Using Gradient Boosting Regression to Improve Ambient Solar Wind Model Predictions. Issue 5 (26th May 2021)
- Record Type:
- Journal Article
- Title:
- Using Gradient Boosting Regression to Improve Ambient Solar Wind Model Predictions. Issue 5 (26th May 2021)
- Main Title:
- Using Gradient Boosting Regression to Improve Ambient Solar Wind Model Predictions
- Authors:
- Bailey, R. L.
Reiss, M. A.
Arge, C. N.
Möstl, C.
Henney, C. J.
Owens, M. J.
Amerstorfer, U. V.
Amerstorfer, T.
Weiss, A. J.
Hinterreiter, J. - Abstract:
- Abstract: Studying the ambient solar wind, a continuous pressure‐driven plasma flow emanating from our Sun, is an important component of space weather research. The ambient solar wind flows in interplanetary space determine how solar storms evolve through the heliosphere before reaching Earth, and especially during solar minimum are themselves a driver of activity in the Earth's magnetic field. Accurately forecasting the ambient solar wind flow is therefore imperative to space weather awareness. Here, we present a machine learning approach in which solutions from magnetic models of the solar corona are used to output the solar wind conditions near the Earth. The results are compared to observations and existing models in a comprehensive validation analysis, and the new model outperforms existing models in almost all measures. In addition, this approach offers a new perspective to discuss the role of different input data to ambient solar wind modeling, and what this tells us about the underlying physical processes. The final model discussed here represents an extremely fast, well‐validated and open‐source approach to the forecasting of ambient solar wind at Earth. Key Points: We present a machine learning approach to use in place of the Wang‐Sheeley‐Arge (WSA) model for predicting solar wind speed near Earth The tool is validated on one whole solar cycle and outperforms established models and a baseline recurrence model This study presents a fast and well‐validatedAbstract: Studying the ambient solar wind, a continuous pressure‐driven plasma flow emanating from our Sun, is an important component of space weather research. The ambient solar wind flows in interplanetary space determine how solar storms evolve through the heliosphere before reaching Earth, and especially during solar minimum are themselves a driver of activity in the Earth's magnetic field. Accurately forecasting the ambient solar wind flow is therefore imperative to space weather awareness. Here, we present a machine learning approach in which solutions from magnetic models of the solar corona are used to output the solar wind conditions near the Earth. The results are compared to observations and existing models in a comprehensive validation analysis, and the new model outperforms existing models in almost all measures. In addition, this approach offers a new perspective to discuss the role of different input data to ambient solar wind modeling, and what this tells us about the underlying physical processes. The final model discussed here represents an extremely fast, well‐validated and open‐source approach to the forecasting of ambient solar wind at Earth. Key Points: We present a machine learning approach to use in place of the Wang‐Sheeley‐Arge (WSA) model for predicting solar wind speed near Earth The tool is validated on one whole solar cycle and outperforms established models and a baseline recurrence model This study presents a fast and well‐validated open‐source contribution to the field of ambient solar wind modeling and prediction … (more)
- Is Part Of:
- Space weather. Volume 19:Issue 5(2021)
- Journal:
- Space weather
- Issue:
- Volume 19:Issue 5(2021)
- Issue Display:
- Volume 19, Issue 5 (2021)
- Year:
- 2021
- Volume:
- 19
- Issue:
- 5
- Issue Sort Value:
- 2021-0019-0005-0000
- Page Start:
- n/a
- Page End:
- n/a
- Publication Date:
- 2021-05-26
- Subjects:
- Space environment -- Periodicals
551.509992 - Journal URLs:
- http://onlinelibrary.wiley.com/journal/10.1002/(ISSN)1542-7390 ↗
http://onlinelibrary.wiley.com/ ↗ - DOI:
- 10.1029/2020SW002673 ↗
- Languages:
- English
- ISSNs:
- 1542-7390
- Deposit Type:
- Legaldeposit
- View Content:
- Available online (eLD content is only available in our Reading Rooms) ↗
- Physical Locations:
- British Library DSC - 8361.669600
British Library DSC - BLDSS-3PM
British Library HMNTS - ELD Digital store - Ingest File:
- 17554.xml