Anisotropies of the Magnetic Field Fluctuations at Kinetic Scales in the Solar Wind: Cluster Observations

Journal Article · Tue Oct 10 04:00:00 EDT 2017 · Astrophysical Journal

DOI:https://doi.org/10.3847/1538-4357/AA8C06· OSTI ID:22875702

Lacombe, Catherine; Alexandrova, Olga; Matteini, Lorenzo ^[1]

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1. LESIA-Observatoire de Paris, PSL Research University, CNRS, UPMC Université Paris 06, Université Paris-Diderot, 5 place Jules Janssen, F-92190 Meudon (France)

We present the first statistical study of the anisotropy of the magnetic field turbulence in the solar wind between 1 and 200 Hz, i.e., from proton to sub-electron scales. We consider 93 ten-minute intervals of the Cluster/STAFF measurements. We find that the fluctuations δB{sub ⊥}{sup 2} are not gyrotropic at a given frequency f, a property already observed at larger scales (∥/⊥ means parallel/perpendicular to the average magnetic B{sub 0}). This non-gyrotropy gives indications of the angular distribution of the wave vectors k: at f< 10 Hz, we find that k{sub ⊥}≫k{sub ∥}, mainly in the fast wind; at f > 10 Hz, fluctuations with a non-negligible k {sub ∥} are also present. We then consider the anisotropy ratio δB{sub ∥}{sup 2}/δB{sub ⊥}{sup 2}, which is a measure of the magnetic compressibility of the fluctuations. This ratio, always smaller than 1, increases with f. It reaches a value showing that the fluctuations are more or less isotropic at electron scales, for f⩾50 Hz. From 1 to 15–20 Hz, there is a strong correlation between the observed compressibility and the one expected for the kinetic Alfvén waves (KAWs), which only depends on the total plasma β. For f>15--20 Hz, the observed compressibility is larger than expected for KAWs, and it is stronger in the slow wind: this could be an indication of the presence of a slow-ion acoustic mode of fluctuations, which is more compressive and is favored by the larger values of the electron to proton temperature ratio generally observed in the slow wind.

• OSTI ID: 22875702
• Journal Information: Astrophysical Journal, Journal Name: Astrophysical Journal Journal Issue: 1 Vol. 848; ISSN ASJOAB; ISSN 0004-637X
• Country of Publication: United States
• Language: English

Related Subjects

79 ASTRONOMY AND ASTROPHYSICS
ANGULAR DISTRIBUTION
ANISOTROPY
COMPRESSIBILITY
CORRELATIONS
ELECTRONS
FLUCTUATIONS
MAGNETIC FIELDS
PLASMA
PROTON TEMPERATURE
PROTONS
SOLAR WIND
TURBULENCE