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Changes for document Stratosphere Sub-Project
From version 16.1
edited by s2s_wiki
on 2021/04/25 23:06
on 2021/04/25 23:06
To version 17.1
edited by s2s_wiki
on 2022/04/08 04:24
on 2022/04/08 04:24
Change comment: added URLs for the under review papers (SNAPSI protocol and first biases paper)
Content changes
| ... | ... | @@ -34,9 +34,13 @@ |
| 34 | 34 | d. Are biases linked to stratospheric processes/variability? E.g., are biases larger before or after SSWs, vortex intensifications, phases of the QBO, etc? |
| 35 | 35 | |
| 36 | 36 | |
| 37 | - These efforts are being led by Zachary Lawrence. The |
|
| 37 | + These efforts are being led by Zachary Lawrence. The first paper is under review, and can be found at | |
| 38 | 38 | |
| 39 | +https:~/~/wcd.copernicus.org/preprints/wcd-2022-12/ | |
| 39 | 39 | |
| 41 | +A second community paper will be submitted in 2022. If you would like to join these efforts, please contact the SNAP co-chairs (Amy Butler, NOAA and Chaim Garfinkel, Hebrew University) or Zachary Lawrence. | |
| 42 | + | |
| 43 | + | |
| 40 | 40 | **Upcoming Activities: |
| 41 | 41 | __S__tratospheric __N__udging __A__nd __P__redictable __S__urface __I__mpacts (SNAPSI - **experiments for operational centres to perform that isolate the role of the stratosphere on predictive skill) |
| 42 | 42 | |
| ... | ... | @@ -56,19 +56,55 @@ |
| 56 | 56 | |
| 57 | 57 | The basic experimental protocol consists of a set of forecast ensembles: (1) a standard, free running forecast ensemble, (2) a 'perfect stratosphere' forecast in which the stratosphere is relaxed towards the observed evolution, and (3) a 'control' forecast in which the stratosphere is relaxed towards climatology. Further details of the experimental protocol will be described in an article soon to be submitted to a peer-reviewed journal. To date, twelve modeling groups at eleven centers are planning to contribute integrations following this protocol. This will allow for an unprecedented, multi-model comparison of the dynamics underlying the surface responses to sudden stratospheric warmings. Moreover, by including 'counterfactual' forecasts in which the stratospheric circulation remains in a climatological state, the experimental protocol will allow for formal attribution statements to be made regarding the surface extremes that followed the stratospheric anomalies. |
| 58 | 58 | |
| 59 | - |
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| 63 | +The paper documenting the Experiment Protocol for damping experiments is under review: | |
| 60 | 60 | |
| 65 | +https:~/~/gmd.copernicus.org/preprints/gmd-2021-394/ | |
| 61 | 61 | |
| 67 | + | |
| 62 | 62 | We have already held very fruitful discussions with QBOi and SATIO-TCS about a joint initiative that would explore stratosphere-troposphere coupling in the tropics using these same experiments, in addition to the four aforementioned goals. A rough timeline is: |
| 63 | 63 | |
| 64 | -Q2 2021 – submission of paper outlining experimental protocol (with input from modelling centres) | |
| 65 | -Q2 2021 – begin modelling experiments | |
| 66 | -Q4 2021 – completion of modelling experiments and transfer of detailed dynamical diagnostics to a shared, open data repository | |
| 67 | -Q1-Q3 2022 – analysis of damped runs and production of ~~4 papers on outcomes | |
| 70 | +Q3 2022 – completion of modelling experiments and transfer of detailed dynamical diagnostics to a shared, open data repository | |
| 71 | +Q3 2022-Q2 2023 – analysis of damped runs and production of ~~4 papers on outcomes | |
| 68 | 68 | |
| 69 | -Anyone interested in participating in the analysis for the 4 community papers is encouraged to contact Peter Hitchcock (aph28@cornell.edu). The data embargo for the broader community will be lifted in |
|
| 73 | +Anyone interested in participating in the analysis for the 4 community papers is encouraged to contact Peter Hitchcock (aph28@cornell.edu). The data embargo for the broader community will tentatively be lifted in 2023. | |
| 70 | 70 | |
| 71 | 71 | |
| 72 | 72 | |
| 73 | 73 | |
| 74 | 74 | \\ |
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| 83 | + [[https:~~/~~/gmd.copernicus.org/preprints/gmd-2021-394/>>url:https://gmd.copernicus.org/preprints/gmd-2021-394/||style="color: rgb(17, 85, 204);" target="_blank"]] | |
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| 92 | + [[https:~~/~~/gmd.copernicus.org/preprints/gmd-2021-394/>>url:https://gmd.copernicus.org/preprints/gmd-2021-394/||style="color: rgb(17, 85, 204);" target="_blank"]] | |
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| 101 | + [[https:~~/~~/gmd.copernicus.org/preprints/gmd-2021-394/>>url:https://gmd.copernicus.org/preprints/gmd-2021-394/||style="color: rgb(17, 85, 204);" target="_blank"]] | |
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| 110 | + [[https:~~/~~/gmd.copernicus.org/preprints/gmd-2021-394/>>url:https://gmd.copernicus.org/preprints/gmd-2021-394/||style="color: rgb(17, 85, 204);" target="_blank"]] | |
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