This code accompanies the paper Ensemble Forecasts of Solar Wind Connectivity to 1 Rs using ADAPT-WSA, to be published in the AGU Journal Space Weather in 2023. This code plots a relative probability distribution of source locations for the solar wind at Earth. The source location is where on the surface of the sun the solar wind comes from. The methodology used here builds this relative probability distribution using Kernel Density Estimation and an ensemble approach powered by the ADAPT-WSA model.
Data for use with this code must be obtained through the Zenodo file data.tar.gz and extracted.
The author can be reached at daniel.e.dasilva@nasa.gov or mail@danieldasilva.org.