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An Automated DIMM Telescope for Antarctica

  • Michael A. Dopita (a1), Peter R. Wood (a1) and Gary R. Hovey (a1)

Abstract

A knowledge of the on-ice seeing is a key requirement for planning future Antarctic observatories. In this paper we discuss the likely negative impact on seeing produced by the development of the deep winter surface temperature inversion (Ekman layer). The Automated Astronomical Site Testing Observatory (AASTO) will deploy, as one of its complement of site-testing instruments, an automated differential image motion monitor (DIMM) telescope designed to generate seeing data throughout the Antarctic winter. Here we describe the multi-aperture concept which has been developed for this mission, and touch upon some of the critical technological considerations associated with the low power budget and with the requirement of autonomous operation at very low temperature (–90°C).

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Copyright

References

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Bally, J., et al. 1996, PASA, 13, 22
Neff, W. D., & Hall, F. F. Jr 1976a, Preprint Volume, 17th Radar Meteorological Conference (Boston: American Meteorological Society), 397
Neff, W. D., & Hall, F. F. Jr 1976b, Antarctic J. US, 11, 143
Neff, W. D., & Hall, F. F. Jr 1978, Preprint Volume, 4th Symposium on Meteorological Observations and Instrumentation, (Boston: American Meteorological Society), 357
Neff, W. D., Ramm, H. E., & Hall, F. F. Jr 1977, Antarctic J. US, 12, 167
Roddier, F. 1981, Prog. Optics, XIX, 281
Sarazin, M., & Roddier, F. 1990, AA, 227, 294
Schwertfeger, W. 1984, Weather and Climate of the Antarctic (New York: Elsevier)
Storey, J. W. V., Ashley, M. C. B., & Burton, M. G. 1996, PASA, 13, 35
Zilitinkevich, S. S. 1972, Boundary-Layer Meteorology, 3, 141

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