Radiocarbon
In this tutorial, we will simulate the radiocarbon age using the AIBECS by
- defining the transport
T(p)and the sources and sinksG(x,p), - defining the parameters
p, - generating the state function
F(x,p)and solving the associated steady-state problem, - and finally making a plot of our simulated radiocarbon age.
Although this tutorial is self-contained, it is slightly more complicated than the first tutorial for simulating the ideal age. (So do not hesitate to start with the idealage tutorial if you wish.)
The tracer equation for radiocarbon is
\[\big(\partial_t + \mathbf{T} \big) \boldsymbol{R} = \frac{\lambda}{h} (\overline{\boldsymbol{R}}_\mathsf{atm} - \boldsymbol{R}) (\boldsymbol{z} ≤ h) - \boldsymbol{R} / \tau.\]
where the first term on the right of the equal sign represents the air–sea gas exchange with a piston velocity $λ$ over a depth $h$ and the second term represents the radioactive decay of radiocarbon with timescale $\tau$.
We need not specify the value of the atmospheric radiocarbon concentration because it is not important for determining the age of a water parcel — only the relative concentration $\boldsymbol{R}/\overline{\boldsymbol{R}}_\mathsf{atm}$ matters.
We start by selecting the circulation for Radiocarbon. .) (And this time, we are using the OCCA matrix by Forget [1].)
using AIBECS
grd, T_OCCA = OCCA.load()The local sources and sinks are simply given by
function G(R,p)
@unpack λ, h, Ratm, τ = p
return @. λ / h * (Ratm - R) * (z ≤ h) - R / τ
endG (generic function with 1 method)We can define z via
z = depthvec(grd)In this tutorial we will specify some units for the parameters. Such features must be imported to be used
import AIBECS: @units, unitsWe define the parameters using the dedicated API from the AIBECS, including keyword arguments and units this time
@units struct RadiocarbonParameters{U} <: AbstractParameters{U}
λ::U | u"m/yr"
h::U | u"m"
τ::U | u"yr"
Ratm::U | u"M"
endunits (generic function with 20 methods)For the air–sea gas exchange, we use a constant piston velocity $\lambda$ of 50m / 10years. And for the radioactive decay we use a timescale $\tau$ of 5730/log(2) years.
p = RadiocarbonParameters(λ = 50u"m"/10u"yr",
h = grd.δdepth[1],
τ = 5730u"yr"/log(2),
Ratm = 42.0u"nM")The parameters are converted to SI units when unpacked. When you specify units for your parameters, you must either supply their values in that unit.
We build the state function F and the corresponding steady-state problem (and solve it) via
F = AIBECSFunction(T_OCCA, G)
x = zeros(length(z)) # an initial guess
prob = SteadyStateProblem(F, x, p)
R = solve(prob, CTKAlg()).uThis should take a few seconds on a laptop. Once the radiocarbon concentration is computed, we can convert it into the corresponding age in years, via
@unpack τ, Ratm = p
C14age = @. log(Ratm / R) * τ * u"s" |> u"yr"and plot it at 700 m using the horizontalslice Plots recipe
using Plots
plothorizontalslice(C14age, grd, depth=700u"m", color=:viridis)look at a zonal average using the zonalaverage plot recipe
plotzonalaverage(C14age, grd; color=:viridis)or look at a meridional slice through the Atlantic at 30°W using the meridionalslice plot recipe
plotmeridionalslice(C14age, grd, lon=-30, color=:viridis)This page was generated using Literate.jl.
- 1Forget, G., 2010: Mapping Ocean Observations in a Dynamical Framework: A 2004–06 Ocean Atlas. J. Phys. Oceanogr., 40, 1201–1221, doi:10.1175/2009JPO4043.1)