Facular points and small-scale magnetic elements

Details Facular points and small-scale magnetic elements Facular points and small-scale magnetic elements

Aug 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990ap%26ss.170....9d&link_type=abstract

(IAU, European Regional Astronomy Meeting, 11th, La Laguna, Spain, July 3-8, 1989) Astrophysics and Space Science (ISSN 0004-640

Astronomy and Astrophysics

Astrophysics

Faculae, Magnetic Field Configurations, Solar Magnetic Field, Stellar Spectra, Continuous Spectra, Magnetic Flux, Photosphere, Visible Spectrum

Scientific paper

Spectroscopic observations, with high spatial resolution, of Ca II K bright points very near the disk center are presented. Magnetic concentrations have been detected in these network (facular) points by only using intensity profiles of the well-known pair of lines Fe I 5250.22 A and 5247.06 A. No brightening of these structures with respect to the quiet photosphere can be ascertained within an accuracy threshold of 1.2 percent.

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