The supernova-regulated ISM. III. Generation of vorticity, helicity and mean flows
arXiv:1705.08642 · doi:10.1051/0004-6361/201731228
Abstract
The forcing of interstellar turbulence, driven mainly by supernova explosions, is irrotational in nature, but the development of significant amounts of vorticity and helicity, accompanied by large-scale dynamo action, has been reported. Several earlier investigations examined vorticity production in simpler systems; here all the relevant processes can be considered simultaneously. We also investigate the mechanisms for the generation of net helicity and large-scale flow in the system. We use a three-dimensional, stratified, rotating and shearing local simulation domain of the size 1x1x2 kpc, forced with SN explosions occurring at the rate typical of the solar neighbourhood in the Milky Way. In addition to the nominal simulation run with realistic Milky Way parameters, we vary the rotation and shear rates, but keep the absolute value of their ratio fixed. Reversing the sign of shear vs. rotation allows us to separate the rotation- and shear-generated contributions. As in earlier studies, we find the generation of significant amounts of vorticity, with on average 65% of the kinetic energy being in the rotational modes. The vorticity production can be related to the baroclinicity of the flow, especially in the regions of hot, dilute clustered supernova bubbles. In these regions, the vortex stretching acts as a sink of vorticity. The net helicities produced by rotation and shear are of opposite signs for physically motivated rotation laws, with the solar neighbourhood parameters resulting in the near cancellation of the total net helicity. We also find the excitation of oscillatory mean flows, the strength and oscillation period of which depend on the Coriolis and shear parameters; we interpret these as signatures of the anisotropic kinetic (AKA) effect. We use the method of moments to fit for the turbulent transport coeffcients, and find values of the order 3-5 km/s.
arXiv comment19 pages, 12 figures, Astronomy and Astrophysics, accepted for publication
References in corpus (39)
- Astrophysical magnetic fields and nonlinear dynamo theory
- The Millennium Arecibo 21-CM Absorption Line Survey. II. Properties of the Warm and Cold Neutral Media
- The Vertical Structure of Warm Ionised Gas in the Milky Way
- Turbulent Structure of a Stratified Supernova-Driven Interstellar Medium
- Mean-field concept and direct numerical simulations of rotating magnetoconvection and the geodynamo
- Differential Rotation and Turbulence in Extended HI Disks
- Supernova Driving. I. The Origin of Molecular Cloud Turbulence
- LOFAR, VLA, and Chandra observations of the Toothbrush galaxy cluster
- Electromotive Force and Large-Scale Magnetic Dynamo in a Turbulent Flow with a Mean Shear
- Direct simulations of a supernova-driven galactic dynamo
- The Distribution of Pressures in a Supernova-Driven Interstellar Medium. I. Magnetized Medium
- The Generation and Dissipation of Interstellar Turbulence - Results from Large Scale High Resolution Simulations
- The supernova-regulated ISM. I. The multi-phase structure
- Constraining turbulence and conduction in the hot ICM through density perturbations
- Local and nonlocal magnetic diffusion and alpha-effect tensors in shear flow turbulence
- Generation of Magnetic Fields in the Multi-phase ISM with Supernova-Driven Turbulence
- Saturated-State Turbulence and Structure from Thermal and Magnetorotational Instability in the ISM: Three-Dimensional Numerical Simulations
- Models of Vertically Stratified Two-Phase ISM Disks with MRI-Driven Turbulence
- The supernova-regulated ISM. II. The mean magnetic field
- Magnetic Fields in the Milky Way
- The mean electromotive force due to turbulence of a conducting fluid in the presence of mean flow
- Cosmic ray driven dynamo in galactic disks. A parameter study
- Structure distribution and turbulence in self-consistently supernova-driven ISM of multiphase magnetized galactic discs
- Filling factors and scale heights of the DIG in the Milky Way
- Turbulence from localized random expansion waves
- Large-scale flow generation by inhomogeneous helicity
- An observational test for correlations between cosmic rays and magnetic fields
- Generation of Large-Scale Vorticity in a Homogeneous Turbulence with a Mean Velocity Shear
- Dynamo saturation in direct simulations of the multi-phase turbulent interstellar medium
- Toward a hybrid dynamo model for the Milky Way
- Vorticity production through rotation, shear and baroclinicity
- The alpha effect in rotating convection with sinusoidal shear
- Supernova-regulated ISM -- V. Space- and time-correlations
- The distribution of mean and fluctuating magnetic fields in the multi-phase ISM
- Reynolds stresses from hydrodynamic turbulence with shear and rotation
- Astrophysical significance of the anisotropic kinetic alpha effect
- Global Models of the Galactic Interstellar Medium: Comparison to X-Ray and H I Observations
- Influence of Ohmic diffusion on the excitation and dynamics of MRI
- Moffatt drift driven large scale dynamo due to fluctuations with nonzero correlation times
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- Advances in mean-field dynamo theory and applications to astrophysical turbulence
- Turbulent dynamo in the two-phase interstellar medium
- The Impact of Type Ia Supernovae in Quiescent Galaxies: II. Energetics and Turbulence
- Clustering and dynamic decoupling of dust grains in turbulent molecular clouds
- The small-scale dynamo in a multiphase supernova-driven medium
- The Catalogue for Astrophysical Turbulence Simulations (CATS)
- Transition from small-scale to large-scale dynamo in a supernova-driven, multiphase medium
- Turbulent viscosity and effective magnetic Prandtl number from simulations of isotropically forced turbulence
- Modelling supernova driven turbulence
- Magnetic and rotational quenching of the effect
- Mechanism of mean flow generation in rotating turbulence through inhomogeneous helicity
- Compressible test-field method and its application to shear dynamos
- Non-linear Galactic Dynamos and the Magnetic Rädler Effect
- The supernova-regulated ISM. IV. A comparison of simulated polarization with Planck observations
- Effects of small-scale dynamo and compressibility on the effect
- Magnetic dynamos in galaxy clusters: the crucial role of galaxy formation physics at high redshifts
- Mean field dynamo action in shear flows. I: fixed kinetic helicity
- Vorticity and magnetic dynamo from subsonic expansion waves
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