X-Ray Forum for NDT Users
It is currently 26.12.2024, 18:17

All times are UTC + 1 hour




Post new topic Reply to topic  [ 2 posts ] 
Author Message
PostPosted: 19.11.2019, 10:35 
Offline
User avatar

Joined: 19.10.2019, 15:47
Posts: 137
The detail visibility is about ½ of image unsharpness (in a "normal" image with "standard noise").
Image Unsharpness (UIm) depends on
- Focal Spot size (FS)
- Spatial Detector Resolution (SRb)
- geometric magnification (v) [hint: "v" for magnification is taken out of ASTM E1000; in German language magnificaiton is Vergroesserung]
This three factors are in the formula for image unsharpness in ASTM E1000:
Image Formula [1]
The two factors in the square root contains the tube and the detector and the magnification. With given tube and detector the magnification is the variable which can be used to optimize the detail visibility or minimum defect discernable. In E1000 is a graph in which the detail visibility is normalized to the detector unsharpness Uf or the visibility of the system with no magnification (v=1) - as used with films before:

The different lines in the graph show different relation ships between focal spot size (phi) and detector unsharpness Uf. With a large focal spot - in the graph [(phi)/Uf=8] already a small magnification will lead to a higher unsharpness as the detector unsharpness. As the film is really sharp but need high dose, large focal spots are used for film exposure and the film is normally in close contact with the object to be inspected. With a small focal spot the lines decrease and details smaller than the detector resolution will be visible. µ-focus systems use high magnifications with very small focal spots for electronic inspection where resolutions in µm range are required.

If we look at the two extremas, we get a better feeling for what is in the graph.
1. No magnification (v=1) [object directly on detector like with film]. In Formula [1] the factor with the focalspot size FS (or [phi]) is Zero as at v=1 the quotient in front of FS is zero.

Finally the Image Unsharpness of the system is the detector unsharpness or two times the spatial resolution of the detector (SRb).

2. Very high magnification (v>>100) [object very close to tube head]. In Formula [1] the factor with the detector unsharpness decreases with the magnification and it becomes infinitesimal small. The quotient in front of the FS mutates to 1.

Finally with very high magnifications the Image Unsharpness of the system is the focal spot size FS.

Between this two extrema all X-ray applications are settled. Having in mind that the it is obvious the small focal spots give only low dose.


Last edited by Klaus on 24.11.2019, 16:32, edited 2 times in total.

Top
 Profile  
Reply with quote  
PostPosted: 19.11.2019, 18:01 
Offline
User avatar

Joined: 19.10.2019, 15:47
Posts: 137
Higher unsharpness could spoil the visibility of indications if noise is in the image (and in which X-ray image is no noise ;) ).


Top
 Profile  
Reply with quote  
Display posts from previous:  Sort by  
Post new topic Reply to topic  [ 2 posts ] 

All times are UTC + 1 hour


Who is online

No registered users


Similar topics

Detail visibility - contrast to noise ratio
Forum: Image Quality Parameters
Author: Klaus
Replies: 1

You cannot post new topics in this forum
You cannot reply to topics in this forum
You cannot edit your posts in this forum
You cannot delete your posts in this forum

Search for:
Jump to:  
cron



Hosted by iphpbb3.com

Impressum | Datenschutz