Illustration of the emergent magnetic flux model: Observations of the large flare of 1981 May 16

Astronomy and Astrophysics – Astrophysics

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Scientific paper

Using the high-resolution data in white light and in Hα of the large, double-ribbon flare of 1981 May 16 obtained at Purple Mountain Observatory, we discussed the changes in the photosphere and chromosphere 8 hours before, and during the initial phase of the flare and analysed the relationship between the emergent magnetic flux, surges, dark filaments and the onset of the flare. We found that an increase in the magnetic flux with the abnormal polarity beside the neutral line produced surges, which in turn gave rise to disturbances and eruptions in the dark filament at the neutral line and led to the large flare. The emergent magnetic flux model of flares is thus verified and extended.

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