PMIP4 CESM dust data
The conc
data files were updated on February 26th 2019 (see conc in the 3D part of the Variables section below). Make sure you use the correct version of the data!
Contact
Information and data provided by Samuel Albani
Data files
- each variable for each climate period is in a separate file. In the
conc
(dust concentration) case, which contains the three-dimensional dust concentration in the atmosphere, ancillary variables are also included in the same file, i.e. those necessary to fully describe the vertical coordinate (lev, ilev, hyai, hybi, hyam, hybm, PS) - file names =
PMIP4_DUST_Albani_<field>_<expt>.nc
field
= see Variables section belowexpt
=PI
(pre-Industrial),MH
(mid-Holocene) orLGM
(Last Glacial Maximum)- The gaussian weights file does not depend on the experiment:
PMIP4_DUST_Albani_gw.nc
Dimensions
- nb_time = 12
- 12 time steps in each file, corresponding to the climatological monthly averages (with the exception of
erod
, the soil erodibility variable), indicated as days since 2020-01-01 00:00:00. They are assumed to all have equal weight - time = [ 14, 44, 74, … 284, 314, 344 ]
- nb_lat, nb_lon = 192, 288 (0.95 x 1.25 degrees)
- latitude_values = [ -90, -89.05759, -88.11518, … 88.11518, 89.05759, 90 ]
- longitude_values = [ 0, 1.25, 2.5, … 356.25, 357.5, 358.75 ]
- size_bin = 4 (dust particle size classes)
- dust size bin edges = 0.1, 1.0, 2.5, 5.0, 10.0 μm (diameters)
- size values = [1, 2, 3, 4]
1
= 0.1-1.0 µm,2
= 1.0-2.5 µm,3
= 2.5-5.0 µm,4
= 5.0-10.0 µm (diameters)
- nb_levels = 26 hybrid sigma-pressure levels
- only for the
conc
variable - check the
PMIP4_DUST_Albani_conc_<expt>.nc
files for details about the hybrid coordinates
Variables
2D dust fields
- erod: Soil erodibility
- soil_erodibility
- dimensions: [latitude, longitude]
- units: binary (
0
or1
)
0
= non-erodible grid cell
1
= erodible grid cell
- emis: Dust emission flux (size-resolved)
- tendency_of_atmosphere_mass_content_of_dust_dry_aerosol_particles_due_to_emission
- dimensions: [time, size, latitude, longitude]
- units: kg m-2 s-1
- load: Dust load (size-resolved)
- atmosphere_mass_content_of_dust_dry_aerosol_particles
- dimensions: [time, size, latitude, longitude]
- units: kg m-2
- aot: Dust Aerosol Optical Thickness (size-resolved) at 550 nm
- atmosphere_optical_thickness_due_to_dust_dry_aerosol_particles
- dimensions: [time, size, latitude, longitude]
- units: 1 (unitless)
- ddep: Dust dry deposition flux (size-resolved)
- tendency_of_atmosphere_mass_content_of_dust_dry_aerosol_particles_due_to_dry_deposition
- dimensions: [time, size, latitude, longitude]
- units: kg m-2 s-1
- wdep: Dust wet deposition flux (size-resolved)
- tendency_of_atmosphere_mass_content_of_dust_dry_aerosol_particles_due_to_wet_deposition
- dimensions: [time, size, latitude, longitude]
- units: kg m-2 s-1
- rfts: Dust Direct Radiative Forcing (TOA, SW)
- toa_net_downward_shortwave_radiative_forcing_due_to_dust_dry_aerosol_particles
- dimensions: [time, latitude, longitude]
- units: W m-2
- rftl: Dust Direct Radiative Forcing (TOA, LW)
- toa_net_downward_longwave_radiative_forcing_due_to_dust_dry_aerosol_particles
- dimensions: [time, latitude, longitude]
- units: W m-2
- rfss: Dust Direct Radiative Forcing (surface, SW)
- surface_net_downward_shortwave_radiative_forcing_due_to_dust_dry_aerosol_particles
- dimensions: [time, latitude, longitude]
- units: W m-2
- rfsl: Dust Direct Radiative Forcing (surface, LW)
- surface_net_downward_longwave_radiative_forcing_due_to_dust_dry_aerosol_particles
- dimensions: [time, latitude, longitude]
- units: W m-2
3D dust field
- conc: Dust concentration (size resolved)
The actual units of the conc
variable in the downloadable NetCDF files (μg m-3) were not consistent with the units listed in the files metadata (kg m-3) and the variable description below.
