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- W199705295 abstract "A strong interplanetary shock accompanied by low‐energy (<300 keV) ion intensity enhancements was observed by the ACE spacecraft at 14:48 UT on 2003 October 24. Energetic particle data collected by the EPAM instrument onboard ACE show that the time profiles of the 47–321 keV ion intensities, the ion anisotropies observed upstream and downstream of the shock, and the downstream energy spectra of the 47–321 keV ions agree with the predictions of the quasi‐linear theory of diffusive shock‐acceleration. This shock was also accompanied by an intense level of magnetic field fluctuations as observed during an extended (6 hours) fore‐shock region by ACE/MAG. Although many of the signatures of this event are consistent with the predictions of the diffusive shock‐acceleration theory acting on a low‐energy particle population, analyses of the elemental abundances of heavy ions from 4He to Fe measured by ACE/ULEIS indicate that the abundances of the accelerated ions are poorly correlated with those measured in the so..." @default.
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- W199705295 date "2005-01-01" @default.
- W199705295 modified "2023-09-23" @default.
- W199705295 title "The Energetic Storm Particle Event on 2003 October 24: A Test of Diffusive Shock Acceleration Theory" @default.
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- W199705295 doi "https://doi.org/10.1063/1.2032693" @default.
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