The Physics of Multiply and Highly Charged Ions 2003
DOI: 10.1007/978-94-017-0542-4_4
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Highly Charged Ion Collision Processes in High Temperature Fusion Plasmas

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Cited by 3 publications
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“…Subsequent to the interaction the excited HCI stabilizes via a combination of radiative decay and autoionization. Studies of charge exchange are important for a fundamental understanding of atomic processes and for applications such as spectral diagnostics of fusion plasmas heated by neutral beam injection [2] and the determination of ion storage times in ion traps and storage rings [3]. Further impetus to this area of research stems from the discovery of x-ray emission from comets by Lisse et al in 1996 [4], for which charge exchange between HCIs in the solar wind and neutrals in the coma of the comet has been established as the main emission mechanism [5].…”
Section: Introductionmentioning
confidence: 99%
“…Subsequent to the interaction the excited HCI stabilizes via a combination of radiative decay and autoionization. Studies of charge exchange are important for a fundamental understanding of atomic processes and for applications such as spectral diagnostics of fusion plasmas heated by neutral beam injection [2] and the determination of ion storage times in ion traps and storage rings [3]. Further impetus to this area of research stems from the discovery of x-ray emission from comets by Lisse et al in 1996 [4], for which charge exchange between HCIs in the solar wind and neutrals in the coma of the comet has been established as the main emission mechanism [5].…”
Section: Introductionmentioning
confidence: 99%
“…Charge exchange as a result of low energy collisions between highly charged ions and gases has become an area of increased interest due to applications in high temperature fusion plasma diagnostics [1] and the observation of x-ray emission from comets [2]. In the first case, heavy ions present as impurities in the plasma capture electrons from inherent or injected neutrals and in the second, heavy ions in the solar wind capture electrons from neutrals in the comet's bow shock region.…”
Section: Introductionmentioning
confidence: 99%