predictions from a baseline model of the next $Δt$ days are used along with $Δwindow$ hours of recent observations and single-value predictions to create a forecasting scenario vector that is compared against a historical database for outcomes. The baseline model used is the combined Air Force Data Assimilative Photospheric Flux Transport-Wang Sheeley Arge (ADAPT-WSA) model and the WSA point parcel simulation, but the method is directly applicable to other deterministic models including components such as Enlil or the Heliospheric Upwind Extrapolation with time dependence model (HUXt). The approach works notably well on the benchmark of whether observations fall within the $p^{th}$ percentile $p\%$ of the time (for $p$ between 0 and 100). Falling back on the mean or median of the predicted distribution as a non-probabilistic prediction yields a direct improvement in root-mean-square error (RMSE) over the original WSA point parcel simulation, and is shown to beat $\approx$ 1 solar rotation recurrence for 1-5 day ahead forecasts. |
| title | Post-processing Probabilistic Forecasts of the Solar Wind by Data Mining Similar Scenarios |
| topic | Solar and Stellar Astrophysics Space Physics |
| url | https://arxiv.org/abs/2603.11284 |