A laboratory study of mechanisms for Auroral Kilometric Radiation generation

被引：0
|
作者：
Ronald, K. [1 ,2 ]
Speirs, D. C. [1 ,2 ]
McConville, S. L. [1 ,2 ]
Gillespie, K. M. [1 ,2 ]
Phelps, A. D. R. [1 ,2 ]
Bingham, R. [1 ,2 ,4 ]
Cross, A. W. [1 ,2 ]
Robertson, C. W. [1 ,2 ]
Whyte, C. G. [1 ,2 ]
He, W. [1 ,2 ]
Cairns, R. A. [3 ]
Vorgul, I. [3 ]
Kellett, B. J. [4 ]
机构：
[1] Univ Strathclyde, SUPA, Glasgow G4 0NG, Lanark, Scotland
[2] Univ Strathclyde, Dept Phys, Glasgow G4 0NG, Lanark, Scotland
[3] Univ St Andrews, Sch Math & Stat, St Andrews, Fife, Scotland
[4] Space Sci Dept, Rutherford Apple Lab, Chilton, England
来源：
35TH INTERNATIONAL CONFERENCE ON INFRARED, MILLIMETER, AND TERAHERTZ WAVES (IRMMW-THZ 2010) | 2010年
基金：
英国工程与自然科学研究理事会;
关键词：
CYCLOTRON MASER RADIATION; PLASMAS; DISTRIBUTIONS; INSTABILITY; SPACE;
D O I：
暂无
中图分类号：
TM [电工技术]; TN [电子技术、通信技术];
学科分类号：
0808 ; 0809 ;
摘要：
An experimental simulation of the Earth's Auroral Magnetosphere has been created. Experiments have been undertaken to study the processes by which the auroral cyclotron maser emission occurs.
引用
收藏
页数：2
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