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Morphology, dynamics and plasma parameters of plumes and inter-plume regions in solar coronal holes
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; Poletto, G.8; Raouafi, N. -E.9; Suess, S. T.10; Teriaca, L.1; Wang, Y. -M.11
2011-06-16
Source PublicationASTRONOMY AND ASTROPHYSICS REVIEW
ISSN0935-4956
Volume19Pages:1-70
AbstractCoronal 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.
KeywordSun Corona Coronal Holes Coronal Plumes Inter-plume Regions Solar Wind
Subject AreaAstronomy & Astrophysics
WOS HeadingsScience & Technology ; Physical Sciences
DOI10.1007/s00159-011-0035-7
WOS KeywordEXTREME-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
Indexed BySCI
Language英语
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS IDWOS:000295976300001
Citation statistics
Cited Times:41[WOS]   [WOS Record]     [Related Records in WOS]
Document Type期刊论文
Identifierhttp://libir.pmo.ac.cn/handle/332002/4489
Collection太阳高能及相关物理过程研究团组
Affiliation1.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
11.USN, Code 7672, EO Hulburt Ctr Space Res, Res Lab, Washington, DC 20375 USA
Recommended Citation
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.
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