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  3. Interstellar Conditions Deduced from Interstellar Neutral Helium Observed by IBEX and Global Heliosphere Modeling

Interstellar Conditions Deduced from Interstellar Neutral Helium Observed by IBEX and Global Heliosphere Modeling

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DOI
10.48350/192802
Publisher DOI
10.3847/1538-4357/ace719
Abstract
In situ observations of interstellar neutral (ISN) helium atoms by the IBEX-Lo instrument on board the Interstellar Boundary Explorer (IBEX) mission are used to determine the velocity and temperature of the pristine very local interstellar medium (VLISM). Most ISN helium atoms penetrating the heliosphere, known as the primary population, originate in the pristine VLISM. As the primary atoms travel through the outer heliosheath, they charge exchange with He+ ions in slowed and compressed plasma, creating the secondary population. With more than 2.4 million ISN helium atoms being sampled by IBEX during ISN seasons 2009–2020, we compare the observations with the predictions of a parameterized model of ISN helium transport in the heliosphere. We account for the filtration of ISN helium atoms at the heliospheric boundaries by charge-exchange and elastic collisions. We examine the sensitivity of the ISN helium fluxes to the interstellar conditions described by the pristine VLISM velocity, temperature, magnetic field, and composition. We show that comprehensive modeling of the filtration processes is critical for interpreting ISN helium observations, as the change in the derived VLISM conditions exceeds the statistical uncertainties when accounting for these effects. The pristine VLISM parameters found by this analysis are the flow speed (26.6 km s−1), inflow direction in ecliptic coordinates (255fdg7, 5fdg04), temperature (7350 K), and B − V plane inclination to the ecliptic plane (53fdg7). The derived pristine VLISM He+ density is 9.7 × 10−3 cm−3. Additionally, we show a strong correlation between the interstellar plasma density and magnetic field strength deduced from these observations.
Date Issued
2023
Publication Type
Article
Subject(s)
500 Science > 530 Physics
500 Science > 520 Astronomy
600 Technology > 620 Engineering
Language(s)
en
Author(s)
Swaczyna, P.
Bzowski, M.
Heerikhuisen, J.
Kubiak, M. A.
Rahmanifard, F.
Zirnstein, E. J.
Fuselier, S. A.
Galli, André  
Space Research and Planetology Physics - Labs Planet in Situ  
Physikalisches Institut - Space Research and Planetology Physics  
Physikalisches Institut der Universität Bern  
McComas, D. J.
Möbius, E.
Schwadron, N. A.
Additional Credits
Space Research and Planetology Physics - Labs Planet in Situ  
Physikalisches Institut der Universität Bern  
Physikalisches Institut - Space Research and Planetology Physics  
Journal
Astrophysical journal
Publisher
Institute of Physics Publishing IOP
ISSN
0004-637X
Access(Rights)
open.access
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