Response of atmospheric river width and intensity to aquaplanet warming: A detection algorithm- and background moisture-independent approach
Data files
May 21, 2025 version files 276.26 GB
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IVT_CMCC-CM2-VHR4_20080601-20101231.nc
21.68 GB
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IVT_CMCC-CM2-VHR4_20480601-20501231.nc
21.67 GB
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IVT_MPI_ESM1-2-HR_20480601-20501231.nc
1.84 GB
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IVT_MPI-ESM1-2-HR_20080601-20101231.nc
1.84 GB
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IVTx_plus0K_remap.nc
7.81 GB
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IVTx_plus2K_remap.nc
7.81 GB
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IVTx_plus4K_remap.nc
7.81 GB
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IVTx_plus6K_remap.nc
7.81 GB
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IVTy_plus0K_remap.nc
7.81 GB
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IVTy_plus2K_remap.nc
7.81 GB
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IVTy_plus4K_remap.nc
7.81 GB
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IVTy_plus6K_remap.nc
7.81 GB
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IWV_plus0K_remap.nc
7.81 GB
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IWV_plus2K_remap.nc
7.81 GB
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IWV_plus4K_remap.nc
7.81 GB
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IWV_plus6K_remap.nc
7.81 GB
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README.md
4.41 KB
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spinears_plus0K.nc
17.58 GB
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spinears_plus2K.nc
17.58 GB
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spinears_plus4K.nc
17.58 GB
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spinears_plus6K.nc
17.58 GB
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TE_spinears_CMCC-CM2-VHR4_20080601-20101231.nc
30.07 GB
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TE_spinears_CMCC-CM2-VHR4_20480601-20501231.nc
30.07 GB
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TE_spinears_MPI_ESM1-2-HR_20480601-20501231.nc
2.51 GB
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TE_spinears_MPI-ESM1-2-HR_20080601-20101231.nc
2.51 GB
Abstract
The width of an atmospheric river (AR) is an important parameter when evaluating its impact. Although previous research suggests ARs will widen with global warming, a precise response has been muddled by the large sensitivity of width to a diverse set of AR detection techniques (ARDTs). Here we propose a methodology that removes the influence of the ARDT by modeling AR integrated vapor transport (IVT) profiles as idealized exponential curves with free parameters given by background IVT, intensity above background IVT, and profile width. Notably, our definition for AR profile width does not include any explicit numerical thresholds, relative or absolute, for IVT. We apply our approach to a series of idealized aquaplanet experiments, first with a baseline sea-surface temperature (SST) distribution, then with +2K, +4K and +6K uniform warming, so as to determine the contributions of each free parameter to AR width. We also apply our approach to high resolution atmosphere-only models forced with SSTs modified to preserve historical variability but following projected warming over 2016-2050. Our results show that contributions to impacts-relevant AR widening comes primarily from enhancements in background IVT and AR intensity, as opposed to from dynamic width changes. This dataset provides data needed to reproduce the results of this study.
This dataset provides integrated vapor transport (IVT) and TempestExtremes catalogs for (i) the CESM2 uniform warming experiments and (ii) the CMCC-CM2-VHR4 and MPI-ESM1-2-HR highresSST experiments. Integrated water vapor is also included for the CESM2 experiments. The data provided here accompany (and can be used to reproduce) the results of the above-mentioned study. Brief descriptions of model experiments are provided below:
The CESM2 model is run under an aquaplanet configuration at 3-hourly time resolution. The aquaplanet has no land, sea, ice, topography, or axial tilt (i.e., perpetual equinox conditions), and features a single-layer “data ocean” which thermally forces the atmosphere with fixed sea surface temperatures (SSTs). Specifically, we use the “QOBS” profile from Neale and Hoskins (2000), while the warming scenarios feature globally uniform SST increases of +2 K, +4 K, and +6 K, respectively. Each respective SST experiment (Baseline, +2K, +4, and +6K) is run for 31 months.
