Output Quantities#
Vertical profile quantities#
Name | SI-Unit | Description |
---|---|---|
clay | kg m-3 | mass concentration of clay-sized particles Particles with a diameter less than or equal to 4.0E-6 m are considered |
dust | kg m-3 | mass concentration of dust-sized particles Particles with a diameter less than or equal to 63.0E-6 m are considered |
e | m2 s-2 | SGS turbulence kinetic energy |
e* | m2 s-2 | resolved-scale turbulence kinetic energy Calculated from variances or fluxes (see https://palm.muk.uni-hannover.de/trac/wiki/doc/tec/advection#statistical_evaluation). |
eta | m | Kolmogorov length scale Only meaningful for DNS mode. The Kolmogorov length scale \(\eta\) is defined by \((\nu^3/\epsilon)^{1/4}\) with \(\nu\) being the kinematic, molecular viscosity and \(\epsilon\) being the turbulent kinetic energy dissipation rate. However, as LES is not resolving the smallest velocity scales, the direct determination of the dissipation rate and therefore of the Kolmogorov length scale is not possible in general. Only if run in DNS mode, a meaningful value of \(\eta\) will be output. |
hyp | hPa | hydrostatic pressure |
kc_X | ppm or kg m-3 | concentration of chemical species X Chemistry quantities requires the prefix kc_. X indicates the species name. Only species names belonging to the selected chemistry mechanism are allowed. |
kc_w*X* | ppm m s-1 or kg s-1 m-2 | resolved-scale turbulent vertical flux of chemical species X Chemistry quantities requires the prefix kc_. X indicates the species name. Only species names belonging to the selected chemistry mechanism are allowed. |
kc_w"X" | ppm m s-1 or kg s-1 m-2 | subgrid-scale turbulent vertical flux of chemical species X Chemistry quantities requires the prefix kc_. X indicates the species name. Only species names belonging to the selected chemistry mechanism are allowed. |
kh | m2 s-1 | eddy diffusivity for heat |
km | m2 s-1 | eddy diffusivity for momentum |
l | m | mixing length |
m_soil | m3 m-3 | volumetric soil moisture |
nc | m-3 | cloud drop number density Requires cloud_scheme = morrison. |
ni | m-3 | ice crystal number density Requires cloud_scheme = 'seifert_beheng' or 'morrison' and microphysics_ice_phase = .T.. |
nr | m-3 | rain drop number density Requires cloud_scheme = 'seifert_beheng'. |
p | Pa | perturbation pressure |
prho | kg m-3 | potential density |
prr | kg kg-1 m s-1 | total precipitation rate of all cloud species Is allowed for all schemes except of cloud_scheme = 'sat_adjust'. |
prr_cloud | kg kg-1 m s-1 | precipitation rate of cloud droplets (by sedimentation) Is allowed for all schemes except of cloud_scheme = 'sat_adjust', but makes only sense if cloud_water_sedimentation = .T.. |
prr_graupel | kg kg-1 m s-1 | precipitation rate of graupel Requires cloud_scheme = 'seifert_beheng' or 'morrison', and microphysics_ice_phase = .T., and snow = .T., and graupel = .T.. |
q | kg kg-1 | water vapor mixing ratio (or total water mixing ratio if cloud physics is switched on) Requires humidity = .T.. |
qc | kg kg-1 | cloud water mixing ratio Requires cloud_scheme = 'seifert_beheng' or 'morrison'. |
qg | kg kg-1 | graupel mixing ratio Requires cloud_scheme = 'seifert_beheng' or 'morrison', and microphysics_ice_phase = .T., and snow = .T., and graupel = .T.. |
qi | kg kg-1 | ice crystal mixing ratio Requires cloud_scheme = 'seifert_beheng' or 'morrison', and microphysics_ice_phase = .T.. |
ql | kg kg-1 | liquid water mixing ratio Requires using the bulk cloud model (BCM) or the Lagrangian cloud model (LCM) via setting of cloud_droplets = .T.. |
qr | kg kg-1 | rain water mixing ratio Requires cloud_scheme = 'seifert_beheng'. |
qs | kg kg-1 | snow mixing ratio Requires cloud_scheme = 'seifert_beheng' or 'morrison', and microphysics_ice_phase = .T., and snow = .T., and graupel = .T.. |
qv | kg kg-1 | water vapor mixing ratio Requires using the bulk cloud model (BCM). |
q*2 | kg2 kg-2 | variance of water vapor mixing ratio (or total water mixing ratio if cloud physics is switched on) Requires humidity = .T.. |
rad_lw_in | W m-2 | incoming longwave radiation flux |
rad_lw_out | W m-2 | outgoing longwave radiation flux |
rad_sw_in | W m-2 | incoming shortwave radiation flux |
rad_sw_out | W m-2 | outgoing shortwave radiation flux |
rh | % | relative humidity Requires humidity = .T.. |
rho | kg m-3 | air density |
