On the Energization of Pickup Ions Downstream of the Heliospheric Termination Shock by Comparing 0.52–55 keV Observed Energetic Neutral Atom Spectra to Ones Inferred from Proton Hybrid SimulationsM. Gkioulidou, Igor Baliukin, M. Opher et al.|The Astrophysical Journal Letters|2022Cited by 30
The Development of a Split-tail Heliosphere and the Role of Non-ideal Processes: A Comparison of the BU and Moscow ModelsMarc Kornbleuth, K. Dialynas, Adam Michael et al.|The Astrophysical Journal|2021Cited by 23
Probing the Length of the Heliospheric Tail with Energetic Neutral Atoms (ENAs) from 0.52 to 80 keVMarc Kornbleuth, M. A. Dayeh, M. Opher et al.|The Astrophysical Journal Letters|2023Cited by 22
The Discrepancy between Observed and Predicted Heliospheric Energetic Neutral Atoms below Solar Wind EnergyAndré Galli, J. D. Richardson, Igor Baliukin et al.|The Astrophysical Journal Letters|2023Cited by 12
Inferring the Interstellar Magnetic Field Direction from Energetic Neutral Atom Observations of the HeliotailMarc Kornbleuth, V. Izmodenov, M. Opher et al.|The Astrophysical Journal Letters|2024Cited by 7