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YoGA Ao features » Historique » Révision 3

Révision 2 (Julien Brule, 18/06/2012 14:18) → Révision 3/15 (Julien Brule, 18/06/2012 14:18)

h1. YoGA Ao features 

 The YoGA_Ao library contains routines to simulate the whole process of image formation through the atmosphere, a telescope and an adaptive optics (AO) system. Following [[ the YoGA Philosophy ]]    YoGA_Ao is designed around a double-sided API: a Yorick API (called hereafter high-level routines) and CUDA-C API accessible to the interpreter through Yorick wrappers (called hereafter advanced routines). 

 There are two ways to use YoGA_Ao, either through the GUI or through the command line possibly using predefined scripts. The following description is valid for both ways but is probably more relevant to command line users. The main difference between the GUI and the command line interface is the way the simulation parameters are imported. In the latter case, the simulation parameters are centralized into a parameter file (.par). Examples of .par files are given in the data/par directory and can be used as templates. The high-level API contains a dedicated routine to read the parameters from this file and import them in the simulation environment. 

 [[YoGA_Ao_features#List_of_features]] [[YoGA_Ao_features#List-of-features]] 

 h2. List of features