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The Kitt Peak Magnetograph III. Automation and the 40-Channel Probe

Published online by Cambridge University Press:  12 April 2016

W. Livingston ,
J. Harvey  and
C. Slaughter
W. Livingston
Affiliation:
Kitt Peak National Observatory*, Tucson, Arizona, U.S.A.
J. Harvey
Affiliation:
Kitt Peak National Observatory*, Tucson, Arizona, U.S.A.
C. Slaughter
Affiliation:
Kitt Peak National Observatory*, Tucson, Arizona, U.S.A.

Extract

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In this paper we describe the 40-channel magnetograph primarily as an example of the automated data system at the McMath Solar Telescope. The principles of the magnetograph itself have been recently given in paper I (Livingston and Harvey, 1970), while the reduction and interpretation of data is covered in paper II (Harvey and Livingston, 1970).

Type
Part II. Auxiliary Telescope Equipment
Information
International Astronomical Union Colloquium , Volume 11: Automation in Optical Astrophysics , 1971 , pp. 52 - 56
Copyright
Copyright © Royal Observatory 1971

References

Livingston, W. and Harvey, J. 1970. “The Kitt Peak Magnetograph. IV. The Fiber-Optic Probe and Results on Weak Fields”, regular paper at IAU Symposium No. 43, “Solar Magnetic Fields”, Paris, August 31-September 4, 1970.Google Scholar
Livingston, W. and Harvey, J., 1970. “The Kitt Peak Magnetograph. I. Principles of the Instrument”, submitted to Solar Phys.Google Scholar
Harvey, J. and Livingston, W., 1970. “The Kitt Peak Magnetograph. II. Reduction and Interpretation of Data”, preprint.Google Scholar
Trumbo, D. E., 1969. “Installation Notes and User’s Guide For Digital Drive Oscillator”, KPNO Eng. Dept. Tech. Rept. No. 6.Google Scholar