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Numerical analyses of self-generated magnetic fields with very small scale in solar corona
Liu, SQ; Li, XQ
2000-12-01
Source PublicationASTRONOMY & ASTROPHYSICS
ISSN0004-6361
Volume364Issue:2Pages:785-792
AbstractWe numerically study the collapse behavior of self-generated magnetic fields described by nonlinear coupling equations. The results show that magnetic fields self-generated by transverse pumping plasmons may collapse, leading to an enhancement of the magnetic field of up to 250 - 500 Gauss in the range around 0.02 - 0.03 km, which corresponds to the inferred inhomogeneity small-scale fields in both the strength and scale in the solar corona.
KeywordSun : Corona Sun : General Sun : Magnetic Fields
Subject AreaAstronomy & Astrophysics
WOS HeadingsScience & Technology ; Physical Sciences
WOS KeywordSPIKES ; FLARES
Indexed BySCI
Language英语
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS IDWOS:000166998400054
Citation statistics
Document Type期刊论文
Identifierhttp://libir.pmo.ac.cn/handle/332002/8287
Collection期刊(老文献)
Affiliation1.Jiangxi Normal Univ, Dept Phys, Nanchang 330027, Peoples R China
2.Acad Sinica, Purple Mt Observ, Nanjing 210008, Peoples R China
3.Nanjiang Normal Univ, Dept Phys, Nanjing 210097, Peoples R China
Recommended Citation
GB/T 7714
Liu, SQ,Li, XQ. Numerical analyses of self-generated magnetic fields with very small scale in solar corona[J]. ASTRONOMY & ASTROPHYSICS,2000,364(2):785-792.
APA Liu, SQ,&Li, XQ.(2000).Numerical analyses of self-generated magnetic fields with very small scale in solar corona.ASTRONOMY & ASTROPHYSICS,364(2),785-792.
MLA Liu, SQ,et al."Numerical analyses of self-generated magnetic fields with very small scale in solar corona".ASTRONOMY & ASTROPHYSICS 364.2(2000):785-792.
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