{"paper":{"title":"The injection of ten electron/$^{3}$He-rich SEP events","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["physics.space-ph"],"primary_cat":"astro-ph.SR","authors_text":"Gang Li, Glenn M. Mason, Linghua Wang, Robert P. Lin, S\\\"am Krucker","submitted_at":"2016-05-25T13:48:31Z","abstract_excerpt":"We have derived the particle injections at the Sun for ten good electron/$^{3}$He-rich solar energetic particle (SEP) events, using a 1.2 AU particle path length (suggested by analysis of the velocity dispersion). The inferred solar injections of high-energy ($\\sim$10 to 300 keV) electrons and of $\\sim$MeV/nucleon ions (carbon and heavier) start with a delay of 17$\\pm$3 minutes and 75$\\pm$14 minutes, respectively, after the injection of low-energy ($\\sim$0.4 to 9 keV) electrons. The injection duration (averaged over energy) ranges from $\\sim$200 to 550 minutes for ions, from $\\sim$90 to 160 mi"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1605.07882","kind":"arxiv","version":1},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"}