On the Discrepancy of Coronal Magnetic Fields in Solar Optics and Radio

Chin. Phys. Lett.

1997, Vol. 14

Issue (1): 77-80 DOI:

Original Articles

On the Discrepancy of Coronal Magnetic Fields in Solar Optics and Radio

MA Yue-hua;LI Xiao-qing

Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing 210042

Cite this article:

MA Yue-hua, LI Xiao-qing 1997 Chin. Phys. Lett. 14 77-80

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Abstract The 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.

Keywords: 96.60.Pb 96.60.Hv

Published: 01 January 1997

PACS:	96.60.Pb
	96.60.Hv	(Electric and magnetic fields, solar magnetism)

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https://cpl.iphy.ac.cn/ OR https://cpl.iphy.ac.cn/Y1997/V14/I1/077

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