maserlib / ExPRES

Exoplanetary and Planetary Radio Emission Simulator
MIT License
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Exoplanetary and Planetary Radio Emission Simulator (ExPRES) V1.3.0

ascl:1902.009 DOI Documentation Status License: MIT

Introduction

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.

Reference: Louis et al., ExPRES: a Tool to Simulate Exoplanetary and Planetary Radio Emissions, A&A 627, A30 (2019)

Repository Description

Directories

Configuration

The config.ini.template file (in src) must be renamed config.ini and edited with the adequate paths:

Examples are provided in the header of config.ini.template.

Running the code

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