The wavelength dependence of seeing

Details The wavelength dependence of seeing The wavelength dependence of seeing

Jul 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978josa...68..877b&link_type=abstract

Optical Society of America, Journal, vol. 68, July 1978, p. 877-883.

Physics

Optics

26

Angular Resolution, Atmospheric Optics, Atmospheric Turbulence, Infrared Astronomy, Telescopes, Turbulence Effects, Atmospheric Models, Inhomogeneity, Limb Darkening, Parametric Frequency Converters, Solar Limb, Wavelengths

Scientific paper

The deleterious effects of atmospheric inhomogeneities on telescope angular resolution (seeing effects) were studied at a wavelength of 10 microns with an imaging upconverter. Seeing was found to be systematically better by a factor of 1.9 at 10 microns than in the visible, in good agreement with theoretical predictions. A discussion of the theory of astronomical seeing is included.

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