Model observers low contrast detectability performance at different kV levels in CT phantom images

2014 ◽  
Vol 30 ◽  
pp. e18-e19
Author(s):  
I. Hernandez-Giron ◽  
A. Calzado ◽  
J. Geleijns ◽  
R.M.S. Joemai ◽  
W.J.H. Veldkamp
Keyword(s):  
2015 ◽  
Vol 31 (7) ◽  
pp. 798-807 ◽  
Author(s):  
I. Hernandez-Giron ◽  
A. Calzado ◽  
J. Geleijns ◽  
R.M.S. Joemai ◽  
W.J.H. Veldkamp
Keyword(s):  

2018 ◽  
Vol 52 ◽  
pp. 61
Author(s):  
Luca Bellesi ◽  
Rolf Wyttenbach ◽  
Diego Gaudino ◽  
Maria Antonietta Piliero ◽  
Francesco Pupillo ◽  
...  

2019 ◽  
Vol 64 ◽  
pp. 89-97 ◽  
Author(s):  
Raffaele Villa ◽  
Nicoletta Paruccini ◽  
Antonia Baglivi ◽  
Michele Signoriello ◽  
Roberto Alejandro Montezuma Velasquez ◽  
...  
Keyword(s):  

2015 ◽  
Author(s):  
Alexandre Ba ◽  
Damien Racine ◽  
Julien G. Ott ◽  
Francis R. Verdun ◽  
Sabine Kobbe-Schmidt ◽  
...  

2000 ◽  
Vol 179 ◽  
pp. 403-406
Author(s):  
M. Karovska ◽  
B. Wood ◽  
J. Chen ◽  
J. Cook ◽  
R. Howard

AbstractWe applied advanced image enhancement techniques to explore in detail the characteristics of the small-scale structures and/or the low contrast structures in several Coronal Mass Ejections (CMEs) observed by SOHO. We highlight here the results from our studies of the morphology and dynamical evolution of CME structures in the solar corona using two instruments on board SOHO: LASCO and EIT.


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