We examine "highresSST" experiments of the High Resolution Model Intercomparison Project (HighResMIP) at 6-hourly resolution, focusing on outputs from the CMCC-CM2-VHR4 and MPI-ESM1-2-HR models. The experiments force CMCC-CM2-VHR4 and MPI-ESM1-2-HR models with modified HadISST2.2 that preserve historical variability but follow RCP8.5 warming over 2016-2050. We analyze ARs and IVT from the two models over the North Pacific to better facilitate comparisons to aquaplanet experiments, focusing specifically on two 31-month intervals: (i) 06/01/2008 to 12/31/2010; and (ii) 06/01/2048 to 12/31/2050.
Description of the data and file structure
Files are provided as .nc files. A brief description of the files are provided:
- spinears_plus0K.nc: TempestExtreme spine AR tags for the CESM2 +0K experiment.
- spinears_plus2K.nc: TempestExtreme spine AR tags for the CESM2 +2K experiment.
- spinears_plus4K.nc: TempestExtreme spine AR tags for the CESM2 +4K experiment.
- spinears_plus6K.nc: TempestExtreme spine AR tags for the CESM2 +6K experiment.
- IVTx_plus0K.nc: IVTx for the CESM2 +0K experiment.
- IVTx_plus2K.nc: IVTx for the CESM2 +2K experiment.
- IVTx_plus4K.nc: IVTx for the CESM2 +4K experiment.
- IVTx_plus6K.nc: IVTx for the CESM2 +6K experiment.
- IVTy_plus0K.nc: IVTy for the CESM2 +0K experiment.
- IVTy_plus2K.nc: IVTy for the CESM2 +2K experiment.
- IVTy_plus4K.nc: IVTy for the CESM2 +4K experiment.
- IVTy_plus6K.nc: IVTy for the CESM2 +6K experiment.
- IWV_plus0K.nc: Integrated water vapor for the CESM2 +0K experiment.
- IWV_plus2K.nc: Integrated water vapor for the CESM2 +2K experiment.
- IWV_plus4K.nc: Integrated water vapor for the CESM2 +4K experiment.
- IWV_plus6K.nc: Integrated water vapor for the CESM2 +6K experiment.
- TE_spinears_MPI-ESM1-2-HR_20080601-20101231.nc: TempestExtreme spine AR tags for the MPI-ESM1-2-HR highresSST experiment over 06/01/2008 to 12/31/2010.
- TE_spinears_MPI-ESM1-2-HR_20480601-20501231.nc: TempestExtreme spine AR tags for the MPI-ESM1-2-HR highresSST experiment over 06/01/2048 to 12/31/2050.
- IVT_MPI-ESM1-2-HR_20080601-20101231.nc: IVT for the MPI-ESM1-2-HR highresSST experiment over 06/01/2008 to 12/31/2010.
- IVT_MPI-ESM1-2-HR_20480601-20501231.nc: IVT for the MPI-ESM1-2-HR highresSST experiment over 06/01/2048 to 12/31/2050.
- TE_spinears_CMCC-CM2-VHR4_20080601-20101231.nc: TempestExtreme spine AR tags for the CMCC-CM2-VHR4 highresSST experiment over 06/01/2008 to 12/31/2010.
- TE_spinears_CMCC-CM2-VHR4_20480601-20501231.nc: TempestExtreme spine AR tags for the CMCC-CM2-VHR4 highresSST experiment over 06/01/2048 to 12/31/2050.
- IVT_CMCC-CM2-VHR4_20080601-20101231.nc: IVT for the CMCC-CM2-VHR4 highresSST experiment over 06/01/2008 to 12/31/2010.
- IVT_CMCC-CM2-VHR4_20480601-20501231.nc: IVT for the CMCC-CM2-VHR4 highresSST experiment over 06/01/2048 to 12/31/2050.
Sharing/Access information
The CESM2 experiments were generated by University of California, Davis. The highresSST experiments, including SST and sea ice forcing data, are available at https://highresmip.org/. The TempestExtremes AR detection software is available on Zenodo at https://doi.org/10.5281/zenodo.15320218.
