supplementary-source-id-info.yaml

CEDS-CMIP-2024-07-08:
  publication_status: never_published
CEDS-CMIP-2024-07-08-supplemental:
  publication_status: never_published
CEDS-CMIP-2024-11-25:
  comment_post_publication: &ceds-pre-2025-03-18-comment >-
    A number of updates have been made in CEDS-CMIP-2025-03-18*.
    These are significantly different from this dataset,
    hence it has been retracted.
CEDS-CMIP-2024-11-25-supplemental:
  comment_post_publication: *ceds-pre-2025-03-18-comment
CEDS-CMIP-2024-10-21-supplemental:
  comment_post_publication: *ceds-pre-2025-03-18-comment
CEDS-CMIP-2024-10-21-supplemental:
  comment_post_publication: *ceds-pre-2025-03-18-comment
CEDS-CMIP-2025-03-18:
  comment_post_publication: &ceds-2025-03-18-comment
    A bug was found in gridding of data for
    that led to spurious emissions for CO, CO2, and NOx,
    for the industrial (IND) and energy (ENE) sectors.
    These spurious emissions span 1961 - 2021.
    Globally, the differences represent less than 0.001% of annual emissions,
    but sometimes individual grid cell changes
    can sometimes represent a factor of 2 change (for small emissions).
CEDS-CMIP-2025-03-18-supplemental:
  comment_post_publication: *ceds-2025-03-18-comment
CR-CMIP-0-2-0:
  publication_status: abandoned
CR-CMIP-0-3-0:
  comment_post_publication: >-
    A number of bugs were identified in v0.3.0,
    see [https://github.com/PCMDI/input4MIPs_CVs/discussions/144](https://github.com/PCMDI/input4MIPs_CVs/discussions/144).
    As far as we are aware, v0.4.0 fixes all major bugs identified in v0.3.0.
    For the full list of updates since v0.3.0 (and before),
    see [https://github.com/climate-resource/CMIP-GHG-Concentration-Generation/blob/main/CHANGELOG.md](https://github.com/climate-resource/CMIP-GHG-Concentration-Generation/blob/main/CHANGELOG.md).
    For further analysis of the changes between versions,
    see [https://github.com/climate-resource/CMIP6-vs-CMIP7-GHG-Concentrations](https://github.com/climate-resource/CMIP6-vs-CMIP7-GHG-Concentrations).
CR-CMIP-0-4-0:
  comment_post_publication: >-
    CR-CMIP-0-4-0 is superceded by CR-CMIP-1-0-0.
    CR-CMIP-1-0-0 switches to much more conventional naming for gases.
    The affected gases are: c2f6 (previously pfc116), c3f8 (pfc218),
    c4f10 (pfc3110), c5f12 (pfc4112), c6f14 (pfc5114), c7f16 (pfc6116),
    c8f18 (pfc7118), cc4f8 (pfc318) and ch3ccl3 (hcc140a).

    In CR-CMIP-1-0-0, a DOI is now also included in each file.
    Please use it so we can track usage of these files.

    In terms of science, CR-CMIP-1-0-0 updates to the latest ice core and AGAGE data,
    as well as using better data sources for HFC23, CF4, C2F6 and C3F8 than CR-CMIP-0-4-0.
    CR-CMIP-1-0-0 also provides a smoother transition from ice core based records
    to more recent records (i.e. flask and in-situ samples)
    and more sensible pre-industrial values for gases with non-zero pre-industrial concentrations.
    It also uses the Scripps CO2 record to handle the period from 1959 
    to the start of the flask and in-situ samples from other networks.

    The CR-CMIP-1-0-0 dataset also provides much better information
    about the original data sources.

    As a result, CR-CMIP-0-4-0 is deprecated.

    For the full CHANGELOG,
    see
    [here](https://github.com/climate-resource/CMIP-GHG-Concentration-Generation/blob/main/CHANGELOG.md).

