Interstellar Neutral Helium in the Heliosphere from IBEX Observations. VI. The He + Density and the Ionization State in the Very Local Interstellar Matter

Bzowski, M.; Czechowski, A.; Frisch, P. C.; Fuselier, S. A.; Galli, André; Grygorczuk, J.; Heerikhuisen, J.; Kubiak, M. A.; Kucharek, H.; McComas, D. J.; Möbius, E.; Schwadron, N. A.; Slavin, J.; Sokół, J. M.; Swaczyna, P.; Wurz, Peter; Zirnstein, E. J. (2019). Interstellar Neutral Helium in the Heliosphere from IBEX Observations. VI. The He + Density and the Ionization State in the Very Local Interstellar Matter. Astrophysical journal, 882(1), p. 60. Institute of Physics Publishing IOP 10.3847/1538-4357/ab3462

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Interstellar neutral gas atoms penetrate the heliopause and reach 1 au, where they are detected by Interstellar
Boundary Explorer (IBEX). The flow of neutral interstellar helium through the perturbed interstellar plasma in the
outer heliosheath (OHS) results in the creation of a secondary population of interstellar He atoms, the so-called
Warm Breeze, due to charge exchange with perturbed ions. The secondary population brings the imprint of the
OHS conditions to the IBEX-Lo instrument. Based on a global simulation of the heliosphere with measurementbased
parameters and detailed kinetic simulation of the filtration of He in the OHS, we find the number density of
the interstellar He+ population to be (8.98±0.12)×10−3 cm−3. With this, we obtain the absolute density of
interstellar H+ as 5.4×10−2 cm−3 and that of electrons as 6.3×10−2 cm−3, with ionization degrees of 0.26 for H
and 0.37 for He. The results agree with estimates of the parameters of the Very Local Interstellar Matter obtained
from fitting the observed spectra of diffuse interstellar EUV and the soft X-ray background.

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