Skip to content

ubsuny/MLFringe-Contrast-CP2P2024

Repository files navigation

MLFringe-Contrast-CP2P2024

this is the project for CP2 spring 2024, The purpose of this project is to find fringe contrast or visibility for PGMI setup using K-space model. The one PGMI and two PGMI setups intensity has been reproduced. The codes are given, also the codes for contrast for two PGMI is given. the contrast is plotted as a function of d, (distance between two gratings).

About

this is the project for CP2 spring 2024

Resources

License

Stars

Watchers

Forks

Releases

No releases published

Packages

No packages published