THE ROTATION PROFILE OF SOLAR MAGNETIC FIELDS BETWEEN +/- 60 degrees LATITUDES
文献类型:期刊论文
作者 | Shi XJ(石祥军)1,2![]() ![]() |
刊名 | ASTROPHYSICAL JOURNAL LETTERS
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出版日期 | 2013-08-10 |
卷号 | 773期号:1页码:1-6 |
关键词 | methods: data analysis Sun: rotation Sun: surface magnetism |
ISSN号 | 2041-8205 |
产权排序 | 第一完成单位 |
通讯作者 | Shi, XJ (reprint author), Chinese Acad Sci, Yunnan Observ, Kunming 650011, Peoples R China. |
英文摘要 | Through a cross-correlation analysis of the Carrington synoptic maps of solar photospheric magnetic fields from Carrington Rotation Nos. 1625 to 2129 (from 1975 February to 2012 October), the sidereal rotation rates of solar magnetic fields between +/- 60 degrees latitudes are investigated. It seems that the temporal variation of rotation rates should be related to the solar cycle phase. The rotation profile of magnetic fields is obtained: the sidereal rotation rates decrease from the equator to mid-latitude and reach their minimum values of about 13.16 deg day(-1) (13.17 deg day(-1)) at 53 degrees (54 degrees) latitude in the northern (southern) hemisphere, then increase toward higher latitudes. This rotation profile is different from the differential rotation law obtained by Snodgrass from a cross-correlation analysis of daily magnetograms, in which the rotation rates show a steep decrease from the equator to the poles. However, it is much closer to the quasi-rigid rotation law derived by Stenflo from an auto-correlation analysis of daily magnetograms. Some possible interpretations are discussed for the resulting rotation profile. |
WOS标题词 | Science & Technology ; Physical Sciences |
学科主题 | Astronomy & Astrophysics |
类目[WOS] | Astronomy & Astrophysics |
研究领域[WOS] | Astronomy & Astrophysics |
关键词[WOS] | DIFFERENTIAL ROTATION ; TEMPORAL VARIATIONS ; SUNSPOT GROUPS ; SUN ; PHOTOSPHERE ; MOTIONS ; SIGNAL |
收录类别 | SCI |
原文出处 | http://iopscience.iop.org/article/10.1088/2041-8205/773/1/L6/meta |
语种 | 英语 |
WOS记录号 | WOS:000322455600006 |
源URL | [http://ir.ynao.ac.cn/handle/114a53/6225] ![]() |
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.University of Chinese Academy of Sciences, Beijing 100049, China |
推荐引用方式 GB/T 7714 | Shi XJ,Xie JL. THE ROTATION PROFILE OF SOLAR MAGNETIC FIELDS BETWEEN +/- 60 degrees LATITUDES[J]. ASTROPHYSICAL JOURNAL LETTERS,2013,773(1):1-6. |
APA | Shi XJ,&Xie JL.(2013).THE ROTATION PROFILE OF SOLAR MAGNETIC FIELDS BETWEEN +/- 60 degrees LATITUDES.ASTROPHYSICAL JOURNAL LETTERS,773(1),1-6. |
MLA | Shi XJ,et al."THE ROTATION PROFILE OF SOLAR MAGNETIC FIELDS BETWEEN +/- 60 degrees LATITUDES".ASTROPHYSICAL JOURNAL LETTERS 773.1(2013):1-6. |
入库方式: OAI收割
来源:云南天文台
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