Assessment of ENSO and other variability in 104 #8
Replies: 7 comments 9 replies
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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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@phillips-ad @swrneale here's a place to discuss ENSO skill and other aspects of variability in the new runs
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