JpGU-AGU Joint Meeting 2020

Presentation information

[E] Oral

P (Space and Planetary Sciences ) » P-EM Solar-Terrestrial Sciences, Space Electromagnetism & Space Environment

[P-EM17] Space Weather and Space Climate

convener:Ryuho Kataoka(National Institute of Polar Research), Antti A Pulkkinen(NASA Goddard Space Flight Center), Kanya Kusano(Institute for Space-Earth Environmental Research, Nagoya University), Kaori Sakaguchi(National Institute of Information and Communications Technology)

[PEM17-18] Statistical Analysis of the Relation between Coronal Mass Ejections and Solar Energetic Particles

*Kosuke Kihara1, Yuwei Huang2, Nobuhiko Nishimura3, Nariaki Nitta4, Seiji Yashiro5, Kiyoshi Ichimoto2, Ayumi Asai2 (1.Department of Astronomy, Kyoto University, 2.Astronomical Observatory, Kyoto University, 3.Institute for Space Earth Environmental Research, 4.Lockheed Martin Advanced Technology Center, 5.The Catholic University of America)

Keywords:Solar Energetic Particles, Coronal Mass Ejections, Space Weather

Solar energetic particles (SEPs), which originate in powerful eruptions in the solar corona, give rise to critical radiation hazards for astronauts and airline passengers, causing damages to satellites, which result in serious societal impacts. Although past studies show some relations between coronal mass ejections (CMEs) and SEP events, they have considerable scatters and it suggests that there are some unknown factors between them. In order to advance our understandings of how the properties of CMEs affect that of SEPs, we have conducted a statistical study of the relation between CMEs and SEP events. Instead of correlating SEP properties with CMEs as conduced in a majority of past studies, we started from all the 257 fast (v > 900 km/s) and wide (Angular width > 60°) CMEs that occurred between December 2006 and October 2017. We detected their associated SEP events in >10 MeV protons from the three directions, GOES, STEREO-A, and STEREO-B. For the detected CME-SEP pairs, we computed three timescales of SEP events, onset time (TO), rise time (TR), and duration (TD), and correlated them with the CME speed and the longitude of the CME source location relative to the Parker spiral footpoint (ΔΦ). It is found that near the Parker spiral footpoint (|ΔΦ| < 60°), TO tends to be short and negatively correlates with CME speed. The correlation between TO, TR and ΔΦ is weaker than TO, but TD and CME speeds have a positive correlation.