Line asymmetries in CA + - Active regions

Details Line asymmetries in CA + - Active regions Line asymmetries in CA + - Active regions

Aug 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990ap%26ss.170...51h&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

2

Line Spectra, Metallicity, Photosphere, Solar Activity, Solar Spectra, Calcium, Solar Granulation, Solar Limb, Solar Magnetic Field

Scientific paper

Spatially-resolved Fe I line bisectors were studied in magnetically
active and non-active regions. In active regions, small-scale velocities
which are of convective origin, were reduced by a factor of 1.9 and
individual bisectors originating in granular-intergranular regions
showed a different behavior.

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