{"paper":{"title":"Scaling Relations in Coronal Mass Ejections and Energetic Proton Events associated with Solar Superflares","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.EP"],"primary_cat":"astro-ph.SR","authors_text":"Kazunari Shibata, Takuya Takahashi, Yoshiyuki Mizuno","submitted_at":"2016-11-18T09:23:09Z","abstract_excerpt":"In order to discuss the potential impact of solar 'superflares' on space weather, we investigated statistical relations among energetic proton peak flux with energy higher than $ 10 \\rm MeV$ ($F_p$), CME speed near the Sun ($V_{CME}$) obtained by {\\it SOHO}/LASCO coronagraph and flare soft X-ray peak flux in 1-8\\AA band ($F_{SXR}$) during 110 major solar proton events (SPEs) recorded from 1996 to 2014. The linear regression fit results in the scaling relations $V_{CME} \\propto F_{SXR}^\\alpha$, $F_p\\propto F_{SXR}^\\beta$ and $F_p\\propto V_{CME}^\\gamma$ with $\\alpha = 0.30\\pm 0.04$, $\\beta = 1.1"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1611.06015","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"}