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- W2018889146 abstract "Charge transfer emission has been reported to be the dominant source of X-rays in cometary atmospheres. The emission model is based on the estimated charge transfer cross sections of solar wind minor/heavy ions and cometary neutrals. We report the results of our measurements on the absolute total one and multielectron transfer cross sections for Oq+ (q = 5, 4) with CO at ~1.5q keV energies using a technique that combines a laser ablation ion source and a reflection time-of-flight mass spectrometer. The total single electron transfer cross sections for O5+ and O4+ ions with CO are 3.42(±0.50) × 10-15 and 2.91(±0.41) × 10-15 cm2, respectively. The cross sections for multielectron transfer are 1.15(±0.37) × 10-15 and 1.03(±0.28) × 10-15 cm2, respectively." @default.
- W2018889146 created "2016-06-24" @default.
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- W2018889146 date "2002-03-10" @default.
- W2018889146 modified "2023-10-16" @default.
- W2018889146 title "Charge Transfer of O5+and O4+with CO at keV Energies" @default.
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- W2018889146 doi "https://doi.org/10.1086/338589" @default.
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