Variation of the profiles of medium-strong photospheric lines with heliographic latitude

Details Variation of the profiles of medium-strong photospheric lines with heliographic latitude Variation of the profiles of medium-strong photospheric lines with heliographic latitude

Mar 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978soph...57...13c&link_type=abstract

Solar Physics, vol. 57, Mar. 1978, p. 13-17. Research supported by the Consiglio Nazionale delle Ricerche.

Physics

4

Latitude, Line Spectra, Photosphere, Solar Spectra, Line Shape, Temperature Effects, Velocity Distribution

Scientific paper

The asymmetric profiles of 11 metallic lines are studied, at mu equals
0.3, as functions of heliographic latitude. Their variations cannot be
interpreted as due to temperature effects, but might imply a dependence
on heliographic latitude of the photospheric velocity field.

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