Energetic particles in plasma astrophysics

被引:4
作者
Dendy, RO [1 ]
Kirk, JG
机构
[1] UKAEA Euratom Fus Assoc, UKAEA Fus, Culham Sci Ctr, Abingdon OX14 3DB, Oxon, England
[2] Max Planck Inst Kernphys, D-69029 Heidelberg, Germany
关键词
D O I
10.1088/0741-3335/41/3A/035
中图分类号
O35 [流体力学]; O53 [等离子体物理学];
学科分类号
070204 ; 080103 ; 080704 ;
摘要
Cosmic ray and gamma-ray astrophysics provides an arena where concepts drawn from many branches of plasma physics can assist in answering questions of fundamental-indeed cosmological-significance. In recent years, striking advances have been made in the quality and resolution of the data available in this field. The present generation of cosmic ray detection arrays and space-based x-ray and gamma-ray observatories, coupled to measurements in other wavebands, are yielding information which invites detailed quantitative interpretation in terms of plasma processes. In parallel with these developments, a systematic picture of the behaviour of energetic particle populations in magnetically confined plasmas has emerged from the deuterium-tritium experimental campaigns on JET and TFTR, and the acceleration of electrons to highly relativistic energies has been demonstrated in laser-plasma interaction experiments. This review is written primarily to assist the deployment in energetic particle astrophysics of methodologies used for studying high-temperature fusion plasmas: three topics are examined. What are the major plasma-oriented questions in energetic particle astrophysics? What solutions have been proposed? How can plasma physics assist in deepening, strengthening and extending current understanding?
引用
收藏
页码:A427 / A435
页数:9
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