Energetic Neutral Atom Fluxes from the Heliosheath: Constraints from in situ Measurements and Models
Author:
Funder
NASA ∣ Goddard Space Flight Center
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
https://iopscience.iop.org/article/10.3847/2041-8213/ac0d5c/pdf
Reference38 articles.
1. Heliospheric energetic neutral atoms: Non-stationary modelling and comparison with IBEX-Hi data
2. SCATTER-FREE PICKUP IONS BEYOND THE HELIOPAUSE AS A MODEL FOR THE INTERSTELLAR BOUNDARY EXPLORER RIBBON
3. Mediation of the solar wind termination shock by non-thermal ions
4. ENERGETIC NEUTRAL ATOMS MEASURED BY THEINTERSTELLAR BOUNDARY EXPLORER(IBEX): EVIDENCE FOR MULTIPLE HELIOSHEATH POPULATIONS
5. The Interstellar Boundary Explorer High Energy (IBEX-Hi) Neutral Atom Imager
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1. The Plasma Pressure Contribution from Low-energy (0.05–2 keV) Energetic Neutral Atoms in the Heliosheath;The Astrophysical Journal;2024-08-01
2. Evidence of a Thick Heliopause Boundary Layer Resulting from Active Magnetic Reconnection with the Interstellar Medium;The Astrophysical Journal;2024-01-01
3. The Discrepancy between Observed and Predicted Heliospheric Energetic Neutral Atoms below Solar Wind Energy;The Astrophysical Journal Letters;2023-09-01
4. Solar wind with Hydrogen Ion charge Exchange and Large-Scale Dynamics (SHIELD) DRIVE Science Center;Frontiers in Astronomy and Space Sciences;2023-06-15
5. What is the heliopause? Importance of magnetic reconnection and measurement requirements;Frontiers in Astronomy and Space Sciences;2023-02-08
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