Studying Anisotropy of Compressible Magnetohydrodynamic Turbulence by Synchrotron Polarization Intensity
arXiv:2001.03276 · doi:10.3847/1538-4357/ab6a1a
Abstract
Based on statistical analysis of synchrotron polarization intensity, we study the anisotropic properties of compressible magnetohydrodynamic (MHD) turbulence. The second-order normalized structure function, quadrupole ratio modulus and anisotropic coefficient are synergistically used to characterize the anisotropy of the polarization intensity. On the basis of pre-decomposition data cubes, we first explore the anisotropy of the polarization intensity in different turbulence regimes and find that the most significant anisotropy occurs in the sub-Alfvénic regime. Using post-decomposition data cubes in this regime, we then study the anisotropy of the polarization intensity from Alfvén, slow and fast modes. Statistics of polarization intensity from Alfvén and slow modes demonstrate the significant anisotropy while statistics of polarization intensity from fast modes show isotropic structures, which is consistent with the earlier results provided in Cho & Lazarian (2002). As a result, both quadrupole ratio modulus and anisotropic coefficient for polarization intensities can quantitatively recover the anisotropy of underlying compressible MHD turbulence. The synergistic use of the two methods helps enhance the reliability of the magnetic field measurement.
arXiv comment13 pages with 12 Figures and 1 Table. Accepted by ApJ
References in corpus (32)
- Theory of Star Formation
- Control of star formation by supersonic turbulence
- Interstellar Turbulence I: Observations and Processes
- The Interstellar Environment of our Galaxy
- Reconnection in a Weakly Stochastic Field
- Faraday Rotation Measure Synthesis
- The Anisotropy of MHD Alfvénic Turbulence
- Simulations of Incompressible MHD Turbulence
- Compressible Magnetohydrodynamic Turbulence: mode coupling, scaling relations, anisotropy, new regime and astrophysical implications
- Thermal Conduction in Clusters of Galaxies
- Simulations of MHD Turbulence in a Strongly Magnetized Medium
- Compressible Sub-Alfvenic MHD turbulence in Low-beta Plasmas
- Compressible MHD Turbulence in Interstellar Plasmas
- Magnetic fields and spiral arms in the galaxy M51
- Cosmic Ray Propagation: Nonlinear Diffusion Parallel and Perpendicular to Mean Magnetic Field
- Velocity Field of Compressible MHD Turbulence: Wavelet Decomposition and Mode Scalings
- Low-Mach-number turbulence in interstellar gas revealed by radio polarization gradients
- Enhancement and suppression of heat transfer by MHD turbulence
- Statistical Description of Synchrotron Intensity Fluctuations: Studies of Astrophysical Magnetic Turbulence
- Magnetic Fields in the Milky Way
- Faraday tomography of the local interstellar medium with LOFAR: Galactic foregrounds towards IC342
- Linear polarization structures in LOFAR observations of the interstellar medium in the 3C196 field
- Spectrum and Anisotropy of Turbulence from Multi-Frequency Measurement of Synchrotron Polarization
- Properties of Interstellar Turbulence from Gradients of Linear Radio Polarization Maps
- Gradients of Synchrotron Polarization: Tracing 3D distribution of magnetic fields
- The Galactic Magneto-Ionic Medium Survey: Moments of the Faraday Spectra
- Radio Synchrotron Fluctuation Statistics as a Probe of Magnetized Interstellar Turbulence
- Studying Magnetohydrodynamic Turbulence with Synchrotron Polarization Dispersion
- Spectral properties of magnetohydrodnamic turbulence revealed by polarization synchrotron emission with Faraday rotation
- The effect of Large Magellanic Cloud on the satellite galaxy population in Milky Way analogous Galaxies
- Tracing magnetic fields by the synergies of synchrotron emission gradients
- Advanced Diagnostics for the Study of Linearly Polarized Emission. I: Derivation
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