Usually several Bright Eye problems are handled by a single analysis program. In many cases, for example, all spectra recorded inline in the deposition vacuum can be analyzed by a single instance of the bright_eye_inline.exe program. In such a case the analysis program reads (when it is started) the file code.wcd (see below in the section about Bright Eyes) which contains the optical model. To prepare the analysis for the individual Bright Eye stations, a fit parameter set specific to the individual bright eye is loaded (it must have the name fit_parameters.fps, see below) . This is much faster than to load a new CODE configuration each time an analysis for a different bright eye is to be started.
The bright_eye_inline.ini file tells the bright_eye_inline.exe program which Bright Eyes are to be watched and analyzed, and how this should be done. Here is an example:
Window title
Inline analysis
Product
Demo
Number of bright eyes
8
Name 1
BE1
Previous 1
Time limit 1
2.5
Name 2
BE2
Previous 2
BE1
Time limit 2
2.5
Name 3
BE3
Previous 3
BE2
Time limit 3
2.5
Name 4
BE4
Previous 4
BE3
Time limit 4
2.5
Name 5
BE5
Previous 5
BE4
Time limit 5
1.5
Name 6
BE6
Previous 6
BE5
Time limit 6
2.5
Name 7
BE7
Previous 7
BE6
Time limit 7
2.5
Name 8
BE8
Previous 8
BE7
Time limit 8
2.5
Comments:
•The window title appears in the caption of the bright_eye_inline.exe program
•The number of bright eyes defines the number of bright eyes.
•For each bright eye you have to define its name, the name of the previous bright eye and the maximum time (Time limit) for the analysis. If you specify a previous bright eye, the program will look up results obtained by the previous station for the current pane and use these values for the fit to be performed. This way partial results obtained by the individual stations are transferred through the system.
Bright_eye_inline.exe will read the ini-file and use the information for its configuration.