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- W2044142708 abstract "Observations of a phase lag between the intensity variations of high-energy galactic cosmic rays and the quiet-time oxygen flux in the energy region 7.6-24 MeV/nucleon during the time period 1974-1975 are reported. Phase lag or hysteresis effects have been observed during the 11-year solar cycle for low-energy galactic cosmic rays and several authors have shown that this hysteresis effect is a function of the velocity and rigidity (and therefore of the ionic charge) of the particles. Assuming a similar rigidity dependence of the phase lag during the transient intensity decrease of both galactic cosmic rays and the anomalous oxygen component in the time period 1974-1975, and comparing the phase lag as observed for protons and helium during the same period with the oxygen measurements, an upper limit of approximately 4 is derived for the ionic charge of the anomalous oxygen component." @default.
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- W2044142708 date "1980-12-01" @default.
- W2044142708 modified "2023-09-24" @default.
- W2044142708 title "On the charge state of the anomalous oxygen component" @default.
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- W2044142708 doi "https://doi.org/10.1029/gl007i012p01033" @default.
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