Installation.md

@@ -30,7 +30,7 @@ This directory should contain only IDL code, and nothing else.
 
 The folder structure needed for the execution of the PRISMA pipeline and detailed in the [Workspace](Workspace) page. 
 
-The complete workspace for the PRISMA pipeline is hosted in a separate repository named [PRISMA-workspace](https://www.ict.inaf.it/gitlab/dario.barghini/prisma-workspace), which is freely available to PRISMA collaborators only, since it hosts detailed information about the PRISMA stations, their location and configuration.
+The complete workspace for the PRISMA pipeline is hosted in a separate repository named [PRISMA-workspace](https://www.ict.inaf.it/gitlab/dario.barghini/prisma-workspace), which is available to PRISMA collaborators only, since it hosts detailed information about the PRISMA stations, their location and configuration.
 If you do not have access to it, the workspace is easily reproducible following the guidelines detailed in the [Workspace](Workspace) page.
 
 If you have access to it, the PRISMA-workspace repository is linked to the pipeline via a git submodule in the `workspace` folder. 
@@ -40,15 +40,14 @@ Most of the directories contained in the workspace will be empty at the beginnin
 
 # Settings
 
-After recreating the workspace, some machine-dependent modifications are needed for the PRISMA pipeline to be fully operative on your computer. 
-They are all enclosed in the [`configuration.ini`](https://www.ict.inaf.it/gitlab/dario.barghini/prisma-workspace/-/blob/main/settings/configuration.ini) file inside the settings directory of the workspace: `/your_path_to_the/workspace/settings/configuration.ini`.
+After installing the code and recreating the workspace, some machine-dependent modifications are needed for the PRISMA pipeline to be fully operative on your computer. 
+Most of them are enclosed in the [`configuration.ini`](https://www.ict.inaf.it/gitlab/dario.barghini/prisma-workspace/-/blob/main/settings/configuration.ini) file inside `(your_path_to_the)/workspace/settings/`.
 More details about this file are given in the [Settings](Settings) page.
 The configuration file in the workspace is designed for execution on the PRISMA servers.
-If you do not have access to the workspace, you can find a template [here](uploads/configuration_template.ini)
+If you do not have access to the workspace, you can find a template [here](uploads/configuration_template.ini).
 
 To make the pipeline working, you have to adjust a few fields in the configuration file.
-To do so, open [`configuration.ini`] with a text editor and modify the following:
-
+To do so, open it with a text editor and modify the following:
 
 ### Path
 
@@ -64,15 +63,28 @@ This is done to allow, for example, the raw data (captures and events) to be on
 This is a API key used for the generation and download of static background maps needed for the triangulation map of events (see [triangulation.pro](triangulation.pro)). 
 The API service is provided by [Geoapify](https://www.geoapify.com/) and it is based on [OpenStreetMap](https://www.openstreetmap.org/) tiles. 
 
-Go to the [login page](https://myprojects.geoapify.com/login) of Geoapify and generate your own API key.
+Go to the [login page of Geoapify](https://myprojects.geoapify.com/login) and generate your own API key.
 This service is free up to a usage limit of 3000 credits / day. 
 The credit price for each map is: `CP = 1 + (# tiles)/4`.
 An average of 12 tiles is needed for each PRISMA map. 
 Therefore you can generate ~750 maps / day.
 
+## Camera configuration
+
+To make the code acknowledge the *existence* of a station, a few steps are needed:
+
+- add the station CODE (e.g., `ITPI01`) and NAME (e.g., `PINOTORINESE`) to the [`solutions.ini`](https://www.ict.inaf.it/gitlab/dario.barghini/prisma-workspace/-/blob/main/settings/solutions.ini) file inside `workspace/settings/`.
+If you do not have access to the workspace, you can find a template [here](uploads/solutions_template.ini).
+- create a folder named after the camera CODE inside `/workspace/settings/configuration/`. 
+This folder must contain an initialization file in the format of `CODE.ini`, with the station and camera specification (e.g., [`ITPI01.ini`](https://www.ict.inaf.it/gitlab/dario.barghini/prisma-workspace/-/blob/main/settings/configuration/ITPI01/ITPI01_20171010.ini)).
+If you do not have access to the workspace, you can find a template here [](uploads/CODE_template.ini).
+
+More details are given in the [Settings](Settings) page.
+
 # Third-part libraries
 
 The PRISMA pipeline makes use of many external third-part IDL libraries in its code, listed here:
+
 - [The IDL Astronomy User's Library](https://idlastro.gsfc.nasa.gov/) ([GitHub](https://github.com/wlandsman/IDLAstro))
 - [Markwardt IDL Library](https://cow.physics.wisc.edu/~craigm/idl/idl.html)
 - [Coyote IDL Program Libraries](http://www.idlcoyote.com/documents/programs.php) ([GitHub](https://github.com/idl-coyote/coyote))
@@ -91,7 +103,7 @@ To install these libraries, follow the download links provided in the list and p
 
 The PRISMA pipeline uses the [NRLMSIS 2.0](https://ccmc.gsfc.nasa.gov/models/NRLMSIS~2.0/) empirical model to define the state of the atmospheric (density and temperature) within the solution of the dynamic evolution of the meteoroid in the atmosphere (see the [dynamic_model.pro](dynamic_model.pro) page). 
 NRLMSIS 2.0 is a major, reformulated upgrade of the previous version, [NRLMSISE-00](https://ccmc.gsfc.nasa.gov/models/NRLMSIS~00/). 
-To run this part of the code, you should build your own executable and place it (and other relevant files needed for the execution) in the `atmosphere/nrlmsis2.0` directory in the workspace.
+To run this part of the code, you should build your own executable and place it (and other relevant files needed for the execution) in the directory `/your_path_to_the/workspace/atmosphere/nrlmsis2.0`.
 This executable has to be named `msis20_windows.exe` for a Microsoft Windows platform or `msis20_linux.exe` for a Linux platform (the version for MacOS is not yet implemented in the pipeline). 
 Refer to the [Atmosphere](Atmosphere) page for more details.