The contribution of high order Zernike modes to wavefront tilt.

Details The contribution of high order Zernike modes to wavefront tilt. The contribution of high order Zernike modes to wavefront tilt.

Apr 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995optco.115..417t&link_type=abstract

Opt. Commun., Vol. 115, No. 5 - 6, p. 417 - 424

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The contribution of high order Zernike modes on average phase gradient is investigated. The resulting temporal power spectra are compared to data collected using the tip/tilt servo at the Sydney University Stellar Interferometer (SUSI). The low frequency part of the power spectrum follows a -2/3 power law which is in agreement with other similar work. Due to the effect of higher order terms, the high frequency power law for average phase gradient becomes -11/3 rather than the -17/3 predicted for the 'tilt' component of the Zernike representation of the wavefront.

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