Predicting Coronal Mass Ejections Using Machine Learning Methods
Abstract/Contents
- Abstract
- Of all the activity observed on the Sun, two of the most energetic events are flares and Coronal Mass Ejections (CMEs). Usually, solar active regions that produce large flares will also produce a CME, but this is not always true (Yashiro et al., 2005). Despite advances in numerical modeling, it is still unclear which circumstances will produce a CME (Webb & Howard, 2012). Therefore, it is worthwhile to empirically determine which features distinguish flares associated with CMEs from flares that are not. At this time, no extensive study has used physically meaningful features of active regions to distinguish between these two populations. As such, we attempt to do so by using features derived from [1] photospheric vector magnetic field data taken by the Solar Dynamics Observatory's Helioseismic and Magnetic Imager instrument and [2] X-ray flux data from the Geostationary Operational Environmental Satellite's X-ray Flux instrument. We build a catalog of active regions that either produced both a flare and a CME (the positive class) or simply a flare (the negative class). We then use machine-learning algorithms to [1] determine which features distinguish these two populations, and [2] forecast whether an active region that produces an M- or X-class flare will also produce a CME. We compute the True Skill Statistic, a forecast verification metric, and find that it is a relatively high value of 0.8 plus or minus 0.2. We conclude that a combination of six parameters, which are all intensive in nature, will capture most of the relevant information contained in the photospheric magnetic field. The code and data used to do this analysis are included here.
Description
| Type of resource | software, multimedia |
|---|---|
| Date created | January 25, 2016 |
Creators/Contributors
| Author | Bobra, Monica G. |
|---|---|
| Author | Ilonidis, Stathis |
Subjects
| Subject | Hansen Experimental Physics Laboratory |
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| Subject | Stanford Physics |
Bibliographic information
| Related item | |
|---|---|
| Location | https://purl.stanford.edu/wt605kh4712 |
Access conditions
- Use and reproduction
- User agrees that, where applicable, content will not be used to identify or to otherwise infringe the privacy or confidentiality rights of individuals. Content distributed via the Stanford Digital Repository may be subject to additional license and use restrictions applied by the depositor.
Preferred citation
- Preferred Citation
- Bobra, M.G. and Ilonidis, S. 2016, ApJ, 821, 127. http://dx.doi.org/10.3847/0004-637X/821/2/127
Collection
Stanford Research Data
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- Contact
- mbobra@stanford.edu
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