Solar Wind and Space Weather
Author:
Publisher
Springer Nature Switzerland
Link
https://link.springer.com/content/pdf/10.1007/978-3-031-58177-9_12
Reference86 articles.
1. Ahmed, O. W., Qahwaji, R., Colak, T., Higgins, P. A., Gallagher, P. T., & Bloomfield, D. S. (2013). Solar flare prediction using advanced feature extraction, machine learning, and feature selection. Solar Physics, 283, 157–175.
2. Arge, C. N., & Pizzo, V. J. (2000). Improvement in the prediction of solar wind conditions using near-real time solar magnetic field updates. Journal of Geophysical Research, 105, 10465–10480.
3. Ashbourn, J. M., & Woods, L. C. (2005). Accelerating the solar wind. The Astrophysical Journal, 623, 511–518.
4. Aulanier, G., Démoulin, P., Schrijver, C. J., Janvier, M., Pariat, E., & Schmieder, B. (2013). The standard flare model in three dimensions, II: Upper limit on solar flare energy. Astronomy and Astrophysics, 549, A66.
5. Ballester, J. L. (1984). A note on magnetic fields and electric currents in solar prominences. Solar Physics, 94, 151–154.
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