Bibcode
Bonet, J. A.; Marquez, I.; Vazquez, M.; Woehl, H.
Referencia bibliográfica
Astronomy and Astrophysics (ISSN 0004-6361), vol. 198, no. 1-2, June 1988, p. 322-330.
Fecha de publicación:
6
1988
Número de citas
23
Número de citas referidas
19
Descripción
The temporal and spatial behaviour of the K I 769.9 nm solar line are
investigated using several series of high spectral resolution low-noise
photoelectric scans obtained at Kitt Peak National Observatory in quiet
and active (plages and sunspots) regions. Corrections due to the
instrumental profile were applied to yield the best line shape. A
systematic center-to-limb investigation of the behaviour of the line
shape was performed in quiet regions. Power and phase spectra of the
main parameters defining the line shape have also been determined.
Within several umbrae at different cos θ positions, an inverse
C-shape or even an "S"-shape of the bisectors was found.