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中文题名:

 太阳风与地球磁层相互作用的实验室模拟    

姓名:

 仝博伟    

保密级别:

 公开    

论文语种:

 中文    

学科代码:

 070401    

学科专业:

 天体物理    

学生类型:

 硕士    

学位:

 理学硕士    

学位类型:

 学术学位    

学位年度:

 2019    

校区:

 北京校区培养    

学院:

 天文系    

研究方向:

 实验室天体物理    

第一导师姓名:

 仲佳勇    

第一导师单位:

 北京师范大学天文系    

提交日期:

 2019-06-21    

答辩日期:

 2019-06-02    

外文题名:

 Laboratory simulation of the interaction between solar wind and theEarths magnetosphere    

中文关键词:

 实验室天体物理 ; 激光 ; 等离 体 ; 磁层顶 ; 太阳风    

中文摘要:
实验室天体物理是?门利?实验室装置研究天体物理现象的新兴学科。通过实验室可 控的?段理解强磁环境下的等离?体物理现象,对我们认识天体等离?体演化具有重要的 意义。太阳风与地球磁层的相互作??直是天体物理的研究热点。本论?主要利?神光 II 激光装置在实验室产?等离?体和磁场环境,?各四束激光束分别作?于靶的两侧。太阳 风由激光和 CH 靶相互作?产?,偶极磁场由激光与螺线圈相互作?产?。实验观察到在 偶极磁场的前端有明显的密度累积,这和天体物理环境中磁层顶端的密度累积很相似。另 外,实验中提出?种利?强激光辐照开螺线圈靶,由热电?回流产?脉冲强磁场的?法, 并在线圈中?获得了?达 70T 的强磁场。这种?法原理清晰,简单易?,我们将激光驱动 的脉冲磁场?于实验室天体物理的研究中。随着激光驱动的脉冲磁场的不断发展,其有望 在激光等离?体领域取得更加?泛的应?。
外文摘要:
Laboratory astrophysics is one new subject that research astrophysical phenomenon by ex- periments facilities. It is significant to know the evolution of astrophysical plasma by studying the plasma dynamics in a controlled experimental environment. Then, the interaction between the so- lar wind and the Earth's magnetosphere has always interested in astrophysics. This thesis presents thegenerationofsteady-stateplasmaandmagneticfieldinthelaboratorywithShenguangIIlasers, four laser beams are applied to the two sides of the target respectively. And the solar wind is gen- erated by the interaction of the laser and the CH target, and the dipole magnetic field is generated by the interaction of the laser and the solenoid. It is observed that there is a significant density ac- cumulation at the front end of the dipole magnetic field,which is similar to the top of the Earth's magnetosphere in the astrophysics environment.we proposed a simple scheme to produce strong magnetic fields due to hot electron flow in an solenoid coil heated by high power laser pulses,The magnetic field strength at the coil center is measured to be 70 T. The generation mechanism of the magnetic field is straightforward and the coil is easy to be fabricated,we utilized such a strong magnetic field in laboratory astrophysics experiments. With the development of the laser-driven magnetic fields, they are expected to be used in more laser-plasma researches.
参考文献总数:

 76    

作者简介:

 1. 仝博伟,仲佳勇. 基于 Z 箍缩装置的实验室天体物理研究 [J]. 物理, 2018, 47(10): 642-647.(中?核?)2. Sun W, Zhong J.Y, Zhang S, Tong B.W, Wang L.F, Zhao K.G, Liu J.Y, Han B, Zhu B.J, YuanD.W, Yuan X.X, Zhang Z, Li Y.T, Zhang Q, Peng J.M, Wang J.Z, Ping Y.L, Xing C.Q, WeiH.G, Liang G.Y, Xie Z.Y, Wang C, Zhao G, Zhang J.The effect of external magnetic field onthe linear stage evolution of Kelvin–Helmholtz instability in laser driven plasma.2019;31:47-51.doi:10.1016/j.hedp.2019.02.003.(SCI 收录, 检索号:000465111800008)3. Yihang Zhang, Zhe Zhang, Baojun Zhu, Weiman Jiang, Lei Cheng, Lei Zhao, Xiaopeng Zhang,Xu Zhao, Xiaohui Yuan, Bowei Tong, Jiayong Zhong, Shukai He, Feng Lu, Yuchi Wu, WeiminZhou,FaqiangZhang,KainanZhou,NaXie,ZhengHuang,YuqiuGu,SumingWeng,MiaohuaXu,Yingjun Li, and Yutong Li. An angular-resolved multi-channel Thomson parabola spectrometerfor laser-driven ion measurement. Review of Scientific Instruments. 2018;89(9):093302-093307.doi:10.1063/1.5042424. (SCI 收录, 检索号:000446159100030)4. Zhao Lei, Xu Miao-Hua, Zhang Yi-Hang, Zhang Zhe, Zhu Bao-Jun, Jiang Wei-Man, ZhangXiao-Peng, Zhao Xu, Tong Bo-Wei, He Shu-Kai, Lu Feng, Wu Yu-Chi, Zhou Wei-Min, Zhang Fa-Qiang, Zhou Kai-Nan, Xie Na, Huang Zheng, Zhong Jia-Yong, Gu Yu-Qiu, Li Yu-Tong, Li Ying-Jun. Laser fast neutron measured by bubble detector. 1–8 (2018). doi:10.7498/aps.67.20181035(SCI 收录, 检索号:000455402400004)    

馆藏号:

 硕070401/19006    

开放日期:

 2020-07-09    

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