Effects of a guided-field on particle diffusion in - - PowerPoint PPT Presentation
Effects of a guided-field on particle diffusion in - - PowerPoint PPT Presentation
Effects of a guided-field on particle diffusion in magnetohydrodynamic turbulence Yue-Kin Tsang Centre for Astrophysical and Geophysical Fluid Dynamics Mathematics, University of Exeter Particle transport in fluids Brownian motion observed
Particle transport in fluids
Brownian motion observed under the microscope dispersion of pollutants in the atmosphere cosmic ray propagation through the interstellar medium We consider passive tracer particles only —- the Lagrangian viewpoint provides an alternative view of the flow structure
Single-particle turbulent diffusion
mean squared displacement: |∆ X(t)|2 , ∆ X(t) = X(t) − X(0) Taylor’s formula (1920) for large t:
- X(t) =
X(0) + t dτ V (τ) |∆ X(t)|2] = 2 t ∞ dτ V (τ) · V (0) = 2tD
assume system is statistically homogeneous and stationary and the integral exists
Lagrangian velocity correlation: CL(τ) = V (τ) · V (0) diffusion coefficient: D = ∞ dτ V (τ) · V (0)
Field-guided MHD turbulence + tracers
Electrically conducting fluid in a 3D periodic domain: ∂ u ∂t + ( u · ∇) u = − 1 ρ0 ∇p + (∇ × B) × B + ν∇2 u + f ∂ B ∂t = ∇ × ( u × B) + η∇2 B ∇ · u = ∇ · B = 0
- f : isotropic random forcing at the largest scales, ∆t-correlated
Field-guided MHD turbulence:
- B(
x, t) = B0ˆ z + b( x, t) Evolution of passive tracer particles: d X(t) dt = V (t) = u( X(t), t)
- X(0) : uniformly distributed over the domain
Previous work: the 2D case
Turbulent transport (ηT ) suppressed when B0 > B∗
0 ∼ Rm−1 (Rm = UL/η)
(Vainshtein & Rosner 1991, Cattaneo & Vainshtein 1991, Cattaneo 1994, Gruzinov & Diamond 1994, Kondi´ c, Hughes & Tobias 2016)
Q : Does suppression of turbulent diffusion occur in 3D ?
Eulerian fields
hydrodynamic
- u
B0 = 1
- u
- b
ν = η ∼ 10−3 Re = Rm ∼ 103 256 × 256 × 256
Ratios of Eulerian r.m.s. velocities
1 2 3 0.9 0.95 1 1.05 1.1 1.15
A urms/wrms
dynamo 0.1 0.2 0.3 1.0 5.0 hydro
1 2 3 0.9 0.95 1 1.05 1.1 1.15
A vrms/wrms
A = forcing amplitude urms wrms ≈ vrms wrms ≈ 1
Particle trajectories
hydrodynamic B0 = 1 transport becomes anisotropic when B0 = 0
Scaling of mean squared displacement
100 200 300 400 50 100 150 200
<(∆x)2> <(∆y)2> <(∆z)2)>
hydrodynamic 100 200 300 400 50 100 150 200 field-guided 10
- 2
10
- 1
10 10
1
10
2
elapsed time, t 10
- 4
10
- 2
10 10
2
10
- 2
10
- 1
10 10
1
10
2
elapsed time, t 10
- 4
10
- 2
10 10
2
t2 t2 t t
Dx=0.24 Dy=0.25 Dz=0.25 Dx=0.04 Dy=0.04 Dz=0.26
ballistic limit: ∼ t2 at small time diffusive scaling: ∼ t at large time, (∆x)2 ∼ 2Dxt , etc
Lagrangian velocity correlation function CL(τ) = V (τ) · V (0)
10 20 30 40 50
τ
- 0.05
0.00 0.05 0.10 0.15 0.20
CL,u CL,v CL,w hydrodynamic
10 20 30 40 50
τ
- 0.05
0.00 0.05 0.10 0.15 0.20
field-guided
hydrodynamic: ∼ exp(−τ), short correlation time field-guided: oscillatory, long correlation time how things depend on the guided-field strength B0?
