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

  • MA YUE-HuA (Purple Mountain Observatory, Academia Sinic) ;
  • LI XIAO-QING (Purple Mountain Observatory, Academia Sinic)
  • Published : 1996.12.01

Abstract

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.

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