Spatial and temporal structure of edge-localized modes

被引：145

作者：

Kirk, A ^{[1
]}

Wilson, HR

Counsell, GF

Akers, R

Arends, E

Cowley, SC

Dowling, J

Lloyd, B

Price, M

Walsh, M

机构：

[1] EURATOM, Culham Sci Ctr, Abingdon OX14 3DB, Oxon, England

[2] EURATOM, FOM, Inst Plasma Phys Rijnhuizen, NL-3439 MN Nieuwegein, Netherlands

[3] Univ London Imperial Coll Sci Technol & Med, London SW7 2BZ, England

[4] Univ Calif Los Angeles, Dept Phys & Astron, Los Angeles, CA 90095 USA

[5] Walsh Sci Ltd, Culham Sci Ctr, Abingdon OX14 3EB, Oxon, England

来源：

PHYSICAL REVIEW LETTERS | 2004年 / 92卷 / 24期

基金：

英国工程与自然科学研究理事会; 欧盟地平线“2020”;

关键词：

D O I：

10.1103/PhysRevLett.92.245002

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

This Letter provides information on the spatial and temporal structure of periodic eruptions observed in magnetically confined laboratory fusion plasmas, called edge-localized modes (ELMs), and highlights similarities with solar eruptions. Taken together, the observations presented in this Letter provide strong evidence for ELMs being associated with a filamentlike structure. These filaments are extended along a field line, are generated on a 100 mus time scale, erupt from the outboard side, and connect back into the plasma. Such structures are predicted by a theoretical model based on the "ballooning" instability, developed for both solar and tokamak applications.

引用

页码：245002 / 1

页数：4

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