U.S. patents available from 1976 to present.
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Wavefront error estimation derived from observation of arbitrary unknown extended scenes

Patent 5350911 Issued on September 27, 1994. Estimated Expiration Date: Icon_subject April 9, 2013. Estimated Expiration Date is calculated based on simple USPTO term provisions. It does not account for terminal disclaimers, term adjustments, failure to pay maintenance fees, or other factors which might affect the term of a patent.

Patent References

Piston error estimation method for segmented aperture optical systems while observing arbitrary unknown extended scenes
Patent #: 5128530
Issued on: 07/07/1992
Inventor: Ellerbroek, et al.

Feedback controlled optics with wavefront compensation Patent #: 5265034
Issued on: 11/23/1993
Inventor: Breckenridge, et al.

Inventors

Application

No. 045841 filed on 04/09/1993

US Classes:

250/201.9, Light beam wavefront phase adaptation356/121LAMP BEAM DIRECTION OR PATTERN

Examiners

Primary: Nelms, David C.
Assistant: Shami, K.

Attorney, Agent or Firm

International Class

G01J 001/20

Abstract

An extended scene wavefront sensing apparatus and procedure that separates (deconvolves) scene effects from wavefront errors of an optical or similar system. The present wavefront sensing apparatus and procedure uses a point source wavefront slope sensor in scene scanning mode and estimates wavefront errors by using a cross-correlation or cross-coherence procedure that operates on the outputs of the point source wavefront slope sensor. A signal processing procedure employed by the point source wavefront slope sensor provides output signals corresponding to wavefront slopes at forward optics pupil locations geometrically projected to the location of the transmission and reflection measurement plane detector pairs. During the scanning process, each of the detector pairs (equivalent to a subaperture) measures the effects of the local unchanging wavefront error in the forward optical system and temporal variations due to the scanning scene. By cross correlating or cross-cohering each detector pair's temporal difference with differences from selected reference detector pairs, the scene induced variations in the measurement are eliminated, thereby leaving the stationary wavefront error component of the measurement. The lead/lag time in the temporal differences output between detector pairs and reference detector pairs are then used to estimate the wavefront slope differences between equivalent subapertures. The wavefront slope differences are used in a reconstructor to generate wavefront errors or wavefront slope errors, except for an unobservable global tilt.

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