Open MatthisAuger opened 1 year ago
Same thing for the surface layer:
Along the boundary: https://user-images.githubusercontent.com/68908668/213604623-a53fcd56-c315-4064-a4e9-12e0b7fc95a5.mp4 And location of the transect
Across the boundary https://user-images.githubusercontent.com/68908668/213604621-acaa47b4-d1f3-4aa0-8237-36f9e76d21c7.mp4 And location of the transect
Update from our meeting 20/1/23:
The movies above show that there are particularly large u velocities at the northern open boundary. To investigate this more, we can:
@MatthisAuger and @PaulSpence and @pedrocol volunteered to look into this.
@adele157 @AndyHoggANU Can you please point me to the latest mom6 panan config that we should use to test the boundary condition settings? We aim to start testing them today. Thanks!
Probably this branch, for 0.1° zstar: https://github.com/COSIMA/mom6-panan/tree/panan-01-zstar-run
Just a quick plot of sea level at the boundary. Those are sea level variations over one year for the 1st year of simulation (red) and the boundary conditions (black) at one particular longitude.
If both variables are supposed to be the sea level above the geoid then it explains the strong U along the boundary. Looking at the Mean Sea Surface plots at 37S it looks like the model has the good order of magnitude of sea level and not the boundary conditions files (the plot is at longitude 70E)
Wow that's a big difference! Might be useful to compare lat/lon maps of SSH in the panantarctic and ACCESS-OM2-01-RYF. Is the RYF just really biased or is there something wrong with the boundary forcing?
Yes, it is a big difference. But the offset surprises me -- I had thought U oscillated a bit and was positive at some times, negative at others.
Maybe it's just a definition of sea level? If yes, SSH gradient perpendicular to the boundary would tell us?
Hi Folks,
We are running 1 month sims varying these params in MOM_input: OBC_SEGMENT_001_VELOCITY_NUDGING_TIMESCALES = .3, 360.0 ! inflow and outflow timescales OBC_TRACER_RESERVOIR_LENGTH_SCALE_OUT = 30000 OBC_TRACER_RESERVOIR_LENGTH_SCALE_IN = 3000
See relevant code here: https://github.com/mom-ocean/MOM6/blob/7467a63efea7025ceb9118448d593709dc1cdf47/src/core/MOM_open_boundary.F90
Since we don't understand this code, the plan is to run the following 2 and 0.5 sensitivity tests: 1) OBC_SEGMENT_001_VELOCITY_NUDGING_TIMESCALES = .6, 720.0 ! inflow and outflow timescales 2 2) OBC_SEGMENT_001_VELOCITY_NUDGING_TIMESCALES = .15, 180.0 ! inflow and outflow timescales .5 3) OBC_TRACER_RESERVOIR_LENGTH_SCALE_OUT = 60000 OBC_TRACER_RESERVOIR_LENGTH_SCALE_IN = 6000 4) OBC_TRACER_RESERVOIR_LENGTH_SCALE_OUT = 15000 OBC_TRACER_RESERVOIR_LENGTH_SCALE_IN = 1500
Trial by brushfire :)
I think one of the configs that inspired our choice of parameters was https://github.com/ESMG/ESMG-configs/tree/dev/esmg/CCS2, although the reservoir length scales are different to that one: they're swapped. I think we adopted that because the other configuration we looked at (https://github.com/ESMG/Arctic6) doesn't override them at all, but we were getting issues leaving them at the defaults.
Thanks @MatthisAuger.
Does the panan model directly use the ACCESS-OM2-01-RYF SSH at the boundary value when calculating its pressure gradient?
It doesn't appear to, at least from your plot. If I'm reading it correctly, it shows SSH increases to the south, implying a westward geostrophic current, but I think your movies show it's mostly eastward. Also a ~0.7m difference over 0.08°=8.9km implies a zonal geostrophic current of ~8.8 m/s at 37S, which is pretty extreme and seems more than what your movies were showing. I also share Andy's surprise that the SSH offset is nearly constant in time, in contrast to the U anomalies.
So all up, I don't think the SSH difference is consistent with the anomalous velocity, but I agree with Adele that lat/lon maps (ideally movies) of SSH difference between the panantarctic and ACCESS-OM2-01-RYF would be helpful, to get a fuller picture of the spatial pattern.
