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Observation and modelling of solar jets
Shen YD(申远灯)
Source PublicationProceedings of the Royal Society A: Mathematical, Physical and Engineering Sciences
2021-02-03
Volume477Issue:2246
DOI10.1098/rspa.2020.0217
Contribution Rank第1完成单位
Indexed ByEI
Keywordflares coronal mass ejections, magnetic fields filaments/prominences solar energetic particles magnetic reconnection
Abstract

The solar atmosphere is full of complicated transients manifesting the reconfiguration of the solar magnetic field and plasma. Solar jets represent collimated, beam-like plasma ejections; they are ubiquitous in the solar atmosphere and important for our understanding of solar activities at different scales, the magnetic reconnection process, particle acceleration, coronal heating, solar wind acceleration, as well as other related phenomena. Recent high-spatio-temporal-resolution, wide-temperature coverage and spectroscopic and stereoscopic observations taken by ground-based and space-borne solar telescopes have revealed many valuable new clues to restrict the development of theoretical models. This review aims at providing the reader with the main observational characteristics of solar jets, physical interpretations and models, as well as unsolved outstanding questions in future studies.

Funding ProjectNatural Science Foundation of China[11922307] ; Natural Science Foundation of China[11773068] ; Natural Science Foundation of China[11633008] ; Yunnan Science Foundation[2017FB006] ; West Light Foundation of the Chinese Academy of Sciences
Funding OrganizationNatural Science Foundation of China[11922307, 11773068, 11633008] ; Yunnan Science Foundation[2017FB006] ; West Light Foundation of the Chinese Academy of Sciences
Language英语
Subject Area天文学 ; 太阳与太阳系 ; 太阳物理学
MOST Discipline Catalogue理学 ; 理学::天文学
SubtypeJournal article (JA)
PublisherRoyal Society Publishing
ISSN1364-5021
URL查看原文
EI Accession Number20211210124175
EI KeywordsMagnetoplasma
EI Classification Number701.2 Magnetism: Basic Concepts and Phenomena - 723.2 Data Processing and Image Processing
Citation statistics
Document Type期刊论文
Identifierhttp://ir.ynao.ac.cn/handle/114a53/24199
Collection选址与日冕观测组
Corresponding AuthorShen YD(申远灯)
AffiliationYunnan Observatories, Chinese Academy of Sciences, Kunming 650216, People's Republic of China
First Author AffilicationYunnan Observatories, Chinese Academy of Sciences
Corresponding Author AffilicationYunnan Observatories, Chinese Academy of Sciences
Recommended Citation
GB/T 7714
Shen YD. Observation and modelling of solar jets[J]. Proceedings of the Royal Society A: Mathematical, Physical and Engineering Sciences,2021,477(2246).
APA Shen YD.(2021).Observation and modelling of solar jets.Proceedings of the Royal Society A: Mathematical, Physical and Engineering Sciences,477(2246).
MLA Shen YD."Observation and modelling of solar jets".Proceedings of the Royal Society A: Mathematical, Physical and Engineering Sciences 477.2246(2021).
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