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| 1 | +# 2026-02-12 update |
| 2 | + |
| 3 | +## CMIP7 forcings: modelling centres’ update |
| 4 | + |
| 5 | +This update provides the status of the delivery of the CMIP7 forcing datasets including an important notification on the historical ozone (v1.2) dataset. |
| 6 | +The homepage for CMIP7 Forcings datasets can be found [here](https://wcrp-cmip.org/cmip-phases/cmip7/cmip7-forcing-datasets/). |
| 7 | + |
| 8 | +**Request for feedback** |
| 9 | + |
| 10 | +Given the update on the error in v1.2 historical ozone dataset and scenario forcing data availability below, |
| 11 | +we would ask modelling centres to provide feedback by completing [this form](https://airtable.com/applbQctZtl09L2Ga/pagKlDzoY8Fd0KCLL/form). |
| 12 | + |
| 13 | +**IMPORTANT: Updated dataset to address discontinuity between the PI control climatology and the historical ozone** |
| 14 | + |
| 15 | +A member of the community raised an issue with a discontinuity between the piControl climatology and the historical ozone. |
| 16 | +The full discussion is at https://github.com/PCMDI/input4MIPs_CVs/issues/400 |
| 17 | + |
| 18 | +The ozone forcing providers have uploaded an updated version (v2.0) of the historical ozone concentrations to correct for the discontinuity in v1.2. |
| 19 | +The new historical ozone forcing v2.0, which can be found at [this link](https://esgf-node.ornl.gov/search?project=input4MIPs&activeFacets=%7B%22mip_era%22%3A%22CMIP7%22%2C%22institution_id%22%3A%22FZJ%22%2C%22source_version%22%3A%222.0%22%7D), |
| 20 | +has an increased historical ozone burden of about 10% (primarily due to a vertical shift in the stratospheric ozone distribution). |
| 21 | + |
| 22 | +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), |
| 23 | +simulations should be re-run with the v2.0 ozone if possible. |
| 24 | +For the piControl simulation, the 1850-1870 mean of v2.0 should be used (no specific piControl file will be produced for v2.0). |
| 25 | +For those modellers who are not be able to repeat the piControl simulations, |
| 26 | +using the v1.2 PI climatology or the 1829-1849 20251025 v1.2 data is fine, since it is expected to be close to the 1850-1870 mean of v2.0. |
| 27 | + |
| 28 | +However, it is preferable for a new historical simulation to be run with v2.0, if possible, |
| 29 | +and in advance of starting scenario simulations. |
| 30 | +If any modelling centres cannot re-run their historical simulations, |
| 31 | +they should contact the ozone forcing providers for guidance on use of future scenario ozone forcing files. |
| 32 | + |
| 33 | +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. |
| 34 | + |
| 35 | +**Available CMIP7 scenario forcing datasets** |
| 36 | + |
| 37 | +To access the summary of CMIP7 ScenarioMIP datasets click [here](https://input4mips-cvs.readthedocs.io/en/latest/dataset-overviews/#cmip7_1). |
| 38 | +The following scenario forcing datasets for the High (H) and Very Low (VL) scenarios are finalised and are now available: |
| 39 | + |
| 40 | +(1) Anthropogenic short-lived climate forcer (SLCF) and CO2 emissions: [IIASA-IAMC-vl-1-0-0](https://esgf-node.ornl.gov/search?project=input4MIPs&activeFacets=%7B%22mip_era%22%3A%22CMIP7%22%2C%22institution_id%22%3A%22IIASA-IAMC%22%2C%22source_version%22%3A%221.0.0%22%2C%22target_mip_list%22%3A%22ScenarioMIP%22%2C%22source_id%22%3A%22IIASA-IAMC-vl-1-0-0%22%7D); IIASA-IAMC-h-1-0-0 (DOI: [10.5281/zenodo.17981825](https://doi.org/10.5281/zenodo.17981825).) |
| 41 | + |
| 42 | +(2) Open biomass burning emissions: [IIASA-IAMC-vl-1-0-0](https://esgf-node.ornl.gov/search?project=input4MIPs&activeFacets=%7B%22mip_era%22%3A%22CMIP7%22%2C%22institution_id%22%3A%22IIASA-IAMC%22%2C%22source_version%22%3A%221.0.0%22%2C%22target_mip_list%22%3A%22ScenarioMIP%22%2C%22source_id%22%3A%22IIASA-IAMC-vl-1-0-0%22%7D); IIASA-IAMC-h-1-0-0 (DOI: [10.5281/zenodo.17981825](https://doi.org/10.5281/zenodo.17981825).) |