Although I'm not sure whether this SSH difference is relevant to the U anomaly, so this is probably a rabbithole, I'm still wondering how the SSH difference can be maintained.
Here is the zonal mean of the SSH at 37S for the cases listed by @PaulSpence
Nudging timescale seems seem to have a strong impact, with a SSH difference of 1cm between the 0.5 and 2 cases, which might be a lot considering that this is a zonal mean over all the longitudes.
About the SSH difference between ACCESS OM and panant, the fields look very different. (I am even wondering if I'm getting the right variables?) Sorry for the not convenient image formats (edit: 2nd was the wrong figure)
2 snapshots on the same day (notice the different colorbar)
mean difference over 1 year
And movie of the difference (mean difference removed):
Discussion from today's meeting: The SSH offset may be arising because we are setting a 0m initial condition for sea level. Averaged south of 37S, the sea level in obs and ACCESS-OM2 is way less than 0m (perhaps equal to the 0.8m offset we are seeing?).
Suggestions from today's meeting:
Check if the boundary condition is mass conserving (check mom6.out and plot a time series of total mass).
There's also ocean.stats
and ocean.stats.nc
to avoid as much manual parsing.
@willaguiar do you feel like looking into whether the regional model and boundary condition are mass conserving? (see last two comments above)
@adele157 Yes! - I can do that and post here the results.
@willaguiar do you feel like looking into whether the regional model and boundary condition are mass conserving? (see last two comments above)
Yes! - I will do it. (I'll post the update/figs here)
But does the SSH difference at the boundary play any role in the U anomalies at the boundary? It doesn't look like it to me - see above
I think we still want to fix the SSH offset though even if it's not causing the anomalies.
On Fri, 3 Feb 2023 at 10:48, Andrew Kiss @.***> wrote:
But does the SSH difference at the boundary play any role in the U anomalies at the boundary? It doesn't look like it to me - see above https://github.com/COSIMA/mom6-panan/issues/17#issuecomment-1407996382
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The total mass time series is plotted below. It seems to me that there is a slight positive trend, but the variability would be about ~0.1% only. So maybe not strictly mass conserving?
We have a ~1m SSH mismatch with ~4000m mean depth, so it would require a mass change of only about 0.025% for the SSH mismatch to disappear.
Your plot shows an initial very rapid adjustment of 0.018% which is remarkably close to the estimated required value. The subsequent variability and drift is about 0.003%.
So it looks like it's trying to make the SSH match, but for some reason it hasn't adjusted remove the SSH mismatch completely.
Can you please calculate the spatial-mean SSH anomaly? That will let us quantify this more accurately.
The spatial-mean SSH anomaly timeseries would be even better...
Here it is the timeseries for the spatial-mean SSH anomaly (Anomaly referent to the first output). @aekiss
@MatthisAuger Perhaps it would also be useful to compare the global-01-v2 simulation with the panan-01 simulation on the time series of SSH at the boundary. That might tell us if it's just a mismatch of the physics between the mom6 model and the boundary forcing, or whether the boundary forcing is doing something weird.
(The first couple of years of global-01-v2 output are missing, but you could compare for a later time period.)
thanks @willaguiar
So that's pretty confusing - it's hard to see how it's possible for the mass to change by more than the SSH would allow. Is the sea ice growing, and does it depress the ocean surface? Perhaps that might account for some of it.
@adele157 Here is the plot of year 1994 SSH zonal mean time series at the boundary, for boundary forcing, mom6 and panan.
@angus-g said the sea ice initial condition is no ice. So the model would definitely increase the sea ice mass, which presumably reduces the ocean mass. And if sea ice depresses the surface, that would give us a smaller mean SSH change than we'd expect from the ocean mass change, which is the same sign as the inconsistency we're trying to explain.
However if the sea ice is at all realistic, it won't quantitatively explain this little mystery. We need ~4e16 kg of new sea ice to account for the remaining 2/3 in this graph, but the Antarctic sea ice mass in ACCESS-OM2-01 varies seasonally between about 0.3e16 and 1.7e16kg, so that's too little mass, with too much variation, to explain the inconsistency between SSH and ocean mass changes.
