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Table 6 Variables used in this paper

From: Magnetic field stretching at the top of the shell of numerical dynamos

Symbol

Meaning

\(\vec {u}\)

Velocity

\(\vec {B}\)

Magnetic field

t

Time

P

Pressure

T

Temperature (or co-density)

\(\epsilon \)

Heat (or buoyancy) source or sink

Ra

Rayleigh number

E

Ekman number

Pr

Prandtl number

Pm

Magnetic Prandtl number

Rm

Magnetic Reynolds number

Rm a

Effective advective magnetic Reynolds number

Rm s

Effective stretching magnetic Reynolds number

Rm e

Effective magnetic Reynolds number

α

Thermal expansivity

g o

Gravitational acceleration on the outer boundary at radius r o

q o

Mean heat flux across the outer boundary

D

Shell thickness

k

Thermal conductivity

κ

Thermal diffusivity

ν

Kinematic viscosity

Ω

Rotation rate

λ

Magnetic diffusivity

U

Typical velocity scale

L

Typical length scale

\(\hat{z}\)

Unit vector in the direction of the rotation axis

r

Radial coordinate

\(\hat{r}\)

Unit vector in the radial direction

\(\vec {r}\)

Position vector

r o

Earth’s core radius

r e

Radial level at which the simulations were analyzed

\(\bar{\delta \tau }\)

Average time difference between snapshots in units of magnetic advection time

B r

Radial component of the magnetic field on the CMB

\(\vec {u}_{h}\)

2D velocity vector tangent to the CMB spherical surface

St/Ad

Ratio of stretching RMS to advection RMS

\({\mathcal {P}}/{\mathcal {T}}\)

Ratio of poloidal flow RMS to toroidal flow RMS

δ h

Tangential divergence

ω r

Radial vorticity

H u

Helical flow correlation

\(\delta _h^-\)

Downwelling process (δ h < 0)

\(\delta _h^+\)

Upwelling process (δ h > 0)

ξ a

Normalized integrated advective

ξ s

Normalized integrated stretching

ξ e

Normalized integrated magnetic field intensification by stretching

γ

Angle between the vectors \(\vec {u}_h\) and \(\nabla _h B_r\)

cos γ

Field–flow alignment factor

ξ Rm

Advection/stretching interference factor

f

Statistical quantity

C, a, b, c

Generic power law fitting coefficients

σ r

Relative misfit of the power law

f dyn

Statistical quantity in dynamo models

n

Number of dynamo models analyzed

\({\mathcal {T}}_1\)

Large-scale degree-1 toroidal synthetic flow

\({\mathcal {P}}_1\)

Large-scale degree-1 poloidal synthetic flow