Physics
Scientific paper
Aug 1985
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985soph...98..197b&link_type=abstract
Solar Physics (ISSN 0038-0938), vol. 98, Aug. 1985, p. 197-217.
Physics
51
Solar Activity, Solar Magnetic Field, Solar Spectra, Circular Polarization, Line Of Sight, Line Spectra, Magnetic Flux, Solar Velocity, Spectral Line Width
Scientific paper
Scatter plots of various pairs of spectral line parameters that describe the magnetic field and the line of sight velocity of an emerging flux region (EFR) are discussed in order to relate magnetic structures and the line of sight velocity field with characteristic areas of an EFR. Eleven slit settings across an EFR, with the slit located across one or more pores during moments of good seeing, are considered. Scatter plots of various spectral line parameters are used to isolate specific magnetic elements such as pores, faculae, and elements with strongly inclined field, and to relate these elements with characteristic portions of the EFR. The model dependency of the conclusions derived from comparison between observed and computed spectral line parameters is assessed.
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