The line response function of stellar atmospheres and the effective depth of line formation

Details The line response function of stellar atmospheres and the effective depth of line formation The line response function of stellar atmospheres and the effective depth of line formation

Aug 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975soph...43..289b&link_type=abstract

Solar Physics, vol. 43, Aug. 1975, p. 289-292.

Physics

71

Line Spectra, Optical Thickness, Spectral Line Width, Stellar Atmospheres, Stellar Spectra, Absorption Spectra, Astronomical Models, Atmospheric Turbulence, Continuous Spectra, Doppler Effect, Magnetic Effects, Stellar Magnetic Fields, Velocity Distribution

Scientific paper

The response function defines the response of line profiles to a depth
variation of such atmospheric parameters as velocity, magnetic field and
turbulence. The properties of this function are derived and compared
with the so-called contribution function.

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