home.md

@@ -7,11 +7,14 @@ function for the current.
 
 The equations and models used in GRAY to compute Gaussian beam propagation, absorption and current drive are summarized in the [Physics](Physics-model) section.
 
-The main development version of the source code is currently managed under a Git [repository](https://maxwell.ydns.eu/git/istp/gray), which allows to compile the code as a stand-alone executable or as a library to be called from within the [JINTRAC](https://git.ccfe.ac.uk/jintrac/jetto-sanco) suite.
+The main development version of the source code is currently managed under a Git [repository](https://maxwell.ydns.eu/git/istp/gray), and it is available  as a stand-alone executable or as a library to be called from within the [JINTRAC](https://git.ccfe.ac.uk/jintrac/jetto-sanco) suite.
 
-Two forks of the code happened in the past, in the process of developing the interface for [integrated modelling](https://wpcd-workflows.github.io)  workflows, and they are currently maintained in different repositories:
+For such version of GRAY, we provide here:
+- Instructions to obtain and install the code
+- Description of the [interface](Interface)
+- Description of the [code parameters](Code-parameters), [input](Input-data) and [output](Output-data) data.
+
+Two forks of the code happened in the past, in the process of developing the interface for the EUROfusion [Integrated Modelling](https://wpcd-workflows.github.io)  workflows, and they are currently maintained in different repositories:
 
 - [IMAS version at EUROfusion](https://gforge-next.eufus.eu/svn/gray)
 - [IMAS version at ITER](https://git.iter.org/projects/HEAT/repos/gray/)
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-
-For the main development version of GRAY, we provide here a complete description of the code [parameters](Code-parameters), [input](Input-data) and [output](Output-data) data.
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