Abstract
A developing active region near the center of the solar disk was observed for 80min at the center and the wings of Hα. Ellerman bombs lying below an arch filament system (AFS) and near sunspots were studied at H -1Å and H -0.75Å. We found that 50% of the bombs appear and desappear in pairs, the axis of each pair forming a small angle with the magnetic field lines of force as evidenced by the AFS, in addition the members of each pair show proper motions with an average relative velocity of 600m/sec. This behaviour suggests their association with bipolar emerging magnetic flux tubes. The average contrast (1.29), lifetime (19 minutes), size (0″.96 x 0″.58) and flux of some 70 bombs was also determined. We find evidence of an increase of the size with height and a fluctuation of the flux with time.
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© 1985 Springer-Verlag
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Zachariadis, T., Alissandrakis, C.E., Banos, G. (1985). Observations of Ellerman bombs in Hα. In: Muller, R. (eds) High Resolution in Solar Physics. Lecture Notes in Physics, vol 233. Springer, Berlin, Heidelberg. https://doi.org/10.1007/BFb0022429
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DOI: https://doi.org/10.1007/BFb0022429
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