PROSWIN: Probabilistic Solar Wind Speed Forecasting Using Deep Distributional Regression From Solar Images

Abstract Accurately predicting fast solar wind conditions is challenging, as uncertainties are large and unquantified by traditional single‐value prediction models. In particular, the risks of high‐speed solar wind streams (HSSs), which can cause damage to technological infrastructure, cannot be reliably assessed without probabilistic forecasts. We present PROSWIN, a probabilistic machine learning model that forecasts the hourly solar wind speed (SWS) at Earth with a 4‐day lead time. The approach combines solar images and magnetograms using a deep neural network coupled to a distributional regression algorithm. Because standard error metrics underweight the relevance of HSS peaks, we further introduce the prediction score (PS) , a model‐selection metric that jointly rewards timeline and HSS peak accuracy. On 14 years of data, our forecast achieves very well‐calibrated uncertainties (<1% average absolute coverage deviation). Using the continuous ranked probability score (CRPS), a metric that assesses distributional accuracy, we obtain a timeline CRPS of 41.0 km/s, an HSS peak CRPS of 45.3 km/s, and a PS of 42.3 km/s. We find that the 171 Å channel is an important complement to the typically used 193 and 211 Å channels and that the PS for model selection improves the applicability of the model. Compared to selected models from the literature, ours is the only one that is accurate for both timeline and HSS peak values, rather than trading one off against the other. These results support the advantages of probabilistic over single‐value solar wind models. The introduced methods are also transferable to other forecasting problems.

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Publication Details

Journal
AGU Advances
Published
2026-10-30
DOI
https://doi.org/10.1029/2026av002524
Primary Topic
Solar and Space Plasma Dynamics
Type
article
Field-Weighted Citation Impact
0.00

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article

PROSWIN: Probabilistic Solar Wind Speed Forecasting Using Deep Distributional Regression From Solar Images

Nadja Klein, Luca Chiarabini, Daniel Collin, Yuri Shprits et al.
4 links
AGU Advances
Solar and Space Plasma Dynamics
article

PROSWIN: Probabilistic Solar Wind Speed Forecasting Using Deep Distributional Regression From Solar Images

Nadja Klein, Luca Chiarabini, Daniel Collin, Yuri Shprits, Stefan J. Hofmeister, Guillermo Gallego
article en

Abstract

Abstract Accurately predicting fast solar wind conditions is challenging, as uncertainties are large and unquantified by traditional single‐value prediction models. In particular, the risks of high‐speed solar wind streams (HSSs), which can cause damage to technological infrastructure, cannot be reliably assessed without probabilistic forecasts. We present PROSWIN, a probabilistic machine learning model that forecasts the hourly solar wind speed (SWS) at Earth with a 4‐day lead time. The approach combines solar images and magnetograms using a deep neural network coupled to a distributional regression algorithm. Because standard error metrics underweight the relevance of HSS peaks, we further introduce the prediction score (PS) , a model‐selection metric that jointly rewards timeline and HSS peak accuracy. On 14 years of data, our forecast achieves very well‐calibrated uncertainties (<1% average absolute coverage deviation). Using the continuous ranked probability score (CRPS), a metric that assesses distributional accuracy, we obtain a timeline CRPS of 41.0 km/s, an HSS peak CRPS of 45.3 km/s, and a PS of 42.3 km/s. We find that the 171 Å channel is an important complement to the typically used 193 and 211 Å channels and that the PS for model selection improves the applicability of the model. Compared to selected models from the literature, ours is the only one that is accurate for both timeline and HSS peak values, rather than trading one off against the other. These results support the advantages of probabilistic over single‐value solar wind models. The introduced methods are also transferable to other forecasting problems.

AGU AdvancesVol. 7(8)
Karlsruhe Institute of Technology (DE), University of California, Los Angeles (US), University of Potsdam (DE), Deutsches Zentrum für Luft- und Raumfahrt e. V. (DLR) (DE), Einstein Center Digital Future (DE), GFZ Helmholtz Centre for Geosciences (DE), Technische Universität Berlin (DE), Columbia University (US)
National Science Foundation
Openalex Percentile: Top 26%
Solar and Space Plasma Dynamics
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