A Ulysses Detection of Secondary Helium Neutrals
Brian E. Wood, Hans-Reinhard Mueller, Manfred Witte

TL;DR
This study detects a secondary helium neutral flow in Ulysses data, consistent with IBEX findings, and estimates its properties, highlighting the importance of flow assumptions in interpreting interstellar helium measurements.
Contribution
It provides the first detection of the secondary helium component in Ulysses data and compares its properties with IBEX measurements, emphasizing the impact of flow assumptions on temperature estimates.
Findings
Detected secondary helium flow in Ulysses data.
Measured flow parameters: V=12.8 km/s, lambda=74.4°, beta=-10.5°, T=3000 K.
Secondary component density is about 5% of the primary.
Abstract
The Interstellar Boundary EXplorer (IBEX) mission has recently studied the flow of interstellar neutral He atoms through the solar system, and discovered the existence of a secondary He flow likely originating in the outer heliosheath. We find evidence for this secondary component in Ulysses data. By coadding hundreds of Ulysses He beam maps together to maximize signal-to-noise, we identify a weak signal that is credibly associated with the secondary component. Assuming a laminar flow from infinity, we infer the following He flow parameters: V=12.8+/-1.9 km/s, lambda=74.4+/-1.8 deg, beta=-10.5+/-4.1 deg, and T=3000+/-1100 K; where lambda and beta are the ecliptic longitude and latitude direction in J2000 coordinates. The secondary component has a density that is 4.9+/-0.9% that of the primary component. These measurements are reasonably consistent with measurements from IBEX, with the…
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