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• W3103652051 startingPage "074" @default.
• W3103652051 abstract "According to the solar protons' data observed by Geostationary Operational Environmental Satellites (GOES) and neutron monitors on the ground of the Earth, and near-relativistic electrons data measured by the ACE spacecraft, the onset times of protons with different energies and near-relativistic electrons have been estimated and compared with the time of solar soft and hard X-ray and radio burst data. The results show that first arriving relativistic and non-relativistic protons and electrons may be accelerated by the concurrent flare. The results also suggest that release times of protons with different energies may be different, and the protons with lower energy may release earlier than those with higher energy. Some protons accelerated by concurrent flares may be further accelerated by CME-driven shock." @default.
• W3103652051 created "2020-11-23" @default.
• W3103652051 creator A5034358836 @default.
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• W3103652051 date "2018-07-01" @default.
• W3103652051 modified "2023-10-03" @default.
• W3103652051 title "Investigation of the possible source for the solar energetic particle event on 2017 September 10" @default.
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• W3103652051 doi "https://doi.org/10.1088/1674-4527/18/7/74" @default.
• W3103652051 hasPublicationYear "2018" @default.
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