IPT Emission Model Data Files for MOP Community Code

Data files for the Io Plasma Torus (IPT) UV and optical emission modeling code for the Magnetospheres of Outer Planets (MOP) community. This dataset contains: Emission tables: Pre-calculated CHIANTI 11.0.2 emission rate tables for single Maxwellian (50×50 Te-ne grid) and double Maxwellian (16×8×12×10 grid) electron distributions, covering UV (550–2100 Å) and optical (3000–10000 Å) wavelengths. HDF5 format. 3D plasma model: Interpolated Jovian plasma torus model (381×381×231 grid) for line-of-sight integration calculations. HDF5 format. CHIANTI 11.0.2: Atomic database files and IDL procedures required for generating custom emission tables. For associated code and documentation, see: https://github.com/egnerney/IPT_Emission_MOP_Community_Code CHIANTI database Acknowledgment: CHIANTI is a collaborative project involving George Mason University, the University of Michigan (USA), University of Cambridge (UK) and NASA Goddard Space Flight Center (USA). https://www.chiantidatabase.org/ Dere et al. 1997; Dufresne et al. 2024