Phase relations between total solar irradiance and the Mg II index
文献类型：期刊论文
| 作者 | Li KJ(李可军)1,2 ; Xu JC(徐景晨)1,3; Xiang NB(向南彬)1,3; Feng, W.4,5
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| 刊名 | ADVANCES IN SPACE RESEARCH
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| 出版日期 | 2016 |
| 卷号 | 57期号:1页码:408-417 |
| 关键词 | Sun: general Sun: activity Sun: chromosphere |
| ISSN号 | 0273-1177 |
| 产权排序 | 第一完成单位 |
| 英文摘要 | The Mg II index is usually used to represent the brightening contribution to total solar irradiance (TSI) by solar bright structures, such as faculae and network. In order to understand variations of TSI, phase relations of TSI and the chromospheric Mg II index is investigated on time-scales of one year and longer. The NOAA daily Mg II index at the time interval of November 17, 1978 October 24, 2007 is utilized to carry out correlation analyses respectively with the daily ACRIM and PMOD composites of TSI. The Mg II index is found to lead TSI by about one solar rotation period for time-scales of one year and longer. Correlation of TSI with the Mg II index on the time-scale of one year is sometimes significantly positive, sometimes statistically insignificant, and sometimes even significantly negative. When sunspot darkening is dominant, the correlation between TSI and Mg II is either negative or not significant. When TSI is backward shifted vs the Mg II index by about one rotation period, correlation between them becomes significantly positive in all years. Thus, it is after about one rotation period that a more prominent intensification is inferred to be contributed to TSI than that immediately, by bright constructions, which is represented by the Mg II index. We propose an explanation for the phase relationship of TSI and the Mg II index. (C) 2015 COSPAR. Published by Elsevier Ltd. All rights reserved. |
| WOS标题词 | Science & Technology ; Physical Sciences |
| 学科主题 | Astronomy & Astrophysics ; Geology ; Meteorology & Atmospheric Sciences |
| 类目[WOS] | Astronomy & Astrophysics ; Geosciences, Multidisciplinary ; Meteorology & Atmospheric Sciences |
| 研究领域[WOS] | Astronomy & Astrophysics ; Geology ; Meteorology & Atmospheric Sciences |
| 关键词[WOS] | MAGNETIC-FLUX ; CYCLES 21-23 ; VARIABILITY ; RECONSTRUCTION ; FLUCTUATIONS ; MODEL ; PROXY |
| 收录类别 | SCI |
| 原文出处 | http://www.sciencedirect.com/science/article/pii/S0273117715007395# |
| 语种 | 英语 |
| WOS记录号 | WOS:000368564300033 |
| 源URL | [http://ir.ynao.ac.cn/handle/114a53/9326]  |
| 专题 | 云南天文台_太阳物理研究组 |
| 作者单位 | 1.Yunnan Observatories, Chinese Academy of Sciences, Kunming 650011, China 2.Key Laboratory of Solar Activity, National Astronomical Observatories, CAS, Beijing 100012, China 3.University of Chinese Academy of Sciences, Beijing 100049, China 4.Research Center of Analysis and Measurement, Kunming University of Science and Technology, Kunming 650093, China 5.Key Laboratory of Modern Astronomy and Astrophysics (Nanjing University) Ministry of Education, Nanjing 210093, China |
| 推荐引用方式 GB/T 7714 | Li KJ,Xu JC,Xiang NB,et al. Phase relations between total solar irradiance and the Mg II index[J]. ADVANCES IN SPACE RESEARCH,2016,57(1):408-417. |
| APA | Li KJ,Xu JC,Xiang NB,&Feng, W..(2016).Phase relations between total solar irradiance and the Mg II index.ADVANCES IN SPACE RESEARCH,57(1),408-417. |
| MLA | Li KJ,et al."Phase relations between total solar irradiance and the Mg II index".ADVANCES IN SPACE RESEARCH 57.1(2016):408-417. |
入库方式： OAI收割
来源：云南天文台
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