Nomenclature

From Atomix


Background (total) velocity

Symbol Description Units
u zonal or longitudinal component of velocity ms−1
v meridional or transverse component of velocity ms−1
w vertical component of velocity ms−1
ue error velocity ms−1
V velocity perpendicular to mean flow ms−1
Wd Profiler fall speed ms−1
UP Flow speed past sensor ms−1
b Along-beam velocity from acoustic Doppler sensor ms−1
b′ Along-beam velocity from acoustic Doppler sensor with background flow deducted ms−1
δz Vertical size of measurement bin for acoustic Doppler sensor m
r Along-beam distance from acoustic Doppler sensor m
δr0 Along-beam bin size for acoustic Doppler sensor m
δr Along-beam bin separation for acoustic Doppler sensor m
θ Beam transmit and receive angle relative to instrument axis for acoustic Doppler sensor ∘

Turbulence properties

Symbol Description Eqn Units
ε The rate of dissipation of turbulent kinetic energy per unit mass by viscosity Wkg−1
B Buoyancy production -- the rate of production of potential energy by turbulence in a stratified flow through the vertical flux of buoyancy. B=gρρ′w′‾ Wkg−1
P The production of turbulence kinetic energy. In a steady, spatially uniform and stratified shear flow, turbulence kinetic energy is produced by the product of the Reynolds stress and the shear, for example P=−u′w′‾∂U∂z . The production is balanced by the rate of dissipation turbulence kinetic energy, ε, and the production of potential energy by the buoyancy flux, B. P=−u′w′‾∂U∂z=ε+B Wkg−1
Rf Flux Richardson number; the ratio of the buoyancy flux expended for the net change in potential energy (i.e., mixing) to the shear production of turbulent kinetic energy. Rf=BP
Γ "Mixing coefficient"; The ratio of the rate of production of potential energy, B, to the rate of dissipation of kinetic energy, ε. Γ=Bε=Rf1−Rf
Ri (Gradient) Richardson number; the ratio of buoyancy freqency squared to velocity shear squared Ri=N2S2
κρ Turbulent eddy diffusivity via the Osborn (1980) model κρ=ΓεN−2 m2s−1
Dll Second-order longitudinal structure function Dll=⟨[b′(r)−b′(r+nδr)]2⟩ m2s−2

Fluid properties and background gradients for turbulence calculations

Symbol Description Eqn Units
SP Practical salinity −
T Temperature ∘C
P Pressure dbar
ρ Density of water ρ=ρ(T,Sa,P) kgm−3
α Temperature coefficient of expansion α=1ρ∂ρ∂T K−1
β Saline coefficient of contraction β=1ρ∂ρ∂SP
S Background velocity shear S=[(∂U∂z)2+(∂V∂z)2]1/2 s−1
ν35 Temperature dependent kinematic viscosity of seawater at a practical salinity of 35 ∼1×10−6 m2s−1
ν00 Temperature dependent kinematic viscosity of freshwater ∼1×10−6 m2s−1
Γa Adiabatic temperature gradient -- salinity, temperature and pressure dependent ∼1×10−4 Kdbar−1
N Background stratification, i.e buoyancy frequency N2=g[α(Γa+∂T∂z)−β∂SP∂z] rads−1

Theoretical Length and Time Scales

Symbol Description Eqn Units
τN Buoyancy timescale τN=1N s
TN Buoyancy period TN=2πN s
LE Ellison length scale (limit of vertical displacement without irreversible mixing) LE=⟨ρ'2⟩1/2∂ρ‾/∂z m
LZ Boundary (law of the wall) length scale LZ=0.39zw with 0.39 being von Kármán's constant m
LS Corssin length scale LS=ε/S3 m
LK Kolmogorov length scale (smallest overturns) LK=(ν3ε)1/4 m
Lo Ozmidov length scale, measure of largest overturns in a stratified fluid Lo=(εN3)1/2 m
LT Thorpe length scale LT m
zw Distance from a boundary zw m

Turbulence Spectrum

These variables are used to express the Turbulence spectrum expected shapes.


Symbol Description Eqn Units
Δt Sampling interval 1fs s
fs Sampling rate fs=1Δt s−1
Δs Sample spacing Δs=UPΔt m
Δl Linear dimension of sampling volume (instrument dependent) m
f Cyclic frequency f=ω2π Hz
ω Angular frequency ω=2πf rads−1
fN Nyquist frequency fN=0.5fs Hz
k Cyclic wavenumber k=fUP cpm
k̂ Angular wavenumber k̂=ωUP=2πk radm−1
k~ Normalized wavenumber e.g., k~=kLK,LK=(ν3/ε)1/4 -
Φ~ Normalized velocity spectrum e.g., Φ~u(k~)=(ϵν5)−1/4Φu(k) -
Ψ~ Normalized shear spectrum e.g., Ψ~(k~)=LK2(ϵν5)−1/4Ψ(k) -
kΔ Nyquist wavenumber, based on sampling volume size Δl kΔ=0.5Δl cpm
kN Nyquist wavenumber, via Taylor's hypothesis kN=fNUP cpm
Ψ(k) Shear spectrum. Use Ψ1, Ψ2 to distinguish the orthogonal components of the shear. Use ΨN for the Nasmyth spectrum, ΨPK for the Panchev-Kesich spectrum and ΨL for the Lueck spectrum. s−2cpm−1
Φ(k) Velocity spectrum. Use Φu, Φv, Φv, or Φ1, Φ2 , Φ3 for the different orthogonal components of the velocity. Use ΦK for the Kolmogorov spectrum. m2s−2cpm−1