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Predicting short-term F-10.7 with transport models
文献类型：期刊论文
| 作者 | Liu, Cheng-ao; Zhao, Xin-hua; Chen, Tao; Li, Hui-chao |
| 刊名 | ASTROPHYSICS AND SPACE SCIENCE
 |
| 出版日期 | 2018 |
| 卷号 | 363期号:12页码:266 |
| 关键词 | Solar magnetic fields Flux transport model F-10.7 |
| ISSN号 | 0004-640X |
| DOI | 10.1007/s10509-018-3476-x |
| 英文摘要 | A solar magnetic flux transport model has the ability to demonstrate the magnetic evolution of the Sun, thus providing a foundation for space weather forecasting. Solar activities have close relationships to the Sun's magnetic fields. To predict the Sun's magnetic environment more precisely, many versions of magnetic flux rope models have been developed. We utilized two models that were created by Yeates et al. (Sol. Phys. 245(1):87, 2007) (hereinafter referred to as the Y model) and Worden and Harvey (Sol. Phys. 195(2):247, 2000) (hereinafter referred to as the WH model) to predict the short-term changes of 10.7cm radio flux (F10.7) during 2003-2014. Both models performed very well in estimating F10.7 values. The statistical results of analyzing the correlation coefficient, mean absolute error, mean square error, relative error, frequency distribution, etc. show that the Y model is superior to the WH model. The meridional flow and diffusion process used in the WH model do not agree with the observations. Such discrepancies may influence estimates of the global flux. |
| 语种 | 英语 |
| 源URL | [http://ir.nssc.ac.cn/handle/122/6606]  |
| 专题 | 国家空间科学中心_空间科学部 |
| 推荐引用方式 GB/T 7714 | Liu, Cheng-ao,Zhao, Xin-hua,Chen, Tao,et al. Predicting short-term F-10.7 with transport models[J]. ASTROPHYSICS AND SPACE SCIENCE,2018,363(12):266. |
| APA | Liu, Cheng-ao,Zhao, Xin-hua,Chen, Tao,&Li, Hui-chao.(2018).Predicting short-term F-10.7 with transport models.ASTROPHYSICS AND SPACE SCIENCE,363(12),266. |
| MLA | Liu, Cheng-ao,et al."Predicting short-term F-10.7 with transport models".ASTROPHYSICS AND SPACE SCIENCE 363.12(2018):266. |
入库方式： OAI收割
来源：国家空间科学中心
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