On the Origin of Energetic Neutral Atoms Detected by the SOHO/CELIAS/HSTOF Sensor

Details On the Origin of Energetic Neutral Atoms Detected by the SOHO/CELIAS/HSTOF Sensor On the Origin of Energetic Neutral Atoms Detected by the SOHO/CELIAS/HSTOF Sensor

Sep 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004aipc..719..229k&link_type=abstract

PHYSICS OF THE OUTER HELIOSPHERE. AIP Conference Proceedings, Volume 719, pp. 229-236 (2004).

Physics

2

Particle Emission, Solar Wind, Solar Wind Plasma, Sources Of Solar Wind, Planetary Bow Shocks, Interplanetary Shocks

Scientific paper

We summarize observational data and present theoretical considerations
in order to estimate the relative contributions of suprathermal pick-up
ions neutralized inside and outside the termination shock to the
energetic neutral atom (ENA) flux in the energy range 55 - 80 keV/amu
detected by the SOHO/CELIAS/HSTOF sensor near Earth's orbit.

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