rho_sea_water | kg m-3 | density of sea water Requires ocean module switched on. |
s | kg m-3 or ppm | concentration of passive scalar Requires passive_scalar = .T.. |
sa | psu | salinity of sea water Requires ocean module switched on. |
salsa_LDSA | micro m2 cm-3 | total lung-deposited surface area |
salsa_N_UFP | m-3 | total aerosol number concentration of particles smaller than 0.1 µm in diameter, i.e. ultrafine particles |
salsa_N_tot | m-3 | total aerosol number concentration |
salsa_PM0.1 | kg m-3 | total mass concentration of particulate matter smaller than 0.1 µm in diameter, i.e. ultrafine particles |
salsa_PM2.5 | kg m-3 | total mass concentration of particulate matter smaller than 2.5 µm in diameter, i.e. ultrafine particles |
salsa_PM10 | kg m-3 | total mass concentration of particulate matter smaller than 10 µm in diameter, i.e. ultrafine particles |
silt | kg m-3 | mass concentration of silt-sized particles Particles with a diameter greater than 4.0E-6 m and less than or equal to 63.0E-6 m are considered |
Sw | 1 | skewness of the w-velocity component Sw is defined as \(w^3 / (w^2)^{1.5}\), where \(w\) is the resolved-scale vertical velocity. |
s*2 | (kg m-3)2 | resolved scale variance of the passive scalar Requires passive_scalar = .T.. |
t_soil | K | soil temperature |
td_lsa_q | kg kg-1 s-1 | horizontal large scale advection tendency for humidity |
td_lsa_thetal | K s-1 | horizontal large scale advection tendency for temperature |
td_nud_q | kg kg-1 s-1 | nudging tendency for humidity |
td_nud_thetal | K s-1 | nudging tendency for temperature |
td_nud_u | m s-2 | nudging tendency for u-component of velocity |
td_nud_v | m s-2 | nudging tendency for v-component of velocity |
td_sub_q | kg kg-1 s-1 | horizontal large scale subsidence tendency for humidity |
td_sub_thetal | K s-1 | horizontal large scale subsidence tendency for temperature |
theta | K | potential temperature |
thetav | K | virtual potential temperature Requires humidity = .T.. |
u | m s-1 | u-component of velocity vector |
ug | m s-1 | u-component of the geostrophic wind |
u*2 | m2 s-2 | variance or horizontal momentum flux of the resolved scale u-velocity component In case of momentum_advec = 'ws-scheme', see statistical evaluation. |
v | m s-1 | v-component of velocity vector |
vg | m s-1 | v-component of the geostrophic wind |
v*2 | m2 s-2 | variance or horizontal momentum flux of the resolved-scale v-velocity component In case of momentum_advec = 'ws-scheme', see statistical evaluation. |
w | m s-1 | w-component of velocity vector |
wq | kg kg-1 m s-1 or W m-2 | total vertical turbulent water flux Sum of w"q" and w*q*. |
wqv | kg kg-1 m s-1 or W m-2 | total vertical turbulent latent heat flux Sum of w"qv" and w*qv*. |
ws | kg m-2 s-1 or ppm m s-1 | total vertical turbulent scalar concentration flux Sum of w"s" and w*s*. Requires passive_scalar = .T.. |
wsa | psu m s-1 | total vertical turbulent salinity flux Sum of w"sa" and w*sa*. Requires ocean mode switched on. |
wtheta | K m s-1 or W m-2 | total vertical turbulent sensible heat flux Sum of w"theta" and w*theta*. |
wthetaBC | K m s-1 or W m-2 | total vertical turbulent sensible heat flux when using the Bott-Chlond scheme Sum of w"theta" and w*thetaBC*. |
wthetav | K m s-1 or W m-2 | total vertical turbulent buoyancy flux Sum of w"theta" and w*thetav*. |
wu | m2 s-2 | u-component of the total vertical turbulent momentum flux Sum of w"u" and w*u*. |
wv | m2 s-2 | v-component of the total vertical turbulent momentum flux Sum of w"v" and w*v*. |
w_subs | m s-1 | large-scale vertical subsidence |
w*e* | m3 s-3 | vertical flux of resolved-scale turbulence kinetic energy |
w*q* | kg kg-1 m s-1 or W m-2 | covariance or resolved-scale vertical turbulent water flux In case of scalar_advec = 'ws-scheme' see statistical evaluation. |
w*qv* | kg kg-1 m s-1 or W m-2 | covariance or resolved-scale vertical turbulent latent heat flux In case of scalar_advec = 'ws-scheme' see statistical evaluation. |
w*p*ddz | Pa m s-2 | divergence of transport of resolved-scale TKE due to pressure fluctuations Identical to term that appears in the resolved-scale TKE budget equation. |
w*s* | kg m-2 s-1 or ppm m s-1 | resolved-scale vertical turbulent scalar concentration flux Requires passive_scalar = .T.. |
w*sa* | psu m s-1 | resolved-scale vertical turbulent salinity flux Requires ocean mode switched on. |