    For basic analysis of the changes between versions,
    see [this repo](https://github.com/climate-resource/CMIP6-vs-CMIP7-GHG-Concentrations).
DRES-CMIP-BB4CMIP7-1-0:
  license_id: CC BY 4.0
  comment_post_publication: >-
    Differences with CMIP6-1-2: The dataset contains data until December 2022 based on GFED4s Global Fire Emissions.
    Furthermore CO2 has been added as separate species.
    This dataset has been developed for the testing phase of CMIP7.

    DRES-CMIP-BB4CMIP7-2-0 extends the data to 2023.
    Modellers are advised to use DRES-CMIP-BB4CMIP7-2-0.
    Tables for validation of the data of various species, geographical areas and sectors 
    can be found on https://www.geo.vu.nl/~gwerf/GFED/GFED4/tables/ for the 1997 onwards period.
DRES-CMIP-BB4CMIP7-2-0:
  doi: 10.25981/ESGF.input4MIPs.CMIP7/2524040
  license_id: CC BY 4.0
  comment_post_publication: >-
    DRES-CMIP-BB4CMIP7-2-1 fixes a bug with NMVOC bulk data for 2023.
    This is the only time slice that is updated.

    As this update does not affect any data before 2021 (inclusive),
    there is no need to restart simulations or make any other changes.
    The new dataset is of course available if people wish to use it.
DRES-CMIP-BB4CMIP7-2-1:
  doi: 10.25981/ESGF.input4MIPs.CMIP7/2524040
FZJ-CMIP-nitrogen-1-0:
  comment_post_publication: >-
    Multiple files shared the same tracking ID.
    They were hence retracted.
    This is fixed in FZJ-CMIP-nitrogen-1-1.
    However, the data is unchanged
    so simulations do not need to be restarted.
FZJ-CMIP-nitrogen-1-1:
  comment_post_publication: >-
    There were faulty N-deposition values in the 1930s across variables
    and the variable wetNOy was 50% too high in both the PI and historical forcing fields
    due to double-counting of some wetNOy components.
    They were hence retracted.
    If you have started simulations with FZJ-CMIP-nitrogen-1-1,
    please restart them with the updated FZJ-CMIP-nitrogen-1-2 data.
    The original issue that identified this is
    <a href="https://github.com/PCMDI/input4MIPs_CVs/issues/385">here</a>
FZJ-CMIP-ozone-1-0:
  comment_post_publication: >-
    The fill value attribute was missing in these files.
    They were hence retracted 
    (although, if you're very careful, they are still usable, you just have to set the fill value manually).
    The original issue that identified this is
    <a href="https://github.com/PCMDI/input4MIPs_CVs/issues/373">here</a>
FZJ-CMIP-ozone-1-1:
  comment_post_publication: >-
    A spurious large value was found in the climatology data related to this dataset,
    see <a href="https://github.com/PCMDI/input4MIPs_CVs/issues/373">here</a>.
    In addition, the latitudinal bounds in this file were not correct.
    Both of these issues are corrected in FZJ-CMIP-ozone-1-2.
FZJ-CMIP-ozone-1-2:
  comment_post_publication: >-
    A member of the community raised an issue with a discontinuity between the piControl climatology and the historical ozone in this version.
    The full discussion is at https://github.com/PCMDI/input4MIPs_CVs/issues/400.

