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@swensosc points out that we often go through all 40 possible iterations in canopy fluxes. We should assess whether this can be reduced in order to improve performance.
The same issue could be caus…
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The SNR model file currently has this issue:
```
$ python -c 'import gammalib; gammalib.GModels("snrs/ctadc_skymodel_gps_sources_snr.xml")'
Traceback (most recent call last):
File "", line 1, in…
cdeil updated
7 years ago
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## Purpose
We want to implement distributed matrix multiplication to enable parallel online regridding in the coupler.
## Cost/Benefits/Risks
* Costs:
* Developer time
* Risks:
* Incorrect regrid…
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**Model Version**: 4.1.2 and 4.2
**Type**: Bug
**Source file**: phys/module_sf_noahmp_glacier.F
**Description**:
Subsurface temperatures exceeding the melting point are simulated by Noah-MP …
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Requestioned by @paullric who asked me to also cc: @ambrad.
As part of HyperFACETS, I have been running some 4km refined simulations (ne30 refined x32) over the WUS. These apply essentially the sam…
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Hi,
I was looking into the code and unable to find where can i put the parameter for the gas density with which cosmic ray will interact?
For example lets say i want to use 30 cm^-3 as the cloud de…
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In the 1950-spinup simulation we have high-frequency 2D and 3D OpenIFS output (various 6-hourly parameters) and low-frequency 2D and 3D FESOM2 output (monthly, for u, v, and w only yearly). This is o.…
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Hi,
if a model writes 3d output on pressure levels as model levels, what is the CMORization approach?
As far as I know: There is no general "plevs" or "alt"/"height" axis in the tables. Are those mi…
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@BSchilperoort used [MATLAB function profiler](https://nl.mathworks.com/help/matlab/ref/profile.html) to explore execution time for functions in stemmus_scope model. Some functions like `ebal`, `RTMf…
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Land models, in the context of climate, are mostly needed to inform land-atmosphere exchanges (source or sink) of water (evaporation and transpiration), energy (latent and sensible heat flux, shortwav…