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The full He signal observed during the 2010 observation season can be explained as a superposition of pristine neutral interstellar He gas and an additional population of neutral He that we call the Warm Breeze. The Warm Breeze is approximately two-fold slower and 2.5 times warmer than the primary interstellar He population, and its density in front of the heliosphere is ~7% that of the neutral interstellar helium. 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Alexashov, D.J. McComas, E.Moebius, J.M. Sok\\'o{\\l}, M.A. Kubiak, M. Bzowski, P. Swaczyna, P. Wurz, S.A. Fuselier, S. Grzedzielski, T. Leonard, V.V. Izmodenov","submitted_at":"2014-05-29T22:40:10Z","abstract_excerpt":"We investigate the signals from neutral He atoms observed from Earth orbit in 2010 by IBEX. The full He signal observed during the 2010 observation season can be explained as a superposition of pristine neutral interstellar He gas and an additional population of neutral He that we call the Warm Breeze. The Warm Breeze is approximately two-fold slower and 2.5 times warmer than the primary interstellar He population, and its density in front of the heliosphere is ~7% that of the neutral interstellar helium. 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