Lysak, Robert L2022-05-192022-05-192022-05-19https://hdl.handle.net/11299/227516Fortran source code for modeling ULF waves in the magnetosphereThis is the update of a three-dimensional code in dipole geometry for modeling Ultra-Low-Frequency (ULF) waves. The previous version is at https://doi.org/10.13020/d1g7-c676. This code has been used in a study of so-called Pi2 pulsations in the magnetosphere, which are waves with a period of 1-2 minutes that are commonly observed during substorms. This code has been used in conjunction with analysis of data from the Van Allen Probes mission.Attribution-NonCommercial-NoDerivs 3.0 United Stateshttp://creativecommons.org/licenses/by-nc-nd/3.0/us/ULF WavesMagnetosphere-Ionosphere CouplingCavity ModesUpdated Fortran program for modeling ULF waves in a three-dimensional magnetosphereDatasethttps://doi.org/10.13020/kbp7-dd42