The Interstellar Boundary Explorer High Energy (IBEX-Hi) Neutral Atom Imager

By H. Funsten, F. Allegrini, P. Bochsler, G. Dunn, S. Ellis, D. Everett, M. Fagan, S. Fuselier, M. Granoff, M. Gruntman and 25 more. 2009

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Interstellar Mapping and Acceleration Probe (IMAP): A New NASA Mission (2018, methodology): “ENAs strike a 15° inclined diamond-like carbon CS on a Si wafer converting ENAs into negative ions (Wurz et al. 1997, 2006; Scheer et al. 2005, 2006; Wieser et al. 2007; Fuselier et al. 2009b; Bzowski et al. 2012; Möbius et al. 2009; Bochsler et al. 2012; Park et al. 2014; Funsten et al. 2009a).”
INTERSTELLAR GAS FLOW PARAMETERS DERIVED FROM INTERSTELLAR BOUNDARY EXPLORER-Lo OBSERVATIONS IN 2009 AND 2010: ANALYTICAL ANALYSIS (2012, background): “These time periods can easily be identified in the IBEX-Lo TOF rates and in the IBEX-Hi background signals and are also removed from analysis.”
SEPARATION OF THE INTERSTELLAR BOUNDARY EXPLORER RIBBON FROM GLOBALLY DISTRIBUTED ENERGETIC NEUTRAL ATOM FLUX (2011, methodology): “After correcting for the survival probability over 100 AU, we use the approach of Funsten et al. (2009a) to calculate the pressure integrated along the LOS for the ribbon and the distributed flux, as shown in Figure 18.”
Helium, Oxygen, Proton, and Electron (HOPE) Mass Spectrometer for the Radiation Belt Storm Probes Mission (2013, methodology): “This technique was first incorporated on the IBEX-Hi energetic neutral atom imager (Funsten et al. 2009) and has been an important tool for quantifying, identifying, and monitoring different types of background in IBEX-Hi.”