Corrected files (where a scaling factor of 1.e-9 was applied to the data of the previous files) were uploaded on February 26th March 2019.
The Download section at the end of this page lists both the crossed out md5sum checksum of the old files, and the checksum of the new files. The new files also have a new comment global attribute saying This file REPLACES the previous file that had a md5sum of xxxxxxx
- mass_concentration_of_dust_dry_aerosol_particles_in_air
- dimensions: [time, size, lev, latitude, longitude]
- units: kg m-3
The PMIP4_DUST_Albani_conc_<exp>.nc
files also store the ancillary variables necessary to fully describe the vertical coordinate
- ilev: hybrid level at interfaces (1000*(A+B))
- atmosphere_hybrid_sigma_pressure_coordinate
- dimensions: [ilev]
- units: 1
- p(n,k,j,i) = a(k)*p0 + b(k)*ps(n,j,i)
- a: hyai b: hybi p0: P0 ps: PS
- PS: Surface pressure
- surface_air_pressure
- dimensions: [time, latitude, longitude]
- units: Pa
- hyam
- hybrid A coefficient at layer midpoints
- hybm
- hybrid B coefficient at layer midpoints
- hyai
- hybrid A coefficient at layer interfaces
- hybi
- hybrid B coefficient at layer interfaces
References
Please cite at least one of the following papers
- Albani, S., Mahowald, N. M., Perry, A. T., Scanza, R. A., Zender, C. S., Heavens, N. G., Maggi, V., Kok, J. F., and Otto-Bliesner, B. L.: Improved dust representation in the Community Atmosphere Model, J. Adv. Model. Earth Syst., 6, 541–570, doi:10.1002/2013MS000279, 2014.
- Note: this paper describes the LGM simulation
- Albani, S., Mahowald, N. M., Winckler, G., Anderson, R. F., Bradtmiller, L. I., Delmonte, B., François, R., Goman, M., Heavens, N. G., Hesse, P. P., Hovan, S. A., Kang, S., Kohfeld, K. E., Lu, H., Maggi, V., Mason, J. A., Mayewski, P. A., McGee, D., Miao, X., Otto-Bliesner, B. L., Perry, A. T., Pourmand, A., Roberts, H. M., Rosenbloom, N., Stevens, T., and Sun, J.: Twelve thousand years of dust: the Holocene global dust cycle constrained by natural archives, Clim. Past, 11, 869-903, doi:10.5194/cp-11-869-2015, 2015.
- Note: this paper describes the mid-Holocene simulation
- Albani, S., Mahowald, N. M., Murphy, L. N., Raiswell, R., Moore, J. K., Anderson, R. F., McGee, D., Bradtmiller, L., Delmonte, B., Hesse, P. P., and Mayewski, P. A.: Paleodust variability since the Last Glacial Maximum and implications for iron inputs to the ocean, Geophys. Res. Lett., 43, doi:10.1002/2016GL067911, 2016.
- Note: this paper describes the pre-Industrial simulation and compares it to the mid-Holocene and LGM simulations in previous papers
Download
You will find below a table with all the available data files, and their md5sum checksum (if you want to check that you download was OK, you can just type md5sum file.nc
and compare the result to what is displayed in the table).
