PMO OpenIR  > 近地天体探测和太阳系天体研究团组
On the discrepancy of coronal magnetic fields in solar optics and radio
Ma, YH; Li, XQ
1997
Source PublicationCHINESE PHYSICS LETTERS
ISSN0256-307X
Volume14Issue:1Pages:77-80
Corresponding AuthorMa, YH()
AbstractThe discrepancy on the coronal magnetic field between solar optics and radio is analysed by using magnetic fibril concept with filling factor and fractal structure model. The magnetic field of about 100 G considered in solar optics is the mean value in a large scale, and that of about 1000 G in solar radio should be the value of fine structures inside ''macro'' loop.
WOS KeywordX-RAY ; ELECTRONS ; FLARES
Indexed BySCI
Language英语
WOS Research AreaPhysics
WOS SubjectPhysics, Multidisciplinary
WOS IDWOS:A1997WP24200021
PublisherALLERTON PRESS INC
Citation statistics
Cited Times:2[WOS]   [WOS Record]     [Related Records in WOS]
Document Type期刊论文
Identifierhttp://libir.pmo.ac.cn/handle/332002/8387
Collection近地天体探测和太阳系天体研究团组
Corresponding AuthorMa, YH
AffiliationCHINESE ACAD SCI,PURPLE MT OBSERV,NANJING 210042,PEOPLES R CHINA
Recommended Citation
GB/T 7714
Ma, YH,Li, XQ. On the discrepancy of coronal magnetic fields in solar optics and radio[J]. CHINESE PHYSICS LETTERS,1997,14(1):77-80.
APA Ma, YH,&Li, XQ.(1997).On the discrepancy of coronal magnetic fields in solar optics and radio.CHINESE PHYSICS LETTERS,14(1),77-80.
MLA Ma, YH,et al."On the discrepancy of coronal magnetic fields in solar optics and radio".CHINESE PHYSICS LETTERS 14.1(1997):77-80.
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