    FZJ-CMIP-ozone-2-0 fixes the underlying issue for the historical period only.
    For piControl, please continue to use the FZJ-CMIP-ozone-1-2 files
    (note that this guidance differs from the email communication sent by the CMIP IPO
    on 12 February 2026).
ImperialCollege-3-0:
  doi: 10.25981/ESGF.input4MIPs.CMIP7/2583902
MRI-JRA55-do-1-6-0:
  license_id: CC BY 4.0
PCMDI-AMIP-1-1-9:
  doi: 10.25981/ESGF.input4MIPs.CMIP6Plus/2583903
  license_id: CC BY 4.0
PCMDI-AMIP-1-1-10:
  license_id: CC BY 4.0
  doi: 10.25981/ESGF.input4MIPs.CMIP7/2575015
PIK-CMIP-1-0-0:
  doi: 10.25981/ESGF.input4MIPs.CMIP7/2583900
  comment_post_publication: >-
    These datasets used an old version of WorldPop/FuturePop data.
    PIK-CMIP-1-0-1 uses revised WorldPop/FuturePop data hence supercedes PIK-CMIP-1-0-0.
    If you have started historical simulations based on `PIK-CMIP-1-0-0`, please restart and use the updated files.
    Note that even for PIK-CMIP-1-0-1, HYDE 3.2 is still used as newer data were not obtained.
    PIK-CMIP-1-0-1 also includes a fix to a bug discovered in the 0.25 degree resolution files in PIK-CMIP-1-0-0
    thanks to @slm7826 and @vnaik60 (see <a href="https://github.com/PCMDI/input4MIPs_CVs/issues/362">#362</a>).
    The 0.5 degree data was not affected by this bug.
SOLARIS-HEPPA-CMIP-4-1:
  publication_status: never_published
SOLARIS-HEPPA-CMIP-4-2:
  license_id: CC BY 4.0
  comment_post_publication: >-
    An issue was encountered with the proton ionization data in v4.2.
    It was hence retracted.
    The original comment from the data provider is
    <a href="https://github.com/PCMDI/input4MIPs_CVs/issues/17#issuecomment-2255378927">here</a>.
SOLARIS-HEPPA-CMIP-4-3:
  license_id: CC BY 4.0
  comment_post_publication: >-
    v4.4 uses the final, absolute TSI scale (in consonance with NNL1) which should be used in CMIP7.
    Hence v4.3 is retracted.
    The change between v4.3 and v4.4 results in a 179 ppm increase of TSI and SSI compared to version 4.3.
    The preliminary TSI/SSI version in 4.3 had adapted the TSI scale from the CTIM instrument alone,
    the newer TSI scale is based on a TSIS-1 and CTIM composite (Coddington and Lean, 2024).
    This composite is also consistent with the TSI 'community consensus' composite
    (spot.colorado.edu/~koppg/TSI/TSI_Composite-SIST.txt).
    The original comment from the data provider is
    <a href="https://github.com/PCMDI/input4MIPs_CVs/issues/66#issuecomment-2422882167">here</a>.
    For further information, see <a href="https://solarisheppa.geomar.de/cmip7">SOLARIS-HEPPA release notes</a>.
SOLARIS-HEPPA-CMIP-4-4:
  comment_post_publication: >-
    v4.5 resolves issues with MEE short-term variability.
    Hence v4.4 is retracted.
    There are no changes to SSI/TSI (so, if you have used v4.4 for SSI/TSI, you do not need to restart).
    The original comment from the data provider is
    <a href="https://github.com/PCMDI/input4MIPs_CVs/issues/139#issuecomment-2493311999">here</a>.
    For further information, see <a href="https://solarisheppa.geomar.de/cmip7">SOLARIS-HEPPA release notes</a>.
SOLARIS-HEPPA-CMIP-4-6:
  doi: 10.25981/ESGF.input4MIPs.CMIP7/2522675
SOLARIS-HEPPA-ScenarioMIP-4-6-a002:
  comment_post_publication: >-
    SOLARIS-HEPPA-ScenarioMIP-4-6 is the same as SOLARIS-HEPPA-ScenarioMIP-4-6-a002,
    it just has updated metadata.
    If you used SOLARIS-HEPPA-ScenarioMIP-4-6-a002, this is fine,
    you do not need to restart your simulations with SOLARIS-HEPPA-ScenarioMIP-4-6.
UCLA-1-0-1:
  comment_post_publication: &ucla-1-0-1-comment >-
