Comparative Analysis of Prediction of Coronal Mass Ejections (CME) based on Sunspot Activities Using Various Machine Learning Models
暂无分享,去创建一个
Chayan Halder | Mohammad Mahruf Mahdi | M. M. Anisuzzaman Nour Tipu | Ken Fahmidur Rahman | C. Halder | M. Mahdi | Ken Fahmidur Rahman
[1] W. Feldman,et al. Solar wind stream interfaces , 1978 .
[2] Russell A. Howard,et al. The solar cycle variation of coronal mass ejections and the solar wind mass flux , 1994 .
[3] D. Webb. Understanding CMEs and their source regions , 2000 .
[4] Ron Kohavi,et al. A Study of Cross-Validation and Bootstrap for Accuracy Estimation and Model Selection , 1995, IJCAI.
[5] Andrew P. Bradley,et al. The use of the area under the ROC curve in the evaluation of machine learning algorithms , 1997, Pattern Recognit..
[6] Christopher T. Russell,et al. Relationships between coronal mass ejection speeds from coronagraph images and interplanetary characteristics of associated interplanetary coronal mass ejections , 1999 .
[7] W. Marsden. I and J , 2012 .
[8] R. Robinson,et al. Coronal disturbances , 1973 .
[9] Michelle F. Thomsen,et al. The electron edge of low latitude boundary layer during accelerated flow events , 1990 .
[10] K. Ramesh. CORONAL MASS EJECTIONS AND SUNSPOTS—SOLAR CYCLE PERSPECTIVE , 2010 .
[11] M. Al-Omari,et al. Automated Prediction of CMEs Using Machine Learning of CME – Flare Associations , 2008 .