{ "id": "1611.06015", "version": "v1", "published": "2016-11-18T09:23:09.000Z", "updated": "2016-11-18T09:23:09.000Z", "title": "Scaling Relations in Coronal Mass Ejections and Energetic Proton Events associated with Solar Superflares", "authors": [ "Takuya Takahashi", "Yoshiyuki Mizuno", "Kazunari Shibata" ], "comment": "17 pages, 5 figures, accepted for publication in Astrophysical Journal Letters", "categories": [ "astro-ph.SR", "astro-ph.EP" ], "abstract": "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 $\\alpha = 0.30\\pm 0.04$, $\\beta = 1.19 \\pm 0.08$ and $\\gamma = 4.35 \\pm 0.50$, respectively. On the basis of simple physical assumptions, on the other hand, we derive scaling relations expressing CME mass ($M_{CME}$), CME speed and energetic proton flux in terms of total flare energy ($E_{flare}$) as, $M_{CME}\\propto E_{flare}^{2/3}$, $V_{CME}\\propto E_{flare}^{1/6}$ and $F_{p}\\propto E_{flare}^{5/6}\\propto V_{CME}^5$, respectively. We then combine the derived scaling relations with observation, and estimated the upper limit of $V_{CME}$ and $F_p$ to be associated with possible solar superflares.", "revisions": [ { "version": "v1", "updated": "2016-11-18T09:23:09.000Z" } ], "analyses": { "keywords": [ "coronal mass ejections", "energetic proton events", "solar superflares", "relations expressing cme mass", "scaling relations expressing cme" ], "note": { "typesetting": "TeX", "pages": 17, "language": "en", "license": "arXiv", "status": "editable" } } }