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Anisotropy of inertial range turbulence in the polar heliosphere
Author(s) -
Horbury T. S.,
Balogh A.,
Forsyth R. J.,
Smith E. J.
Publication year - 1995
Publication title -
geophysical research letters
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.007
H-Index - 273
eISSN - 1944-8007
pISSN - 0094-8276
DOI - 10.1029/95gl03012
Subject(s) - physics , anisotropy , amplitude , isotropy , polar , transverse plane , field (mathematics) , computational physics , turbulence , heliosphere , range (aeronautics) , magnetic field , solar wind , optics , mechanics , mathematics , quantum mechanics , materials science , engineering , structural engineering , pure mathematics , composite material
A variance analysis of high frequency, inertial range fluctuations in the polar magnetic field as recorded by the Ulysses spacecraft indicates that they are largely transverse to the ambient magnetic field direction and highly anisotropic. Despite large changes in the mean field direction caused by the presence of large amplitude Alfvén waves, alignment of minimum variance vectors of 5 minute intervals of linearly detrended data with the mean field direction was good, with around 75% of minimum variance vectors lying within 26° of the mean field direction during a typical 5 day interval. Such fluctuations transverse to the mean field have anisotropies—the ratio of power transverse to the field to that parallel—of around 30. We find a small tendency for the field‐transverse fluctuations to become more isotropic with distance. Intervals whose minimum variance directions are not field‐aligned appear to be indicative of a significantly different type of fluctuations, with higher total variances and lower anisotropy.