Wave-front tilt power spectral density from the image motion of solar pores

Details Wave-front tilt power spectral density from the image motion of solar pores Wave-front tilt power spectral density from the image motion of solar pores

Jul 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992apopt..31.4280a&link_type=abstract

Applied Optics (ISSN 0003-6935), vol. 31, no. 21, July 20, 1992, p. 4280-4284. Research supported by Lockheed Missiles and Space

Mathematics

Probability

7

Image Motion Compensation, Power Spectra, Probability Density Functions, Seeing (Astronomy), Sunspots, Wave Front Deformation, Atmospheric Turbulence, Kolmogoroff Theory, Optical Tracking, Turbulence Effects

Scientific paper

An image-stabilization system that measures wave-front tilt over a telescope aperture due to atmospheric turbulence has been constructed. This system uses small features on the sun as point sources. The wave-front tilt power spectral density has been measured with this system out to more than 500 Hz. The spectra show three distinct asymptotic slopes that do not, in general, agree with theoretical predictions based on the Kolmogorov model.

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