Three-Dimensional Structure of Solar Wind Turbulence

We present a measurement of the scale-dependent, three-dimensional structure of the magnetic field fluctuations in inertial range solar wind turbulence with respect to a local, physically motivated coordinate system. The Alfvenic fluctuations are three-dimensionally anisotropic, with the sense of th...

Disgrifiad llawn

Manylion Llyfryddiaeth
Prif Awduron: Chen, C, Mallet, A, Schekochihin, A, Horbury, T, Wicks, RT, Bale, S
Fformat: Journal article
Cyhoeddwyd: 2012