| ... | ... | @@ -42,9 +42,9 @@ First, each user have to download reference repository (NEMOREF/CROCOREF) with t |
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###### Connexion ssh
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First of all, to retrieve the repository make sure that your public keys have been copied and pasted into the box (see picture below)
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If necessary, you will have to go to your local directory **~/.ssh/** and retrieve the *.pub file
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If not present type on your pc:
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First of all, to retrieve this repository, make sure that your public keys have been copied and pasted into the box (see picture below)
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If necessary, you will have to go to your local directory **~/.ssh/** and to retrieve the *.pub file
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If it is not present within, just type on your pc:
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```console
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ssh-keygen -t rsa -C "key for you"
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| ... | ... | @@ -75,7 +75,7 @@ git config --global http.https://forge.ird.fr.proxy http://proxy.legos.obs-mip.f |
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```
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###### Alternative if ssh/https connexion dont work
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###### Alternative if ssh/https connexion don't work
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Remind in that case, you will download only a snapshot of remote repository, so please take care to choose the correct tag, and then like in this picture below:
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| ... | ... | @@ -126,7 +126,7 @@ If you are not friendly with the repos, the user can proceed in this way to sear |
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**OCEAN** :
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MERCATOR GLORYS (GLobal Ocean ReanalYsis and Simulation) reanalysis are based on the PSY4 system which is a global high resolution ocean monitoring and forecasting system from Mercator.
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MERCATOR GLORYS (GLobal Ocean ReanalYsis and Simulation) reanalysis are based on the PSY4 system which is a global high resolution ocean monitoring and forecasting system from Mercator. It was also developed for the Copernicus Marine Environment Monitoring Service (CMEMS; http://marine.copernicus.eu/). A full description of the system components is available in [Lellouche et al. (2018) ](https://os.copernicus.org/articles/14/1093/2018/)
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* MERCATOR GLORYS2V4
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| ... | ... | @@ -181,7 +181,7 @@ If you are not friendly with the repos, the user can proceed in this way to sear |
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| ssrd(J/m2) (Surface solar radiation downwards) | radsw (W/m2) | also known as downward shortwave radiation at the sea surface (1h ERA5 field : radsw=ssrd/3600) |
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| strd(J/m2) (Surface thermal radiation downwards) | radlw (W/m2) | also known as downward longwave radiation at the sea surface (1h ERA5 field : radlw=strd/3600) |
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| tp(m) (Total precipitation (precip+solid precip(snow))) | precip (kg/(m2s) == mm/s) | keep in mind : 1 mm of water = 1L/m2 = 1Kg/m2 (1h ERA5 field : precip=tp*1000/3600) |
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| snow(m) | snow (kg/(m2s)) | precip*0 |
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| snow(m) | snow (kg/(m2s)) | precip*0 (for our use) |
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| ... | ... | @@ -201,7 +201,7 @@ If you are not friendly with the repos, the user can proceed in this way to sear |
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**BATHY** :
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* Global Bathymetry from ETOPO1, ETOPO2
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* Global Bathymetry from GEBCO 2019 (15arc second ~500m)
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* Global Bathymetry from GEBCO 2019 (15arc second about ~500m)
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* Global Bathymetry From T-UGOm + postprocessing from F.Lyard . It's an improved topography in coastal environments developed by Florent Lyard and Damien Alain for FES2020 including new bathymetry data not taken into account in ETOPO2 and GEBCO1
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| ... | ... | @@ -227,14 +227,14 @@ Is one of the first step of the preprocessing of a Nemo configuration. The inter |
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* from mercator simulation BIOMER4V2R1
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Nemo wait for variable in mol/L, so there is a multiplicative factor to convert inputs from mL/L to mol/L
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Nemo code is waiting for variable unit in mol/L, so there is a multiplicative factor to convert inputs from mL/L to mol/L
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* for N : ratio no3/c = 7.65
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* for P : ratio po4/c = 122
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* for O2 : n=Vo2/Vmol=1000L/22.4L.mol-1=44.6
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| Inputs for initialization and OBC | frequency | Units WOA18 | factor |
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| Inputs for initialization and OBC | frequency used | Units WOA18 | factor to apply |
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|:---:|:---:|:---:|:---:|
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| DIC (Dissolved Inorganic Concentration) | annual | umol.L | 1e-6 |
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| DOC (Dissolved organic Concentration) | annual | umol.L | 1e-6 |
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| ... | ... | @@ -247,13 +247,13 @@ Nemo wait for variable in mol/L, so there is a multiplicative factor to convert |
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| Inputs for optics and deposition process | frequency | Units | - |
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| Inputs for optics and deposition process | frequency used | Units | - |
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|:---:|:---:|:---:|:---:|
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| Percentage of PAR (Photosynthetically available radiation) in shortwave | daily | - | |
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| Dust from atmosphere | monthly | Dust Kg.m-2.s-1 | |
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| Solubility for atm. Iron | annual | - | |
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| atmospheric N deposition | annual | - | |
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| Fe bathy (beach) | annual | - | |
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| Fe bathy (coastline) | annual | - | |
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| river inputs DIC | daily | - | |
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| river inputs DOC | daily | - | |
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| river inputs DIN (Nitrogen) | daily | - | |
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| ... | ... | @@ -289,7 +289,7 @@ All these files are versioned for a configuration given here _CONFIG_CASE_: |
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WEIGHTS/
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> **Note** : We keep this tree structure, we could imagine source modified from other models such as WRF, for some coupled configuration with NEMO for example. In this case, We will have: NEMO_CONFIGS/models/WRFSRC/... see NEMO_CONFIGS/models/SDAP mirrored... see new repo SDAP ?
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> **Note** : We keep this tree structure, we could imagine source modified from other models such as WRF, for some coupled configuration with NEMO for example. In this case, We will have: NEMO_CONFIGS/models/WRFSRC/... see NEMO_CONFIGS/models/SDAP mirrored...
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**2**. setup : configuration file __includefile.ini__ contains set of environment variables corresponding to the CONFIG_CASE config as well as the jobs scripts used to execute the model on a given cluster
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