Machine learning in solar physics

Author:

Asensio Ramos AndrésORCID,Cheung Mark C. M.,Chifu Iulia,Gafeira Ricardo

Abstract

AbstractThe application of machine learning in solar physics has the potential to greatly enhance our understanding of the complex processes that take place in the atmosphere of the Sun. By using techniques such as deep learning, we are now in the position to analyze large amounts of data from solar observations and identify patterns and trends that may not have been apparent using traditional methods. This can help us improve our understanding of explosive events like solar flares, which can have a strong effect on the Earth environment. Predicting hazardous events on Earth becomes crucial for our technological society. Machine learning can also improve our understanding of the inner workings of the sun itself by allowing us to go deeper into the data and to propose more complex models to explain them. Additionally, the use of machine learning can help to automate the analysis of solar data, reducing the need for manual labor and increasing the efficiency of research in this field.

Publisher

Springer Science and Business Media LLC

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference283 articles.

1. Abadi M, Agarwal A, Barham P, Brevdo E, Chen Z, Citro C, Corrado GS, Davis A, Dean J, Devin M, Ghemawat S, Goodfellow I, Harp A, Irving G, Isard M, Jia Y, Jozefowicz R, Kaiser L, Kudlur M, Levenberg J, Mané D, Monga R, Moore S, Murray D, Olah C, Schuster M, Shlens J, Steiner B, Sutskever I, Talwar K, Tucker P, Vanhoucke V, Vasudevan V, Viégas F, Vinyals O, Warden P, Wattenberg M, Wicke M, Yu Y, Zheng X (2015) TensorFlow: large-scale machine learning on heterogeneous systems. https://www.tensorflow.org/

2. Allred JC, Kowalski AF, Carlsson M (2015) A unified computational model for solar and stellar flares. Astrophys J 809(1):104. https://doi.org/10.1088/0004-637X/809/1/104. arXiv:1507.04375 [astro-ph.SR]

3. Altschuler MD, Newkirk G (1969) Magnetic fields and the structure of the solar corona. I: methods of calculating coronal fields. Sol Phys 9(1):131–149. https://doi.org/10.1007/BF00145734

4. Ardizzone L, Kruse J, Wirkert S, Rahner D, Pellegrini EW, Klessen RS, Maier-Hein L, Rother C, Köthe U (2018) Analyzing inverse problems with invertible neural networks. arXiv e-prints arXiv:1808.04730 [cs.LG]

5. Armstrong JA, Fletcher L (2019) Fast solar image classification using deep learning and its importance for automation in solar physics. Sol Phys 294(6):80. https://doi.org/10.1007/s11207-019-1473-z. arXiv:1905.13575 [astro-ph.SR]

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