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• W1977029951 abstract "The study carried out in order to demonstrate that high minor ion outflow speeds of the order of O(5+) outflow speed are consistent with charge state observations is presented. The calculations were based on atomic data, observational constraints concerning electron temperatures, electron densities and flow speeds. Minor ion charge state observations were used in order to place limits on solar wind acceleration and heating mechanisms. The charge states of C, O, Fe and Si ions measured in situ were compared to those calculated from two solar wind models. The use of the planned ultraviolet and charge state observations in order to constrain both the ion outflow speeds and electron temperature is discussed." @default.
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• W1977029951 date "1998-05-01" @default.
• W1977029951 modified "2023-10-17" @default.
• W1977029951 title "High Minor Ion Outflow Speeds in the Inner Corona and Observed Ion Charge States in Interplanetary Space" @default.
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• W1977029951 doi "https://doi.org/10.1086/305516" @default.
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