Direct Observations of Interstellar Neutral Atoms from IMAGE

Physics

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2144 Interstellar Gas, 2151 Neutral Particles

Scientific paper

The Imager for Magnetosphere-to-Aurora Global Exploration (IMAGE) spacecraft was launched in early 2000. Its Low-Energy Neutral Atom (LENA) imager, designed primarily for remote sensing of terrestrial neutral atom emissions generated by plasma heating, has an energy range of 10 to 1000 eV. We report direct LENA observations of interstellar neutral atoms detected by the LENA imager during certain times of the year when the IMAGE orbit geometry is favorable. This is when the spacecraft is "downwind" of the Sun, within the Sun's gravitational focusing cone for interstellar neutral atoms, and beginning to turn into the "upwind" direction. Comparison of LENA observations with numerical models indicates that the LENA instrument has detected primarily interstellar neutral helium, which can be observed by sputtering of adsorbed atoms from the LENA instrument's conversion surface. A summary of the LENA observations of interstellar neutral atoms will be presented, along with a description of the numerical models with which they have been compared.

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