DETERMINATION OF DISPERSION-RELATIONS IN QUASI-STATIONARY PLASMA TURBULENCE USING DUAL SATELLITE DATA

被引:60
作者
DEWIT, TD
KRASNOSELSKIKH, VV
BALE, SD
DUNLOP, MW
LUHR, H
SCHWARTZ, SJ
WOOLLISCROFT, LJC
机构
[1] CNRS,LPCE,F-45071 ORLEANS,FRANCE
[2] UNIV LONDON QUEEN MARY & WESTFIELD COLL,ASTRON UNIT,LONDON E1 4NS,ENGLAND
[3] UNIV LONDON IMPERIAL COLL SCI & TECHNOL,LONDON SW7 2BZ,ENGLAND
[4] TECH UNIV CAROLO WILHELMINA BRAUNSCHWEIG,INST GEOPHYS & METEOROL,D-38106 BRAUNSCHWEIG,GERMANY
[5] UNIV SHEFFIELD,DEPT AUTOMAT CONTROL & SYST ENGN,SHEFFIELD S1 3JD,S YORKSHIRE,ENGLAND
关键词
D O I
10.1029/95GL02543
中图分类号
P [天文学、地球科学];
学科分类号
07 ;
摘要
The joint frequency-wavenumber spectrum is one of the basic quantities for analyzing plasma turbulence. It is shown how the full spectrum can be recovered from wavefields measured by two or more satellites via spectral methods based on wavelet transforms. Compared to standard cross-correlation techniques, different branches in the dispersion relation can be resolved and quasi-stationary wavefields can be accessed. Using this new approach, low frequency magnetic field data from the AMPTE-UKS and AMPTE-IRM spacecraft are investigated and the impact of nonlinear processes on wave propagation at the Earth's foreshock is revealed.
引用
收藏
页码:2653 / 2656
页数:4
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