Abstract
The concentrator on Genesis provided samples of increased fluences of solar wind ions for precise determination of the oxygen isotopic composition. The concentration process caused mass fractionation as a function of the radial target position. This fractionation was measured using Ne released by UV laser ablation and compared with modelled Ne data, obtained from ion-trajectory simulations. Measured data show that the concentrator performed as expected and indicate a radially symmetric concentration process. Measured concentration factors are up to ∼30 at the target centre. The total range of isotopic fractionation along the target radius is 3.8%/amu, with monotonically decreasing 20Ne/22Ne towards the centre, which differs from model predictions. We discuss potential reasons and propose future attempts to overcome these disagreements.
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Heber, V.S., Wiens, R.C., Reisenfeld, D.B. et al. The Genesis Solar Wind Concentrator Target: Mass Fractionation Characterised by Neon Isotopes. Space Sci Rev 130, 309–316 (2007). https://doi.org/10.1007/s11214-007-9179-1
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DOI: https://doi.org/10.1007/s11214-007-9179-1