Morphology, dynamics and plasma parameters of plumes and inter-plume regions in solar coronal holes
文献类型：期刊论文
| 作者 | Wilhelm, K.1; Abbo, L.3; Auchere, F.4; Barbey, N.4; Feng, L.1,2 ; Gabriel, A. H.4; Giordano, S.3; Imada, S.5; Llebaria, A.6; Matthaeus, W. H.7
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| 刊名 | ASTRONOMY AND ASTROPHYSICS REVIEW
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| 出版日期 | 2011-06-16 |
| 卷号 | 19页码:1-70 |
| 关键词 | Sun Corona Coronal holes Coronal plumes Inter-plume regions Solar wind |
| ISSN号 | 0935-4956 |
| 英文摘要 | Coronal plumes, which extend from solar coronal holes (CH) into the high corona and-possibly-into the solar wind (SW), can now continuously be studied with modern telescopes and spectrometers on spacecraft, in addition to investigations from the ground, in particular, during total eclipses. Despite the large amount of data available on these prominent features and related phenomena, many questions remained unanswered as to their generation and relative contributions to the high-speed streams emanating from CHs. An understanding of the processes of plume formation and evolution requires a better knowledge of the physical conditions at the base of CHs, in plumes and in the surrounding inter-plume regions. More specifically, information is needed on the magnetic field configuration, the electron densities and temperatures, effective ion temperatures, non-thermal motions, plume cross sections relative to the size of a CH, the plasma bulk speeds, as well as any plume signatures in the SW. In spring 2007, the authors proposed a study on 'Structure and dynamics of coronal plumes and inter-plume regions in solar coronal holes' to the International Space Science Institute (ISSI) in Bern to clarify some of these aspects by considering relevant observations and the extensive literature. This review summarizes the results and conclusions of the study. Stereoscopic observations allowed us to include three-dimensional reconstructions of plumes. Multi-instrument investigations carried out during several campaigns led to progress in some areas, such as plasma densities, temperatures, plume structure and the relation to other solar phenomena, but not all questions could be answered concerning the details of plume generation process(es) and interaction with the SW. |
| 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] | EXTREME-ULTRAVIOLET OBSERVATIONS ; SLOW MAGNETOSONIC WAVES ; R-CIRCLE-DOT ; MAGNETOHYDRODYNAMIC TURBULENCE DRIVEN ; PRESSURE BALANCE STRUCTURES ; EUV IMAGING SPECTROMETER ; POLAR PLUMES ; WHITE-LIGHT ; TRANSITION-REGION ; QUIET-SUN |
| 收录类别 | SCI |
| 语种 | 英语 |
| WOS记录号 | WOS:000295976300001 |
| 公开日期 | 2012-08-07 |
| 源URL | [http://libir.pmo.ac.cn/handle/332002/4489]  |
| 专题 | 紫金山天文台_太阳高能及相关物理过程研究团组 |
| 作者单位 | 1.Max Planck Inst Sonnensyst Forsch, D-37191 Katlenburg Lindau, Germany 2.Chinese Acad Sci, Purple Mt Observ, Nanjing 210008, Peoples R China 3.INAF Osservatorio Astron Torino, I-10025 Pino Torinese, Italy 4.Univ Paris 11, Inst Astrophys Spatiale, F-91405 Orsay, France 5.Japan Aerosp Explorat Agcy, Inst Space & Astronaut Sci, Sagamihara, Kanagawa 2298510, Japan 6.Observ Astron Marseille Prov, Lab Astrophys Marseille, F-13388 Marseille 13, France 7.Univ Delaware, Bartol Res Inst, Dept Phys & Astron, Newark, DE USA 8.Osserv Astrofis Arcetri, I-50125 Florence, Italy 9.Johns Hopkins Univ, Appl Phys Lab, Laurel, MD 20723 USA 10.Natl Space Sci & Technol Ctr, Huntsville, AL 35805 USA |
| 推荐引用方式 GB/T 7714 | Wilhelm, K.,Abbo, L.,Auchere, F.,et al. Morphology, dynamics and plasma parameters of plumes and inter-plume regions in solar coronal holes[J]. ASTRONOMY AND ASTROPHYSICS REVIEW,2011,19:1-70. |
| APA | Wilhelm, K..,Abbo, L..,Auchere, F..,Barbey, N..,Feng, L..,...&Wang, Y. -M..(2011).Morphology, dynamics and plasma parameters of plumes and inter-plume regions in solar coronal holes.ASTRONOMY AND ASTROPHYSICS REVIEW,19,1-70. |
| MLA | Wilhelm, K.,et al."Morphology, dynamics and plasma parameters of plumes and inter-plume regions in solar coronal holes".ASTRONOMY AND ASTROPHYSICS REVIEW 19(2011):1-70. |
入库方式： OAI收割
来源：紫金山天文台
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