Reply to comment by H. Hasegawa on "Evolution of Kelvin-Helmholtz activity on the dusk flank magnetopause"

被引：4

作者：

Foullon, C. ^{[1
]}

Farrugia, C. J. ^{[2
,3
]}

Fazakerley, A. N. ^{[4
]}

Owen, C. J. ^{[4
]}

Gratton, F. T. ^{[5
]}

Torbert, R. B. ^{[2
,3
]}

机构：

[1] Univ Warwick, Dept Phys, Ctr Fus Space & Astrophys, Coventry CV4 7AL, W Midlands, England

[2] Univ New Hampshire, Ctr Space Sci, Durham, NH 03824 USA

[3] Univ New Hampshire, Dept Phys, Durham, NH 03824 USA

[4] Univ Coll London, Mullard Space Sci Lab, Dorking RH5 6NT, Surrey, England

[5] Univ Buenos Aires, Inst Fis Plasma, CONICET, RA-1428 Buenos Aires, DF, Argentina

来源：

JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS | 2009年 / 114卷

基金：

英国工程与自然科学研究理事会;

关键词：

INTERPLANETARY MAGNETIC-FIELD; CLUSTER OBSERVATIONS; BOUNDARY-LAYER; INSTABILITY; WAVES;

D O I：

10.1029/2009JA014444

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页数：3

共 14 条

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[10]

Hasegawa H, 2009, J GEOPHYS RES-SPACE, V114, DOI [10.1029/2008JA013887, 10.1029/2005JA011538]

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