Conversation
durack1
left a comment
There was a problem hiding this comment.
Nice @znichollscr centralising all this info in one place makes sense to me, and pulls (or at least duplicates) info out of inboxes - as my llnl.gov email is now dead, I have no personal track of these comms that occurred via email in CMIP6, only my version tracking in the CMIP6 Forcing Datasets Summary
|
2026-01-17 update Historical forcingsCMIP7 datasets for AR7 Fast Track CMIP6Plus testing datasets For further details on the CMIP DECK forcing suite please see the CMIP Forcings Task Team webpage, the recent open community drop-in session slides and recording, and the input4MIPs documentation repository (https://input4mips-cvs.readthedocs.io/en/latest/dataset-overviews/) PLEASE NOTE: All CMIP6Plus era data sets are for testing purposes only, i.e. they are not to be relied upon for CMIP7 production runs. Scenarios and harmonisationWe anticipate some scenario forcings datasets may be available for testing as early as April 2025 with others expected by October 2025. With the ScenarioMIP description manuscript now out for review, we anticipate final scenario forcing datasets to be available once the ScenarioMIP team has finalized the protocol and the participating socioeconomic modelling teams (i.e. Integrated Assessment Models, or IAMs) have produced scenarios in line with this protocol. The Forcings Task Team is working on establishing a firmer timeline for the scenario forcing delivery and is at the final stages of planning for the harmonisation, which is part of providing scenario forcings. |
|
2025-01-31 update Update on CMIP6Plus stratospheric aerosol optical property and volcanic sulfur emission datasetsVersion 1.3.0 of the CMIP6Plus stratospheric aerosol optical property and volcanic sulfur emission datasets are now available on ESGF with succinct documentation available here. A key development in this version is the addition of small-magnitude volcanic eruption pre-satellite era, addressing an important bias in previous versions. This development means that the piControl climatology for stratospheric aerosol optical properties should be very stable from now on, and that if you start spinning up your model with this version, we expect minor effects when you implement future updates, including the final version that will be frozen for use in the AR7 Fast Track at the end of February. We encourage users to test the available datasets and provide feedback via the input4MIPs_CVs repository discussions on GitHub. |
|
2025-03-27 update The CMIP Forcings Task Team would like to provide an update on the availability of CMIP7 forcings datasets:
|
|
2025-04-15 update IMPORTANT: Errors in Table 1 of Dunne et al, 2025We are aware that some of you are already following the An evolving Coupled Model Intercomparison Project phase 7 (CMIP7) and Fast Track in support of future climate assessment preprint Table 1. Some errors have been found regarding the volcanic and solar forcing entries, which will be corrected for final submission, and are highlighted in bold below:
The CMIP Panel, WIP and relevant TTs are working on a dynamic format for the experiment specifications to ensure everyone can access the most up to date information rather than referring to a static paper going forwards. In the meantime, for forcings information and descriptions, we strongly recommend referring to the information/documentation found at https://wcrp-cmip.org/cmip-phases/cmip7/cmip7-forcing-datasets/ linking to the dataset overviews at https://input4mips-cvs.readthedocs.io/en/latest/dataset-overviews/ |
|
2025-10-14 update All CMIP7 DECK historical forcings now available!The CMIP Forcings Task Team would like to make you all aware that the full set of CMIP7 DECK historical forcings are now available and can be accessed here and below:
Please continue to ask questions and engage in discussions at the input4MIPs Github discussions and find all information relevant to CMIP7 Forcing datasets at https://wcrp-cmip.org/cmip-phases/cmip7/cmip7-forcing-datasets/ The TT is now working hard on delivering draft and final versions of the scenario forcings and will keep you regularly updated on the progress. |
|
2025-10-17 update Request for feedback on Scenario Emission test datasetsThe testing data for scenario emissions is now on ESGF and available at https://input4mips-cvs.readthedocs.io/en/latest/dataset-overviews/anthropogenic-slcf-co2-emissions/#scenariomip. In order to deliver the final product as soon as possible it is important that the team receives any feedback on the data within the next 1-2 weeks. A Github issue has been set up at #386 to signpost the data and gather feedback from you all. Based on this feedback, the team will revise the data as much as needed to deliver a final product before the end of October. Feedback received after this time will not be integrated into the final product. Contact: Jarmo Kikstra kikstra@iiasa.ac.at CMIP7 stratospheric aerosol paper in open peer reviewThe first documentation paper from the volcanic emissions team documenting the optical property dataset is now open for peer review at https://egusphere.copernicus.org/preprints/2025/egusphere-2025-4990/ and the team welcomes community feedback. |
|
2025-10-29 update CMIP7 DECK historical forcingsThe full set of CMIP7 DECK historical forcings are now available and can be accessed here and below:
Please continue to ask questions and engage in discussions at the input4MIPs Github discussions and find all information relevant to CMIP7 Forcing datasets at https://wcrp-cmip.org/cmip-phases/cmip7/cmip7-forcing-datasets/ CMIP7 scenarios update and forcings developmentScenarios update CMIP7 Scenario forcing development A small number of the scenario forcings (land use, ozone and nitrogen deposition) cannot produce all seven scenarios at the same time. Therefore, a scenario running order has been developed in close collaboration with ScenarioMIP and downstream activities such as ISIMIP, ISMIP7 and CORDEX, who require scenario data by July 2026 to facilitate their contribution to AR7. As outlined in Dunne et al. (2025) the CMIP Panel strongly encourages modelling centres to follow a running order, first running the H and VL scenario simulations, for which scenario forcings will be delivered by January 2026. Within the survey, accompanying this update, we are requesting feedback to support further guidance on the running order of the remaining scenarios up to 2100 and extensions out to 2300/2500.
