A Re-interpretation of the STEREO/STE Observations and it's Consequences
K. C. Hsieh, P. C. Frisch, J. Giacalone, J. R. Jokipii, J. Kota, D. E., Larson, R. P Lin, J. G. Luhmann, L. Wang

TL;DR
This paper reinterprets STEREO/STE observations, suggesting they are due to X-ray emissions from Sco X-1 rather than energetic neutral atoms, challenging previous assumptions about the heliosheath.
Contribution
It offers a new interpretation of the STEREO/STE data, linking observed signals to X-ray sources instead of ENA, impacting understanding of solar wind interactions.
Findings
Observed peak aligns with Sco X-1's position
Energy spectrum matches X-ray emissions from Sco X-1
Challenges previous ENA-based explanations for the data
Abstract
We present an alternate interpretation of recent STEREO/STE observations that were originally attributed to energetic neutral atoms (ENA) from the heliosheath. The signal attributed to the diffuse ENA source instead shows the characteristics of a point source. We point out that the peak intensity seen by STEREO/STE is centered at the ecliptic longitude of the bright X-ray source Sco X-1. The observed energy spectrum and intensity are also consistent with the X-rays from Sco X-1. The problem of energy dissipation at the solar wind termination shock remains unsolved while current understanding of the interaction between the solar wind and interstellar wind awaits future observations.
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