Center-to-limb variations in the two-dimensional contrast of photospheric faculae

Details Center-to-limb variations in the two-dimensional contrast of photospheric faculae Center-to-limb variations in the two-dimensional contrast of photospheric faculae

Apr 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984soph...91..243c&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 91, April 1984, p. 243-258.

Physics

13

Faculae, Photosphere, Solar Magnetic Field, Semiempirical Equations, Solar Limb, View Effects

Scientific paper

The center-to-limb appearance of a facular flux tube is presently sought by means of the semiempirical model of Osherovich et al. (1983), which is in magnetohydrostatic equilibrium and includes tension forces. The results of this model's application are presented as contour maps, cross sections of the contrast on axis, and integrated contrast as a function of viewing angle. It is noted that these results are in keeping with those of Caccin and Severino (1979), but not with the observations of Chapman and Klabunde (1982).

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