日本地球惑星科学連合2016年大会

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セッション記号 P (宇宙惑星科学) » P-EM 太陽地球系科学・宇宙電磁気学・宇宙環境

[P-EM19] 太陽圏・惑星間空間

2016年5月25日(水) 13:45 〜 15:15 302 (3F)

コンビーナ:*坪内 健(東京工業大学大学院理工学研究科)、西野 真木(名古屋大学宇宙地球環境研究所)、成行 泰裕(富山大学人間発達科学部)、座長:大塚 史子(九州大学大学院総合理工学研究院)

14:00 〜 14:15

[PEM19-08] 磁気雲通過開始時刻付近における惑星間空間磁場の計算と観測との比較

*西村 信彦1野崎 錦1ジャクソン バーナード2ユー シューサン2徳丸 宗利1藤木 謙一1林 啓志1袴田 和幸3 (1.名古屋大学宇宙地球環境研究所、2.カリフォルニア大学サンディエゴ校、3.中部大学)

キーワード:コロナ磁場、磁気雲、宇宙天気、太陽風

The solar source of magnetic clouds (MCs) is considered to be either coronal mass ejections (CMEs) or prominence eruptions [Bothmer et al., 1994, 1998]. We suppose that the coronal magnetic fields above CME or prominence eruption sites move outward and are then convected into interplanetary space to arrive at the Earth a short time before the MC start time. We extract the magnetic field close to the solar surface at different heights using the PFSS model [Hakamada, 1998] and propagate this field outward to 1 AU using 3D-reconstructed solar wind velocity [Jackson et al., 2010]. The purpose of our work is to examine whether the direction of interplanetary magnetic field (IMF) agrees with the observed vector field prior to a MC arrival at the Earth. We compare the sign of each component of modeled IMF (in RTN coordinates) with that of IMF observed by ACE three hours before the MC start time (pre MC time) and at the MC start time (MC time). These comparisons are made for six MC events during 2006 - 2007. We find that the sign of Bn, the normal component of IMF in RTN coordinates, extracted from 1.4 Rs (1.2 Rs) agrees best with ACE observations at the pre MC time (at the MC time) for all MC events analyzed here. However, the other two components Br and Bt, the radial and tangential components of IMF in RTN coordinates, extracted from 1.4 Rs (1.2 Rs) do not agree as well with ACE observations at the pre MC time (at the MC time). We conclude that Bn observed by ACE at the pre MC time (at the MC time) is related to that at 1.4 Rs (1.2 Rs) at the location of the sub-Earth point on the Sun. This result shows that we can infer the sign of Bn at the MC time (pre MC time) from the value present at 1.2 Rs (1.4 Rs) at the location of the sub-Earth point, and thus this is an important finding for space weather forecasts. Future work will extend this result to additional MC events.