- xwiki:Main.WebHome
- Phase2
- Stratosphere Sub-Project
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 | - |
|
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 | \\ |
79 | + | |
80 | +(% style="position: absolute; left: 537px; top: 257px; width: 1px; height: 1px; overflow: hidden;" %) | |
81 | +((( | |
82 | +(% class="MsoNormal" style="margin-bottom: 0px; color: rgb(34, 34, 34); font-family: Arial, Helvetica, sans-serif; font-size: small;" %) | |
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"]] | |
84 | + | |
85 | +(% class="MsoNormal" style="margin-bottom: 0px; color: rgb(34, 34, 34); font-family: Arial, Helvetica, sans-serif; font-size: small;" %) | |
86 | + | |
87 | +))) | |
88 | + | |
89 | +(% style="position: absolute; left: 537px; top: 257px; width: 1px; height: 1px; overflow: hidden;" %) | |
90 | +((( | |
91 | +(% class="MsoNormal" style="margin-bottom: 0px; color: rgb(34, 34, 34); font-family: Arial, Helvetica, sans-serif; font-size: small;" %) | |
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"]] | |
93 | + | |
94 | +(% class="MsoNormal" style="margin-bottom: 0px; color: rgb(34, 34, 34); font-family: Arial, Helvetica, sans-serif; font-size: small;" %) | |
95 | + | |
96 | +))) | |
97 | + | |
98 | +(% style="position: absolute; left: 537px; top: 257px; width: 1px; height: 1px; overflow: hidden;" %) | |
99 | +((( | |
100 | +(% class="MsoNormal" style="margin-bottom: 0px; color: rgb(34, 34, 34); font-family: Arial, Helvetica, sans-serif; font-size: small;" %) | |
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"]] | |
102 | + | |
103 | +(% class="MsoNormal" style="margin-bottom: 0px; color: rgb(34, 34, 34); font-family: Arial, Helvetica, sans-serif; font-size: small;" %) | |
104 | + | |
105 | +))) | |
106 | + | |
107 | +(% style="position: absolute; left: 537px; top: 257px; width: 1px; height: 1px; overflow: hidden;" %) | |
108 | +((( | |
109 | +(% class="MsoNormal" style="margin-bottom: 0px; color: rgb(34, 34, 34); font-family: Arial, Helvetica, sans-serif; font-size: small;" %) | |
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"]] | |
111 | + | |
112 | +(% class="MsoNormal" style="margin-bottom: 0px; color: rgb(34, 34, 34); font-family: Arial, Helvetica, sans-serif; font-size: small;" %) | |
113 | + | |
114 | +))) |