R. Kallenbach et al., Fractionation of Si, Ne, and Mg isotopes in the solar wind as measured by SOHO/CELIAS/MTOF, SPACE SCI R, 85(1-2), 1998, pp. 357-370
Using the high-resolution mass spectrometer CELIAS/MTOF on board SOHO we ha
ve measured the solar wind isotope abundance ratios of Si, Ne, and Mg and t
heir variations in different solar wind regimes with bulk velocities rangin
g from 330 km/s to 650 km/s. Data indicate a small systematic depletion of
the heavier isotopes in the slow solar wind on the order of (1.4+/-1.3)% pe
r amu (2 sigma-error) compared to their abundances in the fast solar wind f
rom coronal holes. These variations in the solar wind isotopic composition
represent a pure mass-dependent effect because the different isotopes of an
element pass the inner corona with the same charge state distribution. The
influence of particle mass on the acceleration of minor solar wind ions is
discussed in the context of theoretical models and recent optical observat
ions with other SOHO instruments.