Do we have a timeseries of total sea ice volume or mass?
A timeseries of the total mass of ocean salt would also help distinguish between ocean mass loss due to the open boundaries vs sea ice formation & evap-precip-runoff.
seaice.stats
should give you the sea ice stats, and I think includes mass.
A comparison with the global case (which also starts without sea ice in the first year) might be informative.
Just plotted SSH spatial average time series over the first few years of simulation and got a different time series than this one. I find very small variations around 0 and no big changes during spin up. That might come from weighting the mean with the grid cell area?
In that case the SSH average would remain constant and not follow the total mass change?
Currently looking at mass budget and integrated in and out fluxes at the boundary so more figures to come.
Now looking at the open boundary conditions file.
This is the time series of the meridional flux integrated over the whole boundary. Positive is inflow in the model domain and negative is outflow. So it's mostly inflow during the whole year, with the mean meridional transport being 0.24Sv in the model domain.
This second plot is the cumulative meridional transport along the boundary of the model, for day 90 of the open boundary conditions file, with an overall transport of 0.64Sv from the boundary into the model domain.
Hmm, that's odd, because @angus-g and @AndyHoggANU adjusted v at the northern boundary such that the net sum of transport is zero, see /home/157/ahg157/expts/panan/scripts/convert_forcing.py
Do you mean that your new SSH timeseries is area-weighted, and the previous one wasn't?
@aekiss I think so yes. What do you think @willaguiar?
@adele157 I don't have access to the /home/157/ahg157 folder. Was that condition for the boundary conditions file or directly for the northern boundary of the model? My figure comes from V in the obc file but maybe it is not even taken into account in the model.
New transport at the boundary figures:
Transport at the boundary for the OM4 obc file (+ into the model, - out of the model). Again the total transport seems to be about 3.5 Sv into the model on average:
Transport at the frontier of the model (+ into the model, - out of the model). Strong transport out of the model at the beginning of the run, consistent with the ocean mass drop. Then no trend but a positive mean transport into the model.
And same figure I presented last week with total ocean mass and sea ice mass, but with separated plots this time.
Net surface water flux shows a small increasing trend. Need more diagnostics to see where this trend is coming from.
WFO Anom relative to 2000-2060 mean shows positive trend, that is much smaller than the net input from rivers.
P-E should be also be positive (though we are missing the diagnostics to check). The OBC are fluxing mass into the model as well. Everything is increasing the volume of the SO. Where does this water go? How does the model handle a constant increase in volume/mass over time?
Can we close the mass balance in panan, e.g. total mass change = fw surface + boundary? is there a missing process or does the budget make sense? Where does the excess mass go? Does SSH just increase and drive an outflow (into boundary)?
Ask Chris Chapman - John Rielly
Does the SSH increase with the mass? Why not?
From ocean.stats on the panant-01-zstar-v13 experiment: It confirms that the excess of mass goes into sea level. Not sure how this mean sea level is computed though as it is different from the two previous SSH plots obtained with the model output.
Did we figure out if sea ice levitates or not? That could make a difference in different sea level diagnostics.
Order of magnitude of the total mass change budget:
From previous plot: https://github.com/COSIMA/mom6-panan/issues/17#issuecomment-1493550102 Total mass trend after spin up ~2.56 * 10^6 kg/s
From Paul's comment: https://github.com/COSIMA/mom6-panan/issues/17#issuecomment-1471109234 Net surface mass flux ~1.07 * 10^9 kg/s
From meridional transport into the model: https://github.com/COSIMA/mom6-panan/issues/17#issuecomment-1455225906 Mean flux into the model at the boundary (after spin up)= 0.85Sv, ~ 0.87 * 10^9 kg/s
So right now there is way more mass going in than the total mass change. Where does all this mass go?
@adele157 Still not sure if it levitates. Looking at https://github.com/COSIMA/mom6-panan/issues/17#issuecomment-1455226389 I would say yes, as the ocean and sea ice mass seasonal cycles should compensate each other?
