Comment on "Identification of widespread turbulence of dispersive Alfven waves" by K. Stasiewicz et al.

被引:3
|
作者
Lund, EJ [1 ]
机构
[1] Univ New Hampshire, Ctr Space Sci, Durham, NH 03824 USA
基金
美国国家航空航天局;
关键词
D O I
10.1029/2000GL012216
中图分类号
P [天文学、地球科学];
学科分类号
07 ;
摘要
As shown above, the identification of broad-band ELF emissions as zero frequency Alfvénic structures on the basis of the observed δE/δB [S2000] is not justified, first because they assume, contrary to both their data and previous observations, that the turbulence is one-dimensional, and second because the proposed solution is not unique. The observed ULF/ELF turbulence may be Alfvénic, and Doppler-shifted ULF turbulence may contribute significantly to the measured ELF wave power. Indeed, even a dominant contribution from Doppler-shifted ULF turbulence would still leave enough wave power at fcO+ to account for ion conic formation by cyclotron resonant heating. © Copyright 2001 by the American Geophysical Union.
引用
收藏
页码:1403 / 1404
页数:2
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