Exoplanetary and Planetary Radio Emission Simulator
The ExPRES models CMI (Cyclotron Maser Instability) driven radio emissions. It provides radio dynamic spectra observed from a defined location. Since the CMI emission process is very anisotropic, the relative geometry of the radio source and the observer drives the observability of the source. More info on the ExPRES code: ExPRES on the MASER web site. The code can be launched from the MASER run on demand interface.
The config.ini.template
file (in src) must be renamed config.ini
and edited with the adequate paths:
cdf_dist_path
must point to the local CDF distribution directory.ephem_path
is the path to the directory where the precomputed ephemerides files aremfl_path
is the path to the directory where the precomputed magnetic field line data.save_path
is the path where the data will be saved.ffmpeg_path
points to the ffmpeg
executable, e.g., /opt/local/bin/ffmpeg
ps2pdf_path
points to the ps2pdf
executable, e.g., /opt/local/bin/ps2pdf
Examples are provided in the header of config.ini.template.
The code has been tested under IDL 8.5. You must have a functional installation of IDL 8.5 (or better) on your system.
The IDL interpreter must be configured to look for routines into the src and cdawlib directories.
The operation are initiated with the following batch script:
IDL> @serpe_compile
This compiles all the necessary routines in advance. Then the simulation can be launched:
IDL> main,'file.json'
where file.json
is the input parameter file. This file must comply with the ExPRES-v1.3 JSON-shema