Coordinated observation of local interstellar helium in the Heliosphere Synopsis of the interstellar He parameters from combined neutral gas, pickup ion and UV scattering observations and related…

By E. Möbius, G. Gloeckler, V. Izmodenov, R. Kallenbach, R. Lallement, D. McMullin, J. C. Raymond, R. Skoug, T. Terasawa, W. Thompson and 2 more. 2004

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NEUTRAL INTERSTELLAR HELIUM PARAMETERS BASED ON IBEX-Lo OBSERVATIONS AND TEST PARTICLE CALCULATIONS (2012, methodology): “We compared collimator-averaged total NISHe fluxes expected assuming the prior consensus NISHe flow parameters (Möbius et al. 2004), which are very close to the parameters obtained by Witte (2004) from Ulysses, with the NISH flux in energy step 2 (center energy 27 eV) of the IBEX-Lo detector…”
INTERSTELLAR GAS FLOW PARAMETERS DERIVED FROM INTERSTELLAR BOUNDARY EXPLORER-Lo OBSERVATIONS IN 2009 AND 2010: ANALYTICAL ANALYSIS (2012, background): “◦4 (in J2000) and VISM∞ = 26.4 km s−1 (Möbius et al. 2004), largely determined by the neutral gas observations (Witte 2004) owing to their small uncertainties.”
The Interstellar Medium Surrounding the Sun (2011, methodology): “The velocity vector of interstellar HeI entering the heliosphere is given by direct measurements of HeI atoms, and the fluorescence of backscattered solar 584-Å emission from the HeI (Möbius et al. 2004).”