The line response function of stellar atmospheres and the effective depth of line formation |
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| Authors: | Jacques M. Beckers Robert W. Milkey |
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| Affiliation: | (1) Sacramento Peak Observatory, AFCRL, 88349 Sunspot, N.M., U.S.A.;(2) Kitt Peak National Observatory, 85726 Tucson, Ariz., U.S.A. |
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| Abstract: | 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.Operated by the Association of Universities for Research in Astronomy, Inc., under contract with the National Science Foundation. |
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