ON THE DISCREPANCY OF CORONAL MAGNETIC FIELDS IN SOLAR OPTICS AND RADIO

YUE-HuA MA; XIAO-QING LI

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ON THE DISCREPANCY OF CORONAL MAGNETIC FIELDS IN SOLAR OPTICS AND RADIO KCI 등재 SCOPUS

YUE-HuA MA, XIAO-QING LI

언어ENG
URLhttps://db.koreascholar.com/Article/Detail/387908

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천문학회지 (Journal of The Korean Astronomical Society)

제29권 제S호 (1996.12)
pp.309-311

한국천문학회 (Korean Astronomical Society)

초록

It is analysed the discrepancy about the coronal magnetic field between solar optic and solar radio using magnetic fibril concept with filling factor and fractal structure model. The magnetic field of ~ 100 G considered in solar optics is mean value in a large scale, and that of ~1000 G in solar should be the value of fine structures inside 'macro' loop.

저자

YUE-HuA MA(Purple Mountain Observatory, Academia Sinic)
XIAO-QING LI(Purple Mountain Observatory, Academia Sinic)

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