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MagNet—A Data‐Science Competition to Predict Disturbance Storm‐Time Index ( Dst ) From Solar Wind Data
Ist Teil von
Space Weather, 2023-10, Vol.21 (10)
Ort / Verlag
Washington: John Wiley & Sons, Inc
Erscheinungsjahr
2023
Quelle
EZB Electronic Journals Library
Beschreibungen/Notizen
Abstract
Enhanced interaction between solar‐wind and Earth's magnetosphere can cause space weather and geomagnetic storms that have the potential to damage critical technologies, such as magnetic navigation, radio communications, and power grids. The severity of a geomagnetic storm is measured using the disturbance‐storm‐time (
Dst
) index. The
Dst
index is calculated by averaging the horizontal component of the magnetic field observed at four near‐equatorial observatories and is used to drive geomagnetic disturbance models. As a key specification of the magnetospheric dynamics, the
Dst
index is used to drive geomagnetic disturbance models such as the High Definition Geomagnetic Model—Real Time. Since 1975, forecasting models have been proposed to forecast Dst solely from solar wind observations at the Lagrangian‐1 position. However, while the recent Machine‐Learning (ML) models generally perform better than other approaches, many are unsuitable for operational use. Recent exponential growth in data‐science research and the democratization of ML tools have opened up the possibility of crowd‐sourcing specific problem‐solving tasks with clear constraints and evaluation metrics. To this end, National Oceanic and Atmospheric Administration (NOAA)'s National Centers for Environmental Information and the University of Colorado's Cooperative Institute for Research in Environmental Sciences conducted an open data‐science challenge called “MagNet: Model the Geomagnetic Field.” The challenge attracted 622 participants, resulting in 1,197 model submissions that used various ML approaches. The top models that met the evaluation criteria are operationally viable and retrainable and suitable for NOAA's operational needs. The paper summarizes the competition results and lessons learned.
Plain Language Summary
Solar wind interacting with Earth's magnetosphere can cause geomagnetic storms, damaging critical technologies. The disturbance‐storm‐time (
Dst
) index measures storm severity, driving geomagnetic disturbance models. Traditional
Dst
forecasting relied on solar wind observations, but recent Machine Learning (ML) models show promise. However, many are unsuitable for operational use. To explore viable ML solutions, National Oceanic and Atmospheric Administration and the University of Colorado organized the “MagNet: Model the Geomagnetic Field” challenge. Six hundred and twenty‐two participants submitted 1,197 ML‐based models for predicting Dst. The top‐performing models meeting evaluation criteria are operationally viable and retrainable, meeting NOAA's operational needs. The paper summarizes competition results and insights, emphasizing ML's potential to enhance geomagnetic storm forecasting for practical applications.
Key Points
The MagNet challenge attracted 622 participants from 64 countries who submitted 1,197 models to predict Dst in a real‐time modeling environment
The ensemble average of the top four winning models, which used different modeling architectures, performed better than individual models for both competition and post‐competition data
The challenge revealed notable successes and areas for improvement