W43A Jet: strongly related to the magnetic field testified in laboratory

被引：7

作者：

Pei Xiao-Xing ^{[1
,2
]}

Zhong Jia-Yong ^{[1
,3
]}

Zhang Kai ^{[1
,2
]}

Zheng Wu-Di ^{[4
]}

Liang Gui-Yun ^{[1
]}

Wang Fei-Lu ^{[1
]}

Li Yu-Tong ^{[5
]}

Zhao Gang ^{[1
]}

机构：

[1] Chinese Acad Sci, Natl Astron Observ, Key Lab Opt Astron, Beijing 100012, Peoples R China

[2] Univ Chinese Acad Sci, Beijing 100049, Peoples R China

[3] Beijing Normal Univ, Dept Astron, Beijing 100875, Peoples R China

[4] Inst Appl Phys & Computat Math, Beijing 100094, Peoples R China

[5] Chinese Acad Sci, Inst Phys, Beijing 100190, Peoples R China

来源：

ACTA PHYSICA SINICA | 2014年 / 63卷 / 14期

基金：

中国国家自然科学基金;

关键词：

high energy density physics; high power laser; jets; GIANT-BRANCH STARS; LASER-PRODUCED PLASMAS; INTENSE LASERS; EXPERIMENTAL ASTROPHYSICS; OUTFLOWS;

D O I：

10.7498/aps.63.145201

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

Dual Al plasma jets are generated with eight Shenguang II lasers. With Euler MHD scale law we find that the jet produced in the laboratory is highly similar to astronomical observations after transformation. We propose that the reconnection electric filed should have a possible direct influence on the formation and collimation of the plasma jet.

引用

页数：5

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