Extended Table 1 for ApJL Article "Why Is the Great Solar Active Region 12192 Flare-Rich But CME-Poor?"
Abstract/Contents
- Abstract
- Comparison of magnetic characteristics of three major active regions before and after major flare.
Description
| Type of resource | software, multimedia |
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| Date created | April 10, 2015 |
Creators/Contributors
| Author | Sun, Xudong |
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Subjects
| Subject | Hansen Experimental Physics Laboratory |
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| Subject | Sola Physics |
| Genre | Dataset |
Bibliographic information
| Related Publication | Sun et al., (2015). Why is the great solar active region 12192 flare-rich but CME-poor? ApJL 804:L28 http://dx.doi.org/10.1088/2041-8205/804/2/L28 |
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| Related item |
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| Location | https://purl.stanford.edu/ss540kq5576 |
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
- Sun, Xudong. (2015). Extended Table 1 for ApJL Article "Why Is the Great Solar Active Region 12192 Flare-Rich But CME-Poor?". Stanford Digital Repository. Available at: http://purl.stanford.edu/ss540kq5576
Collection
Stanford Research Data
View other items in this collection in SearchWorksContact information
- Contact
- xudong@sun.stanford.edu
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