Computer Science
Scientific paper
May 1998
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998crasb.326..337p&link_type=abstract
Comptes Rendus de l'Academie des Sciences, Sér. II, Fasc. b, Tome 326, No. 5, p. 337 - 344
Computer Science
Solar Chromosphere: Structure, Solar Chromosphere: Uv Lines, Solar Chromosphere: Emission Lines
Scientific paper
The authors present the results of a statistical analysis carried out from a data base of six solar chromospheric emission lines recorded simultaneously and with high spectral resolution. An empirical and a clustering method for separating the different solar structure contributions have been used and found to be in good agreement. Mean profiles corresponding to the different populations have been built. Correlations of different parameters for each profile allowed one to deduce different properties of the solar chromosphere, such as the existence of magnetic canopies and downflows in active regions.
Bocchialini Karine
Patsourakos Spiros
Vial Jean-Claude
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