Diffusivity at different (weak) B0 Urms
0.5 1 1.5 2 0.2 0.4 0.6 0.8 1 1.2
Urms Dx
hydro 0.1 0.2 0.3 0.5 1 1.5 2 0.2 0.4 0.6 0.8 1 1.2
Urms Dy
0.5 1 1.5 2 0.2 0.4 0.6 0.8 1 1.2
Urms Dz
0.5 1 1.5 2 0.2 0.4 0.6 0.8 1
Urms Dx/Dz
0.5 1 1.5 2 0.2 0.4 0.6 0.8 1
Urms Dy/Dz
diffusion is reduced by B0, including the z-direction anisotropic suppression: Dx, Dy Dz strong Urms( B0) reduces the anisotropy in D’s
Diffusivity at different B0
0.5 1 1.5 2 0.2 0.4 0.6 0.8 1 1.2
Urms Dx
hydro 0.1 0.2 0.3 1.0 5.0 0.5 1 1.5 2 0.2 0.4 0.6 0.8 1 1.2
Urms Dy
0.5 1 1.5 2 0.2 0.4 0.6 0.8 1 1.2
Urms Dz
0.5 1 1.5 2 0.2 0.4 0.6 0.8 1
Urms Dx/Dz
0.5 1 1.5 2 0.2 0.4 0.6 0.8 1
Urms Dy/Dz
At strong guided-field strength, B0 Urms Dx, Dy are strong suppressed, anomalous behavior of Dz Dx/Dz , Dy/Dz ≪ 1 for the values of Urms studied
Anisotropic turbulent diffusion
0.7 0.8 0.9 1 0.2 0.4 0.6 0.8 1
brms /Urms Dx/Dz
0.7 0.8 0.9 1 0.2 0.4 0.6 0.8 1
brms /Urms Dy/Dz
−1.5 −1 −0.5 0.5 1 0.2 0.4 0.6 0.8 1
log(B 0z /Urms) Dx/Dz
−1.5 −1 −0.5 0.5 1 0.2 0.4 0.6 0.8 1
log(B 0z /Urms) Dy/Dz
Particle trajectories B0 = 0.2, Urms = 1.42 Dx/Dz = 0.95
−15 −10 −5 5 10 15 20 −10 −5 5 10 15 −15 −10 −5 5 10 15 y amp=3 , ν=1.25e−03 , η=1.25e−03 , B0z=0.2 , Lz=1 , nx=256 , ny=256 , nz=256 x z
B0 = 1.0, Urms = 0.29 Dx/Dz = 0.24
2 4 6 8 10 −5 5 10 15 −10 −5 5 10 y amp=0.1 , ν=1.25e−03 , η=1.25e−03 , B0z=1 , Lz=1 , nx=256 , ny=256 , nz=256 x z
Particle trajectories B0 = 0.2, Urms = 0.25 Dx/Dz = 0.34
5 10 −5 5 −5 5 10 15 20 25 y amp=0.1 , ν=1.25e−03 , η=1.25e−03 , B0z=0.2 , Lz=1 , nx=256 , ny=256 , nz=256 x z
B0 = 1.0, Urms = 1.39 Dx/Dz = 0.34
−5 5 10 15 −5 5 10 −20 −15 −10 −5 5 10 y amp=3 , ν=1.25e−03 , η=1.25e−03 , B0z=1 , Lz=1 , nx=256 , ny=256 , nz=256 x z
Lagrangian velocity correlation
20 40 60 80 100 −0.005 0.005 0.01 0.015 0.02 0.025
B0z =0.2 , Urms =0.25 CL,u CL,v CL,w
5 10 15 20 −0.1 0.1 0.2 0.3 0.4 0.5 0.6 0.7 0.8
B0z =0.2 , Urms =1.42
20 40 60 80 100 −0.02 −0.01 0.01 0.02 0.03 0.04
B0z =1.0 , Urms =0.29 elapsed time
5 10 15 20 −0.2 0.2 0.4 0.6 0.8 1 1.2
B0z =1.0 , Urms =1.39 elapsed time
Velocity decorrelation time
10
−1
10 10 10
1
10
2
u r m s τx
dynamo 0.1 0.2 1.0 5.0 hydro
10 10 10
1
10
2
10
3
u r m s/B0 τxB0
Velocity decorrelation time
10
−1
10 10 10
1
10
2
u r m s τx
−1 −2
dynamo 0.1 0.2 1.0 5.0 hydro
10 10 10
1
10
2
10
3
u r m s/B0 τxB0
−1 −2
urms/B0 > 1 : τx ∼ (urms)−1 [τxB0 ∼ (urms/B0)−1] urms/B0 < 1 : τx ∼ B0(urms)−2 [τxB0 ∼ (urms/B0)−2]
- ngoing work: ensemble averaging to get better statistics