If you want to download a file, click on the PMIP4 CESM dust data download link and then on the file you need.
md5sum output | Data file |
---|---|
8859ab3b77ce01008785b05fec5cc459 | PMIP4_DUST_Albani_aot_LGM.nc |
a99c8627d21cdc67ab989437b0808e00 | PMIP4_DUST_Albani_aot_MH.nc |
118d105d29a7da31e5a443fba87c4e96 | PMIP4_DUST_Albani_aot_PI.nc |
0e8fb61f0eea7dd9beb756312ee440cb Do not use files that have the crossed out md5sum below | PMIP4_DUST_Albani_conc_LGM.nc |
3864a144e192eaaa2f0920a32725ac77 Do not use files that have the crossed out md5sum below | PMIP4_DUST_Albani_conc_MH.nc |
038ccdb03dd0bf34a96c8912d59d9463 Do not use files that have the crossed out md5sum below | PMIP4_DUST_Albani_conc_PI.nc |
3727a77888c8809a0f87c8e51e37668b | PMIP4_DUST_Albani_ddep_LGM.nc |
568f5f2ecc516a618b27aebbf6ac8475 | PMIP4_DUST_Albani_ddep_MH.nc |
01db9ba162a3ec1f8bd0d0bc2abcc63a | PMIP4_DUST_Albani_ddep_PI.nc |
d29ad13c7508a0389ef0740c83069d1a | PMIP4_DUST_Albani_emis_LGM.nc |
7ecaf8a616bd31ccb600c8162ad8f815 | PMIP4_DUST_Albani_emis_MH.nc |
5eff212c3cfc96bacc119eedfe0ee91e | PMIP4_DUST_Albani_emis_PI.nc |
e14a6ffba0b74a9211ad67e9642b5987 | PMIP4_DUST_Albani_erod_LGM.nc |
5d6f767abbca1e560a5fc326e828aee1 | PMIP4_DUST_Albani_erod_MH.nc |
24e8470134020cecdc552afd2dddf425 | PMIP4_DUST_Albani_erod_PI.nc |
1cf6720ad615ad97b50842298fd02f51 | PMIP4_DUST_Albani_gw.nc |
6c7f9d1a84c36540b42ea6bb1eeadf59 | PMIP4_DUST_Albani_load_LGM.nc |
76079e93089a87e3fd128b9895db3297 | PMIP4_DUST_Albani_load_MH.nc |
2e121549b158cf9dad1761ea681ca835 | PMIP4_DUST_Albani_load_PI.nc |
e47e21fa07df86629e1de6b38459eae0 | PMIP4_DUST_Albani_rfsl_LGM.nc |
46a397182b1c0324173a0bd84b8bf9b9 | PMIP4_DUST_Albani_rfsl_MH.nc |
f9bb094451dd31a8b6d92ba320944307 | PMIP4_DUST_Albani_rfsl_PI.nc |
1359e872a421df6970da5e3e50f453cd | PMIP4_DUST_Albani_rfss_LGM.nc |
cfb9261506308e84d90d1041a8cafb19 | PMIP4_DUST_Albani_rfss_MH.nc |
6b3e529f314775270fd87007c45d4e1b | PMIP4_DUST_Albani_rfss_PI.nc |
a43755b757169c516d2aad9cdffa1456 | PMIP4_DUST_Albani_rftl_LGM.nc |
fb7474a2c61668f9f2b5d88199fdf03b | PMIP4_DUST_Albani_rftl_MH.nc |
b2de8b84a236764234a9abc9cbd3bbb7 | PMIP4_DUST_Albani_rftl_PI.nc |
dfc96dbbe1bf33fc6f9e0cf7a16b8f2a | PMIP4_DUST_Albani_rfts_LGM.nc |
5ad9e6586b2bc7771a7b1b0688767476 | PMIP4_DUST_Albani_rfts_MH.nc |
98b9b2a122b9b9c86bd432e6d1dac502 | PMIP4_DUST_Albani_rfts_PI.nc |
182e86d78be48fc5c2c1ec57f13aa021 | PMIP4_DUST_Albani_wdep_LGM.nc |
f83c22185608042a92107609f59ef658 | PMIP4_DUST_Albani_wdep_MH.nc |
1dc20b285c666765cf9ea61e53a20549 | PMIP4_DUST_Albani_wdep_PI.nc |