Note: H and VL will be made available first to allow the |
|
@znicholls that is all the updates added pending one this week |
The table in this update isn't formatting correctly (specifically the bold isn't showing). Do we care? |
|
2026-02-12 update CMIP7 forcings: modelling centres’ updateDate issued: 12 February 2026 This update provides the status of the delivery of the CMIP7 forcing datasets including an important notification on the historical ozone (v1.2) dataset. The homepage for CMIP7 Forcings datasets can be found here. Request for feedback IMPORTANT: Updated dataset to address discontinuity between the PI control climatology and the historical ozone The ozone forcing providers have uploaded an updated version (v2.0) of the historical ozone concentrations to correct for the discontinuity in v1.2. The new historical ozone forcing v2.0, which can be found at this link, has an increased historical ozone burden of about 10% (primarily due to a vertical shift in the stratospheric ozone distribution). The CMIP Panel co-chairs are recommending that, for modelling centres who rely on ozone as an external forcing, piControl, historical, and other relevant DECK (e.g., AMIP), simulations should be re-run with the v2.0 ozone if possible. For the piControl simulation, the 1850-1870 mean of v2.0 should be used (no specific piControl file will be produced for v2.0). However, it is preferable for a new historical simulation to be run with v2.0, if possible, and in advance of starting scenario simulations. If any modelling centres cannot re-run their historical simulations, they should contact the ozone forcing providers for guidance on use of future scenario ozone forcing files. If any modelling centres run historical simulations with both v1.2 and v2.0 forcing, these simulations would be of interest to the Forcings Task Team. Available CMIP7 scenario forcing datasets (1) Anthropogenic short-lived climate forcer (SLCF) and CO2 emissions: IIASA-IAMC-vl-1-0-0; IIASA-IAMC-h-1-0-0 (DOI: 10.5281/zenodo.17981825.) (2) Open biomass burning emissions: IIASA-IAMC-vl-1-0-0; IIASA-IAMC-h-1-0-0 (DOI: 10.5281/zenodo.17981825.) (4) Greenhouse gas concentrations: CR-vl-1-0-0; CR-h-1-0-0 (DOI: No DOI provided.) (6) Stratospheric volcanic SO2 emissions and aerosol optical properties: UOEXETER-ScenarioMIP-2-2-2 (No DOI provided) PLEASE NOTE: Version 2.2.1 of the ScenarioMIP stratospheric aerosol optical properties has been updated to version 2.2.2 to fix an issue with the tropospheric mask. This issue resulted in a ~10% discrepancy between pre-industrial and ScenarioMIP stratospheric aerosol optical depth. Version 2.2.1 has been deprecated and version 2.2.2 (accessible here) should be used for ScenarioMIP runs. This only applies to ScenarioMIP files, stratospheric aerosol optical properties for DECK simulations are unchanged (version 2.2.1). (9) Solar: SOLARIS-HEPPA-ScenarioMIP-4-6 (No DOI provided) (12) Population density: PIK-vl-1-0-0; PIK-ln-1-0-0; PIK-l-1-0-0; PIK-ml-1-0-0; PIK-m-1-0-0; PIK-hl-1-0-0; PIK-h-1-0-0 (No DOI provided) Please note that the van Vuuren et al. (2025) paper has been resubmitted with updates to two scenario names (VLLO becomes VL and VLHO becomes LN) plus a new scenario (HL). The updated table can be found at https://wcrp-cmip.org/mips/scenariomip/ and below. The updated or new scenarios are highlighted in bold.
Following the H and VL scenario forcings delivery, the CMIP Panel has decided that M and HL will be next in the running order. Status of outstanding datasets Ozone concentrations and nitrogen deposition Aerosol optical properties/MACv2-SP Future extensions Impact of delays on downstream activities Where to ask questions and raise issues about the forcing datasets |
|
@znicholls have added today's update above and fixed the bolding in 2025-04-15 update |
|
No changes to the database between 'main' branch and 565950e |
|
No changes to the database between 'main' branch and f120409 |
|
2026-02-16 update Further to the update circulated on 12 February, there has been an iteration on the recommendation for piControl as follows: Recommendation for pre-industrial controlThe piControl forcing should come from files with the source ID FZJ-CMIP-ozone-1-2 data, (there are no specific piControl files available in the FZJ-CMIP-ozone-2-0 data). Note that this guidance differs from the email communication sent by the CMIP IPO on 12 February 2026. For pre-industrial control, there are two options. The first is the monthly climatology file (frequency value of monC). This dataset averages over a longer simulation, essentially removing variability like the QBO. If you wish to use this forcing for your piControl, simply apply it on repeat. The second is a transient file which has a time range equal to 182901-184912 in the filename. This file is found in the same directory as the historical forcing so please be careful to only use it for piControl and do not include it in historical forcing. This transient piControl forcing includes the QBO signal but uses average solar forcing and repeating 1850 emissions. If you wish to use this forcing for your piControl, simply apply it on repeat. For full details on the ozone dataset please see Ozone concentrations - input4MIPs Controlled Vocabularies (CVs) |
|
No changes to the database between 'main' branch and 4e631db |
|
No changes to the database between 'main' branch and 2908684 |
|
No changes to the database between 'main' branch and 6b1214c |
|
2026-02-24 update The land use forcing data for the H and VL scenarios are now available – please see details at https://input4mips-cvs.readthedocs.io/en/latest/dataset-overviews/land-use/#cmip7_1 and direct links below If you find an issue, please create an issue on GitHub so that the identification and resolution of this issue is publicly accessible. Thank you to the dataset providers, Louise Chini and George Hurtt, for all their efforts. |
Description
Checklist
Please confirm that this pull request has done the following:
Data released on ESGFN/AESGF update pulled in hereN/Achangelog/