A real-time field-sequential stereoscopic image converter

2004 ◽  
Vol 50 (3) ◽  
pp. 903-910 ◽  
Author(s):  
Chul-Ho Choi ◽  
Byong-Heon Kwon ◽  
Myung-Ryul Choi
Keyword(s):  
Real Time ◽  
Image Converter ◽  
Stereoscopic Image

New type of IR to visible real-time image converter: design and fabrication

1991 ◽  
Author(s):  
Fangkui Sun ◽  
Mao-hua Yang ◽  
Shao-hong Gao ◽  
Shi-jie Zhao
Keyword(s):  
Real Time ◽  
Image Converter ◽  
Real Time Image ◽  
New Type ◽  
Converter Design ◽  
Time Image

Real-time intensity-dependent all-optical switch of reverse image converter from wavelength to wavelength based on bacteriorhodopsin film

2005 ◽  
Vol 249 (4-6) ◽  
pp. 563-568 ◽  
Author(s):  
Guiying Chen ◽  
Chunping Zhang ◽  
Xiaodong Shang ◽  
Zongxia Guo ◽  
Xingyu Wang ◽  
...  
Keyword(s):  
Real Time ◽  
Optical Switch ◽  
Image Converter ◽  
All Optical ◽  
All Optical Switch

A New Real-Time Non-Coherent to Coherent Light Image Converter The Hybrid Field Effect Liquid Crystal Light Valve

1975 ◽  
Vol 14 (3) ◽  
Author(s):  
Jan Grinberg ◽  
Alex Jacobson ◽  
William Bleha ◽  
Leroy Miller ◽  
Lewis Fraas ◽  
...  
Keyword(s):  
Liquid Crystal ◽  
Real Time ◽  
Field Effect ◽  
Image Converter ◽  
Coherent Light ◽  
Light Image ◽  
Light Valve

Some Recent Results in Quiescent Prominence Spectrometry

1979 ◽  
Vol 44 ◽  
pp. 41-47
Author(s):  
Donald A. Landman
Keyword(s):  
Real Time ◽  
Computer System ◽  
Spectral Response ◽  
Absolute Intensity ◽  
Solar Observatory ◽  
Target Size ◽  
Small Target ◽  
Signal Averaging ◽  
Quiescent Prominence

This paper describes some recent results of our quiescent prominence spectrometry program at the Mees Solar Observatory on Haleakala. The observations were made with the 25 cm coronagraph/coudé spectrograph system using a silicon vidicon detector. This detector consists of 500 contiguous channels covering approximately 6 or 80 Å, depending on the grating used. The instrument is interfaced to the Observatory’s PDP 11/45 computer system, and has the important advantages of wide spectral response, linearity and signal-averaging with real-time display. Its principal drawback is the relatively small target size. For the present work, the aperture was about 3″ × 5″. Absolute intensity calibrations were made by measuring quiet regions near sun center.

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