Assessment of ENSO and other variability in 104 #8
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The easiest thing to do first is for me to add a ridiculous screenshot that @megandevlan and I looked at for the evolution of ENSO between 98 and 109. Bottom line it's complicated and data insufficient, but promising! |
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Another metric, this is looking at the correlation of SST anomalies and the Nino 3.4 index within the Nino 3.4 box at various lag//lead times. It looks like 104 B1850 (peach dashed line) and the historical run (red dashed line) are two of the better performing simulations. Still showing somewhat of a too-regular ENSO pattern with elevated correlations well ahead of and after ENSO events, but certainly an improvement on other simulations. |
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Looking at 104 in the CVDP, there were a couple metrics that gave me pause. First, the standard deviation of SST in the Tropical Pacific for DJF: compared to that seen in 99 and obs: I haven't seen such limited variability in the tropical Pacific SSTs in any prior CESM3 run. Here is a histogram of the nino3.4 standard deviations by month for 104LT/MT (observational estimates = orange lines): compared to those from 92/98/99 (and earlier CESM3 runs): |
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I also have concerns about the CESM3 simulated patterns of ENSO teleconnections and attach a related figure below. The top two panels are CESM3 (98b). The mid left is GPCP, right is CESM2. The bottom ones are CESM3 biases versus each. Note the weakness of the NH ITCZ bias in the eastern Pacific and the strength in the SH. I see the same issue for radiative flues and across all members of CESM3. I suspect the issue is related to the equatorial dry zone bias. |
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The nino3.4 autocorrelation looks better w/112 (upper right panel) compared to the 104 variants (2nd row), and looks more similar to the CESM2-piControl (bottom 2 rows): The Tropical Pacific variability looks better in 112 as well: The ENSO teleconnections are also slightly improved, and the Tropical Pacific dry slot has also improved slightly. Good news! |
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Great point - for all metrics it helps to provide some range of uncertainty against the CESM2 LE when possible. ENSO in particular has considerable internal noise. |
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Given that in the past we had seen issues with the upper tropospheric westerlies in the Pacific sector, I had been meaning to check what that's currently looking like since it could impact ENSO teleconnections. Happy to report it looks good! No problems there. |
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SST anomaly variance in the Nino 3.4 region is more reasonable in 121; the monthly max is still a little low, but better than 116/118. |
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These are good and are the kinds of things we would like to review at the
next CESM Project Meeting.
…On Thu, Jan 9, 2025 at 9:24 AM Meg Fowler ***@***.***> wrote:
SST anomaly variance in the Nino 3.4 region is more reasonable in 121; the
monthly max is still a little low, but better than 116/118.
image.png (view on web)
<https://github.com/user-attachments/assets/4d733578-8399-4585-8b3e-d47454847517>
But the period of ENSO looks to be *really* long in 121.
Screenshot.2025-01-09.at.9.24.21.AM.png (view on web)
<https://github.com/user-attachments/assets/5dd19943-4589-4201-9de7-d928fac69fef>
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Adam has the CVDP diagnostics here too: https://webext.cgd.ucar.edu/BLT1850/b.e30_beta04.BLT1850.ne30_t232_wgx3.121/cvdp/. I don't have any more to say about these at this point, beyond what Meg's already said above. ENSO variance is improved, there may be too much in the spring but time will tell, and period seems long. |
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I have run two 121 time periods through the CVDP, years 20-156 and 60-156, with results here. For most of the plots, note the full 121 time period is in the upper right, while the shorter 60-156 time period is the first plot in the second row. The last 6 plots are time slices from the CESM2-picontrol. I do not see much of a difference at all between the 121 metrics for years 20-156 and those for years 60-156. Overall, 121 seems to be a positive step forward. ENSO teleconnections, nino3.4 spectra and hovmollers, sst standard deviations in the tropics and the tropical pacific dry slot are all improved and/or near the best seen in the 1XX series of runs. 121's La Nina Hovmoller plot shows a particular improvement with capturing a 2nd year La Nina which is great to see. |
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Also in reference to the CAM7 meeting today where there were questions about when certain ENSO biases appeared in the development cycle: I created a slide for a CAS meeting back in November where I tried to look back on the timings of things: |
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A group of us discussed yesterday the possibility of using initialized predictions of 1997/1998 to explore the issue of the long decorrelation timescale of Nino3.4. I'm thinking we should maybe pause on this plan. I've been looking at how this particular metric evolves over the 121 historical simulation. Firstly, below is a comparison of the Nino3.4 autocorrelation between the 121 simulations and the historical simulations from CMIP6 and LENS2. For observations I'm using 1854-2024, for LENS2 I'm using 1920-2024, for the 121 simulations I'm using the full length of the simulation. There are indications from this that the historical is closer to the observations than the piControl.
In the process of making this plot, I noticed that the historical got even closer to the observations if I used a more recent time period. So, what I'm plotting below is the month at which the lagged autocorrelation crosses zero for 50 year running segments for the 121 simulations and observations. From this we can see that the nino3.4 autocorrelation systematically evolves over the historical simulation to become more like observations. Observations don't show that same evolution, so I don't think this is a real global warming signal that we should be having in the model. But something over the historical simulation is kicking it into being more like observations. At some point, someone mentioned that maybe it's a problem resulting from the model being too cold. Seems like this would fit with that hypothesis. Also @gustavo-marques I wonder if it's worth checking how the salinity bias you mentioned is evolving over the historical simulation.
But overall, I'm not convinced that an initialized 1997/1998 prediction is going to help us with this problem now. |
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I agree with @islasimpson here. Separately, I wanted to share this result from GFDL, who are in the process tuning up ENSO in CM5. Below shows that reducing the entrainment rate in their deep convection scheme (rkm_dp1 = 0.9->0.5) increases the amplitude of the teleconnections (regression of Nino3.4 on Z500). This may be something to consider. |
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Adding onto @islasimpson's suggestion that it's the cold bias driving too long of an ENSO period, there's some support in the 1850 runs for this (though I've excluded run 91 as an outlier) - scatter plot of mean equatorial Pacific SST vs. month of transition in the autocorrelation plots: |
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I split 121's BLTHIST run into three time periods (1850-1939, 1940-2012 and 1850-2012) and compared them against CESM2-LENS in a new CVDP comparison. Notable results:
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Adding onto @phillips-ad comments above, I used years 1940-2012 for 121_hist in the plots below. 121_4xco2 is cut to be years 50-152.
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These a really interesting. Given Adam's composite hovmollers and that most of the lack of transition to La Nina is away from the East Pacific, I'm wondering @megandevlan could you repeat the autocorrelation, but for the nino4, nino3 and even nino1+2 regions separately? |
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I have created a CVDP comparison using the following simulations and time slices:
The comparison is here: A few items are notable:
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I see a fairly dramatic difference in ENSO teleconnections between 234pi and 235pi - with 234 being the better performer. See for example the ENSO PSL teleconnections in CMAT |
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The most recent versions of CESM3 continue to score well in CMAT. #245 shows some of the best overall scores on record. |
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The newer versions of the model continue to score well in CMAT. Here a number of runs are sorted by overall score. |
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@phillips-ad @swrneale here's a place to discuss ENSO skill and other aspects of variability in the new runs
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