日本地球惑星科学連合2014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-EM33_1AM1] プラズマ宇宙:観測・実験の計画・手法,装置開発,プラズマ計測

2014年5月1日(木) 09:00 〜 10:45 503 (5F)

コンビーナ:*松清 修一(九州大学大学院総合理工学研究院流体環境理工学部門)、杉山 徹(独立行政法人海洋研究開発機構 地球シミュレータセンター)、座長:杉山 徹(独立行政法人海洋研究開発機構 地球シミュレータセンター)

10:30 〜 10:45

[PEM33-06] レーザー実験を用いた無衝突衝撃波研究の現状と課題

*松清 修一1坂和 洋一2蔵満 康浩3富田 健太郎1森田 太智2山崎 了4高部 英明2 (1.九州大学、2.大阪大学、3.国立中央大学、4.青山学院大学)

キーワード:無衝突衝撃波, レーザー実験, 数値実験

Collisionless shocks are ubiquitous in various space and astrophysical environments like a termination shock of a stellar wind, planetary bow shocks, supernova remnant shocks, etc. Recently, collisionless shocks have been able to be experimentally generated by using high power laser facilities. One of the advantages in an experimental study is that both the global and the local structures of the phenomenon are simultaneously accessible in principle, which is inherently difficult in-situ or remote sensing observations in space. However, the shocks produced in the laser experiments and the method for measuring them are quite different from those in space. A majority of the shocks produced in laser experiments are unmagnetized shocks. The methodology for measuring their local quantities in the transition region has not been established. On the other hand, basic structures and dissipation mechanisms in an unmagnetized shock have not been well understood theoretically. So far high Mach number electrostatic shocks are thought to be generated by the counter streams of two non-identical plasmas. In this study microstructures of such electrostatic shocks are studied by using a full particle-in-cell simulation. In addition, characteristics and issues of currently adopted method of measuring local quantities in shock transition region, known as Thomson scattering measurement, are also discussed.