WPI #120
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WPI #120
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Changed the EKEV, EBND, WE, and DE variables to be 2 dimensional with the first dimension being the species. Now each species can have their own energy grid range. This is in preperation for being able to simulate relativistic electrons
Update to the restart, initialization, and satellite routines to correctly handle the species dependent energy grids
Added an initialization file that includes the radiation belt electrons (1 MeV to 10 MeV) based on the work done by Xingzhi.
Added interpolation on intial read for the energy and pitch angles, but currently pitch angle interpolation does not work as we do not store the pitch angle bins in the initialization or restart files
Updated the initialization file to include a larger range of electron energies for both the default electron species and the rad belt electron species
Removed negatives from fluxes in the initialization file, also fixed an issue with the satellite outputs not having the correct energy grids
…energy_by_species
There have been several updates since I started this branch, these changes bring us to a working point with the current upstream changes
…iss and input_ram/BAS_bavDxx, respectively.
Change paths for hiss and BAS chorus diffusion files
coefficients tensors
…boundary condition
New bav files
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This branch was originally forked from Miles' repository and updates the energy_by_species branch. It includes modifications and additions related to the WPI simulations work