| 43 | + |
| 44 | +(4) Greenhouse gas concentrations: [CR-vl-1-0-0](https://esgf-node.ornl.gov/search?project=input4MIPs&activeFacets=%7B%22mip_era%22%3A%22CMIP7%22%2C%22target_mip_list%22%3A%22ScenarioMIP%22%2C%22institution_id%22%3A%22CR%22%2C%22source_version%22%3A%221.0.0%22%2C%22source_id%22%3A%22CR-vl-1-0-0%22%7D); CR-h-1-0-0 (DOI: [No DOI provided](https://doi.org/dev-test).) |
| 45 | + |
| 46 | +(6) Stratospheric volcanic SO2 emissions and aerosol optical properties: [UOEXETER-ScenarioMIP-2-2-2](https://esgf-node.ornl.gov/search?project=input4MIPs&activeFacets=%7B%22mip_era%22%3A%22CMIP7%22%2C%22target_mip_list%22%3A%22ScenarioMIP%22%2C%22institution_id%22%3A%22uoexeter%22%2C%22source_version%22%3A%222.2.2%22%2C%22source_id%22%3A%22UOEXETER-ScenarioMIP-2-2-2%22%7D) (No DOI provided) |
| 47 | + |
| 48 | +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](https://eur05.safelinks.protection.outlook.com/?url=https%3A%2F%2Faims2.llnl.gov%2Fsearch%3Fproject%3Dinput4MIPs%26versionType%3Dall%26activeFacets%3D%257B%2522source_id%2522%253A%2522UOEXETER-ScenarioMIP-2-2-2%2522%257D&data=05%7C02%7CEleanor.ORourke%40ext.esa.int%7C8e629563147841a4a17908de539c0630%7C9a5cacd02bef4dd7ac5c7ebe1f54f495%7C0%7C0%7C639040126755937301%7CUnknown%7CTWFpbGZsb3d8eyJFbXB0eU1hcGkiOnRydWUsIlYiOiIwLjAuMDAwMCIsIlAiOiJXaW4zMiIsIkFOIjoiTWFpbCIsIldUIjoyfQ%3D%3D%7C0%7C%7C%7C&sdata=zkRCokoVmfaEVjlr4J28Jda6gcwCRtn%2BN8CJjJXk7T0%3D&reserved=0)) 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). |
| 49 | + |
| 50 | +(9) Solar: [SOLARIS-HEPPA-ScenarioMIP-4-6](https://esgf-node.ornl.gov/search?project=input4MIPs&activeFacets=%7B%22mip_era%22%3A%22CMIP7%22%2C%22target_mip_list%22%3A%22ScenarioMIP%22%2C%22institution_id%22%3A%22SOLARIS-HEPPA%22%2C%22source_version%22%3A%224.6%22%2C%22source_id%22%3A%22SOLARIS-HEPPA-ScenarioMIP-4-6%22%7D) (No DOI provided) |
| 51 | + |
| 52 | +(12) Population density: [PIK-vl-1-0-0](https://esgf-node.ornl.gov/search?project=input4MIPs&activeFacets=%7B%22mip_era%22%3A%22CMIP7%22%2C%22target_mip_list%22%3A%22ScenarioMIP%22%2C%22institution_id%22%3A%22PIK%22%2C%22source_version%22%3A%221.0.0%22%2C%22source_id%22%3A%22PIK-vl-1-0-0%22%7D); [PIK-ln-1-0-0](https://esgf-node.ornl.gov/search?project=input4MIPs&activeFacets=%7B%22mip_era%22%3A%22CMIP7%22%2C%22target_mip_list%22%3A%22ScenarioMIP%22%2C%22institution_id%22%3A%22PIK%22%2C%22source_version%22%3A%221.0.0%22%2C%22source_id%22%3A%22PIK-ln-1-0-0%22%7D); [PIK-l-1-0-0](https://esgf-node.ornl.gov/search?project=input4MIPs&activeFacets=%7B%22mip_era%22%3A%22CMIP7%22%2C%22target_mip_list%22%3A%22ScenarioMIP%22%2C%22institution_id%22%3A%22PIK%22%2C%22source_version%22%3A%221.0.0%22%2C%22source_id%22%3A%22PIK-l-1-0-0%22%7D); [PIK-ml-1-0-0](https://esgf-node.ornl.gov/search?project=input4MIPs&activeFacets=%7B%22mip_era%22%3A%22CMIP7%22%2C%22target_mip_list%22%3A%22ScenarioMIP%22%2C%22institution_id%22%3A%22PIK%22%2C%22source_version%22%3A%221.0.0%22%2C%22source_id%22%3A%22PIK-ml-1-0-0%22%7D); [PIK-m-1-0-0](https://esgf-node.ornl.gov/search?project=input4MIPs&activeFacets=%7B%22mip_era%22%3A%22CMIP7%22%2C%22target_mip_list%22%3A%22ScenarioMIP%22%2C%22institution_id%22%3A%22PIK%22%2C%22source_version%22%3A%221.0.0%22%2C%22source_id%22%3A%22PIK-m-1-0-0%22%7D); PIK-[hl-1-0-0](https://esgf-node.ornl.gov/search?project=input4MIPs&activeFacets=%7B%22mip_era%22%3A%22CMIP7%22%2C%22target_mip_list%22%3A%22ScenarioMIP%22%2C%22institution_id%22%3A%22PIK%22%2C%22source_version%22%3A%221.0.0%22%2C%22source_id%22%3A%22PIK-hl-1-0-0%22%7D); PIK-h-1-0-0 (No DOI provided) |
| 53 | + |
| 54 | +Please note that the [van Vuuren et al. (2025) paper](https://egusphere.copernicus.org/preprints/2025/egusphere-2024-3765/egusphere-2024-3765.pdf) |
