Astronomy and Astrophysics – Astrophysics
Scientific paper
Apr 1981
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981a%26a....97...75s&link_type=abstract
Astronomy and Astrophysics, vol. 97, no. 1, Apr. 1981, p. 75-78.
Astronomy and Astrophysics
Astrophysics
20
Faculae, Line Spectra, Solar Magnetic Field, Solar Spectra, Sunspots, Correlation, Magnetic Flux
Scientific paper
In a sunspot the measured magnetic fields are in agreement for all 12 lines observed, indicating the reliability of the observational method used. On the other hand, the discrepancies between the fields observed in 12 different lines are quite large for faculae, which is a characteristic of unresolved structures. There is, however, a good correlation between the measured magnetic field and the equivalent width of the corresponding line. An analysis in terms of 'relative magnetic curve of growth' is proposed. Application to star spots is discussed.
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