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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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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