This issue has been mentioned on ACCESS Hive Community Forum. There might be relevant details there:
https://forum.access-hive.org.au/t/mom6-regional-modelling-mini-hackathon-may/725/2
re. https://github.com/COSIMA/mom6-panan/issues/17#issuecomment-1493624446, if the mass flux into the model is about 1000x more than the mass change, is there a units error somewhere in the diagnostics or our calculations?
@PaulSpence does Net surface water flux (precip+melt+|runoff+ice calving-evap)
in https://github.com/COSIMA/mom6-panan/issues/17#issuecomment-1471109234 take into account sea ice formation as well as melt, or only sea ice melt?
And does positive sign indicate a flux into the model?
@MatthisAuger re. https://github.com/COSIMA/mom6-panan/issues/17#issuecomment-1493627968, let me see if I understand your argument for seeing the effects of levitation from these ocean & ice mass timeseries https://github.com/COSIMA/mom6-panan/issues/17#issuecomment-1455226389
In a global model, levitation would affect how much the ocean SSH is affected by mass transfer into sea ice:
However things are complicated by the open boundary - in the non-levitating case, would the pressure gradient at the boundary due to a seasonal SSH cycle at the boundary (from to the seasonal sea ice) cause seasonal pumping of mass in/out of the model, reducing the SSH and ocean mass signals? Is that what causes the seasonal cycle in the bottom figure here https://github.com/COSIMA/mom6-panan/issues/17#issuecomment-1455225906? It flows outward in the melt season and inward in the freeze season, which is what is expected from this scenario.
The SSH doesn't show a clear seasonal cycle here https://github.com/COSIMA/mom6-panan/issues/17#issuecomment-1493550102 and and even less in this other SSH diagnostic https://github.com/COSIMA/mom6-panan/issues/17#issuecomment-1437844709 (it's odd that these look so different - do we know why?) and the seasonal cycle in ocean mass is much weaker than in sea ice mass https://github.com/COSIMA/mom6-panan/issues/17#issuecomment-1455226389 so that is consistent with mass transfer to sea ice being compensated by inflow at the open boundary. Presumably there is enough of a seasonal cycle in SSH at the open boundary to drive these compensating flows.
So if this scenario is correct, while the fairly non-seasonal SSH timeseries might look like evidence for non-levitating, it is actually also inconsistent with levitating ice with seasonal boundary inflow/outflow. Does that sound right?
Of course to settle the levitation question, we should look at the model parameters. In MOM5 this is controlled by max_ice_thickness
- does anyone know the equivalent in MOM6? There's DEPRESS_INITIAL_SURFACE
and TRIM_IC_FOR_P_SURF
, but from a quick glance they seem to be intended for setting up initial conditions with ice shelves, rather than adjustments with sea ice changes during a model run. But I could be wrong. They both default to false anyway.
Are we using a Boussinesq formulation? If so, that will conserve volume rather than mass (but of course the difference will be way too small to explain our factor of 1000 mismatch).
This issue has been mentioned on ACCESS Hive Community Forum. There might be relevant details there:
https://forum.access-hive.org.au/t/mom6-regional-modelling-mini-hackathon-may/725/4
Last week we discussed the processes at the model frontier and how the model was behaving with boundary conditions. It seems like they are not the candidates for the large jump and trends between the models anymore, but it might be still interesting to look at what is happening there.
I made a few videos, looking at the bottom layer of Temperature, Salinity, U, and V outputs from the hycom1 model and boundary conditions. This is focused on the bottom layer as initially the interest was on the lower overturning cell, but I can make these videos in any other layer or region if needed.
Here are all the parameters along the boundary over longitudes 50W-10W. These are the outputs over the first few months of the model, boundary conditions, and differences between outputs and boundary conditions.
https://user-images.githubusercontent.com/68908668/212576484-8d820569-b8e9-4e81-af0b-e6a70f6d1ecd.mp4
Same thing but across the boundary this time, at longitude 70E if I remember correctly.
https://user-images.githubusercontent.com/68908668/212576858-1dba86a5-2a4f-4624-857c-b131f959ebd6.mp4
For both videos, T and S do not vary a lot as it is the bottom layer, but U outputs seem to go a bit crazy compared to boundary conditions. As I said just tell me if you are interested in similar plots for other regions or layers. I can make those closer to the surface if you want to see how the model reacts to stronger changes in boundary conditions temperature or salinity.