On the Relationship Between G-Band Bright Point Dynamics and Their Magnetic Field Strengths
文献类型：期刊论文
| 作者 | Yang, Yunfei1,2; Li, Qiang1; Ji, Kaifan1 ; Feng, Song1,2; Deng, Hui1; Wang F(王锋)1,3; Lin, Jiaben2
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| 刊名 | SOLAR PHYSICS
 |
| 出版日期 | 2016-04-01 |
| 卷号 | 291期号:4页码:1089-1105 |
| ISSN号 | 0038-0938 |
| 关键词 | Bright points, Photosphere Dynamics, Magnetic Magnetic fields, Photosphere |
| 通讯作者 | Ji, KF (reprint author), Kunming Univ Sci & Technol, Yunnan Key Lab Comp Technol Applicat, Fac Informat Engn & Automat, Kunming 650500, Peoples R China. |
| 产权排序 | 第三完成单位 |
| 英文摘要 | G-band bright points (GBPs) are regarded as good manifestations of magnetic flux concentrations. We aim to investigate the relation between the dynamic properties of GBPs and their longitudinal magnetic field strengths. High spatial and temporal resolution observations were recorded simultaneously with G-band filtergrams and Narrow-band Filter Imager (NFI) Stokes I and V images with Hinode/Solar Optical Telescope. The GBPs are automatically identified and tracked in the G-band images, and the corresponding longitudinal magnetic field strength of each GBP is extracted from the calibrated NFI magnetograms by a point-to-point method. After categorizing the GBPs into five groups by their longitudinal magnetic field strengths, we analyzed the dynamics of each group of GBPs. The results suggest that with increasing longitudinal magnetic field strengths of GBPs correspond to a decrease in their horizontal velocities and motion ranges as well as by showing more complex motion paths. This suggests that magnetic elements showing weaker magnetic field strengths move faster and farther along straighter paths, while stronger elements move more slowly in more erratic paths within a smaller region. The dynamic behaviors of GBPs with different longitudinal magnetic field strengths can be explained by that the stronger flux concentrations withstand the convective flows much better than weaker ones. |
| 学科主题 | Astronomy & Astrophysics |
| WOS标题词 | Science & Technology ; Physical Sciences |
| 类目[WOS] | Astronomy & Astrophysics |
| 研究领域[WOS] | Astronomy & Astrophysics |
| 关键词[WOS] | SOLAR OPTICAL TELESCOPE ; ACTIVE-REGION ; FLUX TUBES ; WAVE-PROPAGATION ; QUIET SUN ; PHOTOSPHERE ; SIMULATIONS ; CALIBRATION ; DISPERSAL ; ELEMENTS |
| 收录类别 | SCI |
| 原文出处 | http://link.springer.com/article/10.1007%2Fs11207-016-0889-y |
| 语种 | 英语 |
| WOS记录号 | WOS:000378240000004 |
| 源URL | [http://ir.ynao.ac.cn/handle/114a53/9615]  |
| 专题 | 云南天文台_其他 |
| 作者单位 | 1.Faculty of Information Engineering and Automation/Yunnan Key Laboratory of Computer Technology Application, Kunming University of Science and Technology, 650500, Kunming, China 2.Key Laboratory of Solar Activity, National Astronomical Observatories, Chinese Academy of Sciences, 100012, Beijing, China 3.Yunnan Observatory, Chinese Academy of Sciences, 650011, Kunming, China |
| 推荐引用方式 GB/T 7714 | Yang, Yunfei,Li, Qiang,Ji, Kaifan,et al. On the Relationship Between G-Band Bright Point Dynamics and Their Magnetic Field Strengths[J]. SOLAR PHYSICS,2016,291(4):1089-1105. |
| APA | Yang, Yunfei.,Li, Qiang.,Ji, Kaifan.,Feng, Song.,Deng, Hui.,...&Lin, Jiaben.(2016).On the Relationship Between G-Band Bright Point Dynamics and Their Magnetic Field Strengths.SOLAR PHYSICS,291(4),1089-1105. |
| MLA | Yang, Yunfei,et al."On the Relationship Between G-Band Bright Point Dynamics and Their Magnetic Field Strengths".SOLAR PHYSICS 291.4(2016):1089-1105. |
入库方式： OAI收割
来源：云南天文台
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