Abstract

A short compilation of various radio methods of the determination of magnetic fields in the solar corona is given which, completed by observations in other spectral ranges (e.g. the optical and X-ray ranges), results in a complex picture of the magnetic field. Some topics of interest are the following: (1) Comparison with a standard reference magnetic field in the solar corona, (2) Possible evidence of substantial small-scale fluctuations of the magnetic field (e.g. in active regions), (3) Indication of magnetic fields substantially in excess of the standard distribution (e.g. in limb flare events)

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