Skip to main content

Observations of Ellerman bombs in Hα

  • Session 4. The Surface fine structure as a Probe of the Solar Interior
  • Conference paper
  • First Online:
  • 121 Accesses

Part of the book series: Lecture Notes in Physics ((LNP,volume 233))

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.

This is a preview of subscription content, log in via an institution.

Preview

Unable to display preview. Download preview PDF.

Unable to display preview. Download preview PDF.

References

Download references

Author information

Authors and Affiliations

Authors

Editor information

Richard Muller

Rights and permissions

Reprints and permissions

Copyright information

© 1985 Springer-Verlag

About this paper

Cite this paper

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

Download citation

  • DOI: https://doi.org/10.1007/BFb0022429

  • Published:

  • Publisher Name: Springer, Berlin, Heidelberg

  • Print ISBN: 978-3-540-15678-9

  • Online ISBN: 978-3-540-39608-6

  • eBook Packages: Springer Book Archive

Publish with us

Policies and ethics