    This version was retracted
    because the increasing and decreasing labels are backwards.
    The labels are fixed in UCLA-1-0-2*.
  doi: &ucla-1-0-1-doi >-
   10.25981/ESGF.input4MIPs.CMIP6Plus/2583904
UCLA-1-0-1-constant:
  comment_post_publication: *ucla-1-0-1-comment
  doi: *ucla-1-0-1-doi
UCLA-1-0-1-decreasing:
  comment_post_publication: *ucla-1-0-1-comment
  doi: *ucla-1-0-1-doi
UCLA-1-0-1-increasing:
  comment_post_publication: *ucla-1-0-1-comment
  doi: *ucla-1-0-1-doi
UCLA-1-0-2:
  doi: *ucla-1-0-1-doi
UCLA-1-0-2-constant:
  doi: *ucla-1-0-1-doi
UCLA-1-0-2-decreasing:
  doi: *ucla-1-0-1-doi
UCLA-1-0-2-increasing:
  doi: *ucla-1-0-1-doi
UOEXETER-CMIP-0-1-0:
  publication_status: never_published
UOEXETER-CMIP-1-1-2:
  publication_status: never_published
UOEXETER-CMIP-1-1-3:
  comment_post_publication: >-
    v1.2.0 includes climatology data (for piControl simulations)
    and updates the handling of small eruptions.
    Hence v1.1.3 is deprecated.
UOEXETER-CMIP-1-2-0:
  comment_post_publication: >-
    v1.3.0 updates the handling of small eruptions in the pre-satellite era.
    Hence v1.2.0 is deprecated.
UOEXETER-CMIP-1-3-0:
  comment_post_publication: >-
    v1.3.1 does minor plus updates and adds the aerosol number density requested by some modelling groups.
    Hence v1.3.0 is deprecated.
UOEXETER-CMIP-1-3-1:
  comment_post_publication: >-
    v2.0.0 includes the following key updates:
    i) new H2SO4 number density variable replacing aerosol number density;
    ii) correction to the 1920-1978 ice-core dataset,
    improving consistency with pyrheliometer measurements and CMIP6.
    As a result of this change, the mean historical SAOD has decreased a bit, but it is still higher than CMIP6.
    Hence v1.3.1 is deprecated.
UOEXETER-CMIP-2-0-0:
  comment_post_publication: >-
    v2.2.1 resolves issues with NaN values in v2.0.0
    and updates a few other issues
    (notably the latitudinal distrbution of the Agung eruption).
    These updates affect both the historical values
    and the pre-industrial climatologies.
    As a result of this change, v2.0.0 is deprecated.
    Please restart any simulations that used v2.0.0
    and use v2.2.1 instead.
  doi: 10.25981/ESGF.input4MIPs.CMIP7/2522673
  further_info_url: https://input4mips-cvs.readthedocs.io/en/latest/dataset-overviews/stratospheric-volcanic-so2-emissions-aod/
UOEXETER-CMIP-2-2-1:
  further_info_url: https://input4mips-cvs.readthedocs.io/en/latest/dataset-overviews/stratospheric-volcanic-so2-emissions-aod/
  doi: 10.25981/ESGF.input4MIPs.CMIP7/2522673
UOEXETER-ScenarioMIP-2-2-1:
  further_info_url: https://input4mips-cvs.readthedocs.io/en/latest/dataset-overviews/stratospheric-volcanic-so2-emissions-aod/
  comment_post_publication: >-
    v2.2.2 resolves issues with troposphere masking in v2.2.1.
    As a result of this change, v2.2.1 is deprecated.
    Please restart any scenario simulations that used v2.2.1
    and use v2.2.2 instead.
UofMD-landState-3-0:
  license_id: CC BY 4.0
  comment_post_publication: >-
    v3.0 contains a number of spurious spikes post-1950.
    These have been addressed in v3.1.
    As a result, v3.0 has been retracted.
UofMD-landState-3-1:
  license_id: CC BY 4.0
  comment_post_publication: >-
    v3.1 contains an extra variable (crpbf_total) in the land-use management file.
    This is filled with zeroes, so will not affect simulations.
    However, for completeness, we have released an update (v3.1.1)
    which removes this unnecessary variable
    (but using v3.1 is fine if that is what you're doing already).