Skip Monte Carlo computations for g-points with high gasous optical depths#68
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MennoVeerman wants to merge 5 commits intomicrohh:developfrom
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Skip Monte Carlo computations for g-points with high gasous optical depths#68MennoVeerman wants to merge 5 commits intomicrohh:developfrom
MennoVeerman wants to merge 5 commits intomicrohh:developfrom
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…ntroduced tau_frac_threshold will be used in next commit) and simplify command line code
…ouble precision now
…h g-point. If this ratio is above a provided threshold value (command line argumen, with a default of 0.1), compute surface and tod fluxes and flux absorption rates based on the 1D computations
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Would it not make more sense in terms of physics to also include the ratio of mean free path to grid spacing? Whether you need 3D also depends on that. |
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Instead of using f_tau, we can switch to using the ratio between the gas mean free path and the grid spacing to decide whether to do monte carlo or not. This ratio can be provided by the user and defaults to ~1? |
…st mean free path and the small horizontal grid dimension to decide whether to use 3D monte carlo or simply the 1D solution
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G-points with high gaseous optical depth barely show any impact of clouds, but introduce a significant amount of noise. User can define a threshold ratio between the maximum gas and cloud optical depths (per-cell, not vertically integrated). If the ratio exceeds this threshold, use 1D fluxes instead of MC ray tracing. This threshold defaults to 0.1, in which case less than half of the g-points are run in 3D