High-speed rotating mirror system for wide-angle image projection.

1974 ◽  
Author(s):  
William L. Foley
2008 ◽  
Author(s):  
Guangbiao Gong ◽  
Yiquan Ji ◽  
Shanbing Zhu ◽  
Ruirui Zhang ◽  
Weimin Shen
Keyword(s):  

2019 ◽  
Vol 10 (1) ◽  
pp. 179 ◽  
Author(s):  
Hojong Choi ◽  
Jaemyung Ryu

Conventionally, a bright, very wide-angle optical system is designed as a floating type optical system that moves two or more lens groups composed of multiple lens in order to focus accurately. These have been widely used as phase detection auto focus (AF) methods within conventional digital single-lens reflex (DSLR) cameras. However, a phase detection AF optical system cannot be used when recording motion pictures. In contrast, a compact system camera (CSC) performs AF by the contrast method, where a stepper motor is used as the driving source for moving the optical lens. Nonetheless, to ensure that the focusing lens is lighter, these stepper motors should not have high torque and AF must be possible by moving only one lens. Yet, when focusing is performed with only one lens, aberration change due to focusing lens movement is magnified. Therefore, a very wide-angle optical system comprised of a half-angle of view more than 40 degrees and F of 1/4 has not been developed. Here, a very wide-angle optical system was designed with high resolving power that enables high speed AF, even in contrast mode, by moving only one lens while minimizing aberration change.


1982 ◽  
Vol 21 (4) ◽  
pp. 589 ◽  
Author(s):  
R. H. Freeman ◽  
H. R. Garcia

2013 ◽  
Vol 84 (8) ◽  
pp. 085102 ◽  
Author(s):  
J. H. Yang ◽  
X. F. Yang ◽  
L. Q. Hu ◽  
Q. Zang ◽  
X. F. Han ◽  
...  

2003 ◽  
Vol 12 (2) ◽  
Author(s):  
T. N. Dorokhova ◽  
N. I. Dorokhov

AbstractThe Mt. Dushak-Erekdag Observatory (Central Asia, Turkmenistan, 58° E longitude) is located just in the longitudes gap of asteroseismological networks. It is the southernmost observatory of the former Soviet Union, its latitude is +38°. The sky seeing at the site is one of the best in Central Asia: a low light pollution, high and stable sky transparency, over 200 usable nights per year. The altitude is above 2000 m.Odessa Astronomical Observatory has its 0.8 m telescope with a two-star high-speed photometer there, which frequently participates in international programs and multi-site campaigns. An accuracy of the photometry amounts to 1 mmag. Besides, a 1 m wide-angle telescope and a dual-tube telescope with 0.5m mirrors are installed at the observatory.The developed infrastructure at the site and the stable economy in Turkmenistan make the Mt. Dushak-Erekdag Observatory very interesting for the WET observations.


2019 ◽  
Vol 90 (9) ◽  
pp. 093502
Author(s):  
T. Farley ◽  
N. R. Walkden ◽  
F. Militello ◽  
M. Sanna ◽  
J. Young ◽  
...  

2017 ◽  
Vol 5 (1) ◽  
Author(s):  
Yayue Pan ◽  
Yong Chen ◽  
Zuyao Yu

In micro-stereolithograhy (μSL), high-speed fabrication is a critical challenge due to the long delay time for refreshing resin and retaining printed microfeatures. Thus, the mask-image-projection-based micro-stereolithograhy (MIP-μSL) using the constrained surface technique is investigated in this paper for quickly recoating liquid resin. It was reported in the literature that severe damages frequently happen in the part separation process in the constrained-surface-based MIP-μSL system. To conquer this problem, a single-layer movement separation approach was adopted, and the minimum delay time for refreshing resin was experimentally characterized. The experimental results verify that, compared with the existing MIP-μSL processes, the MIP-μSL process with single-layer movement separation method developed in this paper can build microstructures with complex geometry, with a faster build speed.


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