Abstract
Monochromatic rasters of six EUV lines taken in the centre of a coronal hole are analysed and the cell-network structure at different heights in the solar atmosphere is shown. Also a comparison with the average cell-centre and network intensities of another coronal hole is performed showing a good agreement between the two.
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Calamai, G., Drago, F.C. & Pettini, G. Analysis of the supergranulation structure in coronal holes. Sol Phys 65, 167–170 (1980). https://doi.org/10.1007/BF00151390
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DOI: https://doi.org/10.1007/BF00151390