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

In response to the comment of P. Foukal (1989), it is shown that, in the limb-darkening observations, multiplier hysteresis and image motion (seeing) can be ruled out as major sources of error.

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Bibliographic Details
Published inSolar physics Vol. 120; no. 1; pp. 205 - 207
Main Authors NECKEL, H, LABS, D
Format Journal Article
LanguageEnglish
Published Boston, MA Reidel 01.01.1989
Dordrecht
Subjects
Astronomy
Earth, ocean, space
Exact sciences and technology
Fundamental astronomy and astrophysics. Instrumentation, techniques, and astronomical observations
Observation and data reduction techniques. Computer modeling and simulation
Multiplier
Solar limb
Darkening
Hysteresis
Photometry
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Summary:In response to the comment of P. Foukal (1989), it is shown that, in the limb-darkening observations, multiplier hysteresis and image motion (seeing) can be ruled out as major sources of error.
Bibliography:ObjectType-Article-2
SourceType-Scholarly Journals-1
ObjectType-Feature-1
content type line 23
ISSN:0038-0938
1573-093X
DOI:10.1007/BF00148544