This document briefly introduces ongoing work to enhance the 3D radiative transfer solver which is coupled to the DALES model. It turns out that strong aspect ratios lead to an enhanced downward direction of radiation propagation in the Tenstream radiative transfer solver. To overcome this, at least partially, I played with some implementations of higher order solvers.
The cloud field has strong aspect ratios with horizontal resolution of 100m and a vertical resolution of 12m, encompassing 96*96*456 voxels. One particular problem, it seems, are the heat spots which are generated at the surface. It was known before that the Tenstream is not very diffusive with only two streams in the vertical and to represent the horizontal spread of diffuse radiation correctly, we now introduce 8 streams also for the vertical propagation of radiation.
Following graphs show the error distributions for the total radiative flux at the surface for each solver compared to MonteCarlo benchmark simulations.
I.e. histogram( E_srfc(*) - E_srfc(3D MYSTIC) ) for several solar zenith angles
Following graph gives the relative Root Mean Squared Error for the individual solvers at several solar zenith angles.
max(abs(E_surface(*) - E_surface(MYSTIC)))
(sidenote: to account for montecarlo noise, I smoothed the difference fields with a 2D uniform filter with size 4)
SZA | 1D max difference [W/m2] | 8_10 max difference [W/m2] | 8_16 max difference [W/m2] |
---|---|---|---|
0 | 356 | 195 | 136 |
20 | 905 | 210 | 157 |
40 | 898 | 295 | 186 |
60 | 602 | 271 | 132 |
80 | 92 | 123 | 44 |
Following graphs show the srfc irradiance (direct + diffuse)
Following graphs show the srfc irradiance (direct + diffuse)
Just to make sure that mennos cloud field is not just a freak accident, lets do the same analysis on the by now well known I3RC1 cumulus cloud field which was use many times before for our benchmarking
Following graphs show the error distributions for the total radiative flux at the surface for each solver compared to MonteCarlo benchmark simulations.
I.e. histogram( E_srfc(*) - E_srfc(3D MYSTIC) ) for several solar zenith angles
max(abs(E_surface(*) - E_surface(MYSTIC)))
SZA | 1D | 8_10 | 8_16 |
---|---|---|---|
0 | 422 | 230 | 167 |
20 | 779 | 257 | 187 |
40 | 835 | 264 | 192 |
60 | 547 | 231 | 149 |
80 | 132 | 109 | 69 |