Fast codes for computing the solar gyrosynchrotron radio emission; analytical and numerically defined electron distribution functions are supported. The codes are implemented as executable libraries (DLL or SO) callable from IDL or Python.
See the files CallingConventions.pdf, AnalyticalDistributions.pdf, and Diagram.pdf for more details and calling conventions, and the folder Examples for the usage examples. The folder Binaries contains the compiled Windows DLL and Linux SO libraries.
This is the first release of the codes (27 July 2021).