Scanning pupil approach to aspheric surface slope error tolerancing in head-up display optics

2015 ◽  
Author(s):  
V. P. Sivokon
2010 ◽  
Vol 2010 ◽  
pp. 1-9 ◽  
Author(s):  
Sheng Yuan ◽  
Matthew Church ◽  
Valeriy V. Yashchuk ◽  
Kenneth A. Goldberg ◽  
Richard S. Celestre ◽  
...  

We present details of design of elliptically bent Kirkpatrick-Baez mirrors developed and successfully used at the advanced light source for submicron focusing. A distinctive feature of the mirror design is an active temperature stabilization based on a Peltier element attached directly to the mirror body. The design and materials have been carefully optimized to provide high heat conductance between the mirror body and substrate. We describe the experimental procedures used when assembling and precisely shaping the mirrors, with special attention paid to laboratory testing of the mirror-temperature stabilization. For this purpose, the temperature dependence of the surface slope profile of a specially fabricated test mirror placed inside a temperature-controlled container was measured. We demonstrate that with active mirror-temperature stabilization, a change of the surrounding temperature by more than 3 K does not noticeably affect the mirror figure. Without temperature stabilization, the rms slope error is changed by approximately 1.5 μrad (primarily defocus) under the same conditions.


Solar Energy ◽  
2020 ◽  
Vol 195 ◽  
pp. 461-474 ◽  
Author(s):  
Ye Wang ◽  
Daniel Potter ◽  
Charles-Alexis Asselineau ◽  
Clotilde Corsi ◽  
Michael Wagner ◽  
...  

1998 ◽  
Vol 5 (3) ◽  
pp. 797-800 ◽  
Author(s):  
Riccardo Signorato ◽  
Olivier Hignette ◽  
José Goulon

The angular acceptance of piezoelectric (Pzt) bimorph mirrors is limited by the maximum length of commercially available Pzt ceramic plates. To overcome this limit and manufacture longer devices, several (2n + 1) 150 mm-long bimorph Pzt stacks were assembled side-to-side. Two prototype mirrors, 450 (n = 1) and 750 (n = 2) mm long, were designed, assembled, polished and optically characterized. They are fully UHV compatible and are now installed in the monochromatic section of the ESRF beamlines ID26 and ID32. Both mirrors cover the full range of required bending radii (1 km concave–3.5 km convex). Junctions between segments do not spoil the optical surface quality. The surface slope error r.m.s. can be kept well below 1 arcsec over the full bending range. Adaptive compensation for low-frequency figure errors was shown to be easy and reliable. After compensation, residual shape errors are of the order of 40 nm r.m.s. over 700 mm.


2018 ◽  
Author(s):  
Ye Wang ◽  
Daniel Potter ◽  
Charles-Alexis Asselineau ◽  
Clotilde Corsi ◽  
Michael Wagner ◽  
...  

1980 ◽  
Vol 102 (4) ◽  
pp. 305-315 ◽  
Author(s):  
L. Wen ◽  
L. Huang ◽  
P. Poon ◽  
W. Carley

Different analytical methods for computing the flux distribution on the focal plane of a paraboloidal solar concentrator are reviewed. An analytical solution in algebraic form is also derived for an idealized model. The effects resulting from using different assumptions in the definition of optical parameters used in these methodologies are compared and discussed in detail. These parameters include solar irradiance distribution (limb darkening and circumsolar), reflector surface specular spreading, surface slope error, and concentrator pointing inaccuracy. The type of computational method selected for use depends on the maturity of the design and the data available at the time the analysis is made.


2005 ◽  
Vol 76 (5) ◽  
pp. 053103
Author(s):  
L. Gavinho ◽  
C. Cusatis ◽  
I. Mazzaro ◽  
G. Tirao

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