Photometric System For Charge-Coupled Device (CCD) Imaging

Author(s):  
R. Schild ◽  
S. Kent
1998 ◽  
Vol 14 (03) ◽  
pp. 202-213
Author(s):  
Clifford J. Mugnier

A problem in modular shipbuilding is the lack of a reliable, low-cost method of obtaining and utilizing dimensional control in 3D. Photogrammetry has been successfully used as a tool for this application, but because of the large number of systematic errors associated with film-based cameras, only very large shipyards are using it. Recently, developments in Charge Coupled Device (CCD) imaging arrays for cameras have allowed some success in applying photogrammetric techniques dimensional control Mainstream photogrammetric software and hardware configurations have been expensive and complicated. Digital camera systems and computers were purchased and programmed to tie existing inexpensive software packages with Geometric Dilution of Control (GDOP) error propagation analysis, originally designed for topographic mapping, into a tool for production shipyard fabrication dimensional control.


1981 ◽  
Author(s):  
F. L. Roesler ◽  
F. Scherb ◽  
R. Oliversen ◽  
K. Jaehnig ◽  
T. Williams ◽  
...  

2011 ◽  
Vol 78 (2) ◽  
pp. 604-606 ◽  
Author(s):  
Michael J. Tessaro ◽  
Sameh S. M. Soliman ◽  
Manish N. Raizada

ABSTRACTA whole-cell biosensor for glutamine (GlnLux) was constructed by transforming anEscherichia coliglutamine (Gln) auxotroph with a constitutiveluxreporter gene. Measurements of Gln in plant extracts using GlnLux correlated with quantification using high-performance liquid chromatography (Spearman'sr= 0.95). GlnLux permitted charge-coupled-device (CCD) imaging of Gln from whole plant organs.


Author(s):  
M. E. Mochel ◽  
J. M. Mochel

A liquid nitrogen cooled charge coupled device (CCD) camera with DEC 11-73 computer has been fitted to the Vacuum Generators HB5 scanning transmission electron microscope (STEM). Typically, diffraction patterns are produced in the VG HB5 STFM by rocking the beam on the sample or alternatively by rastering the electrons that emerge from the sample and displaying the resultant scanned image on the CRT. The image is often noisy because the beam current is small (≈1010 a) and the range of interesting intensities is large.


Author(s):  
M.H. White ◽  
D.R. Lampe ◽  
F.C. Blaha ◽  
I.A. Mack

1989 ◽  
Vol 8 ◽  
pp. 631-634
Author(s):  
D.A. Hunter ◽  
H.C. Harris ◽  
W.A. Baum ◽  
J.H. Jones ◽  
T.J. Kreidl

The Wide-Field and Planetary Camera (WF/PC) is a CCD imaging instrument which is part of the Hubble Space Telescope. Ground-based observations have been made with a CCD system similar to those of the WF/PC in order to establish the standard star sequence to be used for in-flight photometric calibration. Because the WF/PC passbands differ from those in previous photometric use, the filters and CCDs will define a new photometric system. We outline here the procedures used to establish the calibration fields to be used in flight (see Harris et al. 1988 for additional details).


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