| 55 | +has been resubmitted with updates to two scenario names (VLLO becomes VL and VLHO becomes LN) plus a new scenario (HL). |
| 56 | +The updated table can be found at https://wcrp-cmip.org/mips/scenariomip/ and below. |
| 57 | +The updated or new scenarios are highlighted in bold. |
| 58 | + |
| 59 | +Scenario | Scenario extension | Primary emission or temperature design criteria |
| 60 | +----------------------------------------------------------------- | ------------------ | ------------------------------------------------------------------------------------------------------------------------- |
| 61 | +High (H) | H-ext | Emissions as high as plausible consistent with climate policy rollback |
| 62 | +**High Low (HL)** | HL-ext | High emissions until second half of the century, followed by rapid decline to net zero CO2 in 2100 |
| 63 | +Medium (M) | M-ext | Emissions consistent with current policies frozen as of 2025 |
| 64 | +Medium Low (ML) | ML-ext | Medium emissions until 2040 followed by gradual decline to net zero CO2 in 2100 |
| 65 | +Low (L) | L-ext | Emissions consistent with staying likely below 2C and not returning to 1.5C before end of the century |
| 66 | +Very Low (VL) **(Formerly Very Low Low Overshoot; VLLO)** | VL-ext | Emissions consistent with limiting warming to 1.5C at the end of the century with overshoot as low as plausible |
| 67 | +Low to Negative (LN) **(Formerly Very Low High Overshoot; VLHO)** | LN-ext | Emissions consistent with limiting warming to 1.5C at end of the century with high overshoot compared to the VL scenario. |
| 68 | + |
| 69 | +Following the H and VL scenario forcings delivery, the CMIP Panel has decided that M and HL will be next in the running order. |
| 70 | + |
| 71 | +**Status of outstanding datasets** |
| 72 | + |
| 73 | +_Land use_ |
| 74 | + |
| 75 | +Preparation of the final H and VL land use scenario forcing datasets is nearing completion and we are anticipating publication by end of February. |
| 76 | + |
| 77 | +_Ozone concentrations and nitrogen deposition_ |
| 78 | + |
| 79 | +Due to delays in the dependent datasets, the delivery of H and VL ozone and nitrogen deposition scenario datasets is now estimated for 10 March. |
| 80 | + |
| 81 | +_Aerosol optical properties/MACv2-SP_ |
| 82 | + |
| 83 | +The expected date for publication for H and VL aerosol plumes scenarios is end of February. |
| 84 | + |
| 85 | +_Future extensions_ |
| 86 | + |
| 87 | +The timeline for future extensions will be confirmed in the coming weeks following delivery of the land use data. |
| 88 | + |
| 89 | +**Impact of delays on downstream activities** |
| 90 | + |
| 91 | +During November 2025, modelling centres completed a survey indicating likely initiation and delivery of CMIP7 DECK and Assessment Fast Track data. |
| 92 | +Around 14 centres responded that they were intending to provide piControl, historical, |
| 93 | +and H and VL scenario data by 1 July 2026 to support downstream activities including ISIMIP, CORDEX and ISMIP7. |
| 94 | +ISIMIP has recently strongly emphasised their preference to receive historical simulation data as soon as possible |
| 95 | +and scenario data ideally by May/June at the latest to allow for their contribution to AR7. |
| 96 | + |
| 97 | +**Where to ask questions and raise issues about the forcing datasets** |
| 98 | + |
| 99 | +These discussions are all being [captured on the input4MIPs GitHub](https://github.com/PCMDI/input4MIPs_CVs/discussions). |
| 100 | +Issues related to any datasets can also be raised here https://github.com/PCMDI/input4MIPs_CVs/issues. |
| 101 | +Please go to these pages to read and engage in any discussions. |
| 102 | +The page has search functionality so you can find what you need. |
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