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Bright points in Ha wings and connected mass flows in the solar chromosphere

  • Session 2. The High Resolution Structure of the Sun
  • Conference paper
  • First Online:
High Resolution in Solar Physics

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

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Abstract

Many mass flows in the chromosphere are physically connected with bright photospheric points. Bidimensional spectroscopy with high spatial resolution is very well suited for the study of both kinds of structures. We give some preliminary results derived from recent observations of the MSDP at the Pic-du-Midi.

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Bibliography

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Richard Muller

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© 1985 Springer-Verlag

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Mein, P., Malherbe, J.M., Mouradian, Z., Mein, N., Muller, R. (1985). Bright points in Ha wings and connected mass flows in the solar chromosphere. In: Muller, R. (eds) High Resolution in Solar Physics. Lecture Notes in Physics, vol 233. Springer, Berlin, Heidelberg. https://doi.org/10.1007/BFb0022413

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  • DOI: https://doi.org/10.1007/BFb0022413

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  • Publisher Name: Springer, Berlin, Heidelberg

  • Print ISBN: 978-3-540-15678-9

  • Online ISBN: 978-3-540-39608-6

  • eBook Packages: Springer Book Archive

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