scholarly journals Real-time restoration of white-light confocal microscope optical sections

2007 ◽  
Vol 16 (3) ◽  
pp. 033009 ◽  
Author(s):  
Madhusudhanan Balasubramanian
2007 ◽  
Vol 227 (3) ◽  
pp. 203-215 ◽  
Author(s):  
J. H. FRANK ◽  
A. D. ELDER ◽  
J. SWARTLING ◽  
A. R. VENKITARAMAN ◽  
A. D. JEYASEKHARAN ◽  
...  

2013 ◽  
Vol 22 (06) ◽  
pp. 1360019
Author(s):  
DAMON BLANCHETTE ◽  
EMMANUEL AGU

Spectral rendering, or the synthesis of images by taking into account the constituent wavelengths of white light, enables the rendering of iridescent colors caused by phenomena such as dispersion, diffraction, interference and scattering. Caustics, the focusing and defocusing of light through a refractive medium, can be interpreted as a special case of dispersion where all the wavelengths travel along the same paths. In this paper we extend Adaptive Caustic Mapping (ACM), a previously proposed caustics mapping algorithm, to handle physically-based dispersion. Because ACM can display caustics in real-time, it is amenable to extension to handle the more general case of dispersion. We also present a novel algorithm for filling in the gaps that occur due to discrete sampling of the spectrum. Our proposed method runs in screen-space, and is fast enough to display plausible dispersion phenomena at real-time and interactive frame rates.


2019 ◽  
Vol 89 (3) ◽  
pp. 554-564.e1 ◽  
Author(s):  
Emanuele Rondonotti ◽  
Silvia Paggi ◽  
Arnaldo Amato ◽  
Giuseppe Mogavero ◽  
Alida Andrealli ◽  
...  

2014 ◽  
Author(s):  
Panagiota Petrou ◽  
Georgios Koukouvinos ◽  
Dimitrios Drygiannakis ◽  
Dimitris Goustouridis ◽  
Ioannis Raptis ◽  
...  

2006 ◽  
Author(s):  
Takashi Sakurai ◽  
Seiji Yamamoto ◽  
Atsuo Miyakawa ◽  
Yoshihiko Wakazono ◽  
Takato O. Yoshida ◽  
...  

1979 ◽  
Vol 50 ◽  
pp. 27-1-27-10 ◽  
Author(s):  
R.J. Scaddan ◽  
B.L. Morgan ◽  
J.C. Dainty

AbstractA speckle interferometer is described which has been used to measure the separations and position angles of binary star systems. The present instrument uses an image intensifier to enable the enlarged stellar images to be recorded on cine-film. The exposure time is typically 8 msec and the camera can be operated at up to 20 frames per second. The instrument incorporates a means of calibrating the magnitude difference of the binary star systems.A pair of achromatising lenses have been designed which will correct the radial chromatic dispersion in the speckle patterns and allow exposures to be made in “white” light. A system is under development which uses an image intensifier and a plumbicon television camera to acquire the data and a hard-wired autocorrelator to perform the analysis in real time. With this system the limiting magnitude of the technique should be significantly improved.


2019 ◽  
Vol 17 (31) ◽  
pp. 7360-7368 ◽  
Author(s):  
D. Sirbu ◽  
L. Zeng ◽  
P. G. Waddell ◽  
A. C. Benniston

Reaction of a julolidine-based BODIPY compound with silver(i) ions in the presence of white light produced the oxidised julolidine version (OXJUL) containing a quaternary nitrogen.


2013 ◽  
Vol 21 (22) ◽  
pp. 26192 ◽  
Author(s):  
Chien-Hung Yeh ◽  
Yen-Liang Liu ◽  
Chi-Wai Chow

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