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- W1989036701 abstract "This paper describes results obtained from the Prognoz 8 ion composition experiment which indicates that He + ions may be more abundant in the solar wind than previous measurements have indicated. The experiment has a sufficiently high mass resolution to accurately discriminate between H + , He ++ , He + , and O + ions over the energy range 0.35–5.2 keV/el. Furthermore, the fact that the experiment is continuously monitoring in the solar direction means that fairly good statistics can be aquired as well. In a few cases, He + /He ++ ratios up to ≈0.05 have been found, but in most cases when He + was observed it was generally of the order 0.3–3% of the He ++ content. We compare our results with previous measurements of He + ions in the solar wind and discuss also other constituents with M/q = 4 as alternative candidates. Finally, a possible explanation for the high He + abundance in the disturbed solar wind is given." @default.
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- W1989036701 date "1985-05-01" @default.
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- W1989036701 title "Observations of He<sup>+</sup> ions in the solar wind" @default.
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- W1989036701 doi "https://doi.org/10.1029/ja090ia05p04367" @default.
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