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Multiplier hysteresis and image motion errors in limb darkening scans obtained in April 1981 (and later)

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Abstract

In response to the comment of P. Foukal (1989) we show that in our limb darkening observations multiplier hysteresis and image motion (seeing) can be ruled out as major sources of error.

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References

  • Foukal,P.: 1989, Solar Phys.

  • Neckel, H., and Labs, D.: 1984, Solar Phys. 90, 205.

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  • Neckel, H., and Labs, D.: 1987, Solar Phys. 110, 139.

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  • Neckel, H., and Labs, D.: 1988 in “Solar Radiative Output Variations”, P. Foukal ed., p. 201.

  • Petro, L.D., Foukal, P.V., Rosen, W.A., Kurucz, R.L., and Pierce, A.K.: 1984, Astrophys.J. 283, 426.

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Authors and Affiliations

  1. Hamburger Sternwarte, Gojenbergsweg 112, 80, Hamburg, Bergedorf, F.R.G.

    Heinz Neckel

  2. Landessternwarte Königstuhl, D-6900, Heidelberg, F.R.G.

    Dietrich Labs

Authors
  1. Heinz Neckel
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  2. Dietrich Labs
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Neckel, H., Labs, D. Multiplier hysteresis and image motion errors in limb darkening scans obtained in April 1981 (and later). Sol Phys 120, 205–207 (1989). https://doi.org/10.1007/BF00148544

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  • DOI: https://doi.org/10.1007/BF00148544

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