Detection of Energetic Helium Atoms of Heliospheric Origin at 1 AU

Details Detection of Energetic Helium Atoms of Heliospheric Origin at 1 AU Detection of Energetic Helium Atoms of Heliospheric Origin at 1 AU

May 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001agusm..sh22f04s&link_type=abstract

American Geophysical Union, Spring Meeting 2001, abstract #SH22F-04

Physics

2104 Cosmic Rays, 2114 Energetic Particles, Heliospheric (7514), 2124 Heliopause And Solar Wind Termination, 2144 Interstellar Gas, 2151 Neutral Particles

Scientific paper

The time-of-flight mass spectrometer CELIAS/HSTOF on the Solar and Heliospheric Observatory (SOHO), which detected the energetic hydrogen atoms of heliospheric origin in the energy range of 58-88 keV, has also detected and measured the flux of energetic helium atoms of heliospheric origin in the energy range of 90-150 keV. We report on the time variations in the flux of these energetic He atoms in the ecliptic. Plausible interpretation and implications of the observed flux variations will be presented.

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