Signature of a Heliotail Organized by the Solar Magnetic Field and the Role of Nonideal Processes in Modeled IBEX ENA Maps: A Comparison of the BU and Moscow MHD Models

@article{Kornbleuth2021SignatureOA,
  title={Signature of a Heliotail Organized by the Solar Magnetic Field and the Role of Nonideal Processes in Modeled IBEX ENA Maps: A Comparison of the BU and Moscow MHD Models},
  author={M. Z. Kornbleuth and Merav Opher and I. I. Baliukin and Maher A. Dayeh and Eric J. Zirnstein and Matina Gkioulidou and Konstantinos Dialynas and Arnaud Galli and John D. Richardson and Vladislav Izmodenov and Gary P. Zank and Stephen Anthony Fuselier},
  journal={The Astrophysical Journal},
  year={2021},
  volume={921}
}
Energetic neutral atom (ENA) models typically require post-processing routines to convert the distributions of plasma and H atoms into ENA maps. Here we investigate how two kinetic-MHD models of the heliosphere (the BU and Moscow models) manifest in modeled ENA maps using the same prescription and how they compare with Interstellar Boundary Explorer (IBEX) observations. Both MHD models treat the solar wind as a single-ion plasma for protons, which include thermal solar wind ions, pick-up ions… 

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