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)
  • 발행 : 1996.12.01

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.

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