w*theta* | K m s-1 or W m-2 | covariance or resolved-scale vertical turbulent sensible heat flux In case of scalar_advec = 'ws-scheme' see statistical evaluation. |
w*theta*2 | K2 m s-1 | resolved-scale third moment |
w*theta*BC | K m s-1 or W m-2 | resolved-scale vertical turbulent sensible heat flux when using the Bott-Chlond scheme |
w*thetav* | K m s-1 or W m-2 | resolved-scale vertical turbulent buoyancy flux |
w*u* | m2 s-2 | covariance or u-component of resolved-scale vertical turbulent momentum flux In case of momentum_advec = 'ws-scheme' see statistical_evaluation. |
w*u*u*ddz | m2 s-3 | divergence of turbulent transport of resolved-scale TKE Identical to term that appears in the resolved-scale TKE budget equation. |
w*v* | m2 s-2 | covariance or v-component of resolved-scale vertical turbulent momentum flux In case of momentum_advec = 'ws-scheme' see statistical evaluation. |
w*2 | m2 s-2 | variance or horizontal momentum flux of the resolved-scale w-velocity component In case of momentum_advec = 'ws-scheme', see statistical evaluation. |
w*2theta* | K m2 s-2 | resolved-scale third moment |
w*3 | m3 s-3 | third moment of the resolved-scale w-velocity component |
w"e | m3 s-3 | turbulent vertical flux of subgrid-scale TKE |
w"eddz | m2 s-3 | divergence of turbulent vertical flux of subgrid-scale TKE |
w"q" | kg kg-1 m s-1 or W m-2 | subgrid-scale vertical turbulent water flux |
w"qv" | kg kg-1 m s-1 or W m-2 | subgrid-scale vertical turbulent latent heat flux |
w"s" | kg m-2 s-1 or ppm m s-1 | subgrid-scale vertical turbulent scalar concentration flux Requires passive_scalar = .T.. |
w"sa" | psu m s-1 | subgrid-scale vertical turbulent salinity flux Requires ocean mode switched on. |
w"theta" | K m s-1 or W m-2 | subgrid-scale vertical turbulent sensible heat flux |
w"thetav" | K m s-1 or W m-2 | subgrid-scale vertical turbulent buoyancy flux |
w"u" | m2 s-2 | u-component of subgrid-scale vertical turbulent momentum flux |
w"v" | m2 s-2 | v-component of subgrid-scale vertical turbulent momentum flux |
3d-array quantities#
Name | SI-Unit | Description |
---|---|---|
clay | kg m-3 | mass concentration of clay-sized particles Particles with a diameter less than or equal to 4.0E-6 m are considered |
div_new | s-1 | flow divergence after corrector step After calling the pressure solver the divergence is usually reduced by several orders of magnitude, except for grid locations near topography, where the divergence at wall-bounded grid points is often only slightly reduced. In the majority of application this does not significantly impact the simulation results. However, attention has to be paid in case of dispersion studies (Eulerian approach), where chemical species or passive tracers might be impacted. Due to the non-vanishing divergence an additional sink/source term is implicitly imposed by the advection scheme, even though we already consider a correction term in the advection-term discretization. Due to this numerical error the scalar transport cannot be considered as fully conservative any more. Usually additional source/sink term is small and can be neglected. Anyhow, users should carefully check their simulation results in this regard. |
div_old | s-1 | flow divergence at predictor step (before corrector step) |
dust | kg m-3 | mass concentration of dust-sized particles Particles with a diameter less than or equal to 63.0E-6 m are considered |
dust_mc_bin<b> | kg m-3 | mass concentration of a dust size bin <d> is one of the dust size bin numbers: 1, 2, 3, ... . |
e | m2 s-2 | SGS turbulence kinetic energy |
hr | K s-1 | heating rate Indicates the heating/cooling of an air volume by direct heating/cooling of the air volume by radiation flux divergences (only RRTMG), by diabatic processes at plants, as well as by surface forcing. Note, no heating/cooling by advection, condensation, etc. is considered. This quantity is especially useful to evaluate katabatic flows where radiative cooling of air volumes, emission at plant surfaces, and radiative surface cooling is dominant. |
im_hf_roof | K m s-1 | heatflux at building roof Only 3D output possible. |
im_hf_roof_waste | K m s-1 | waste heatflux at building roof Only 3D output possible. |
im_hf_wall_win | K m s-1 | heatflux at building walls and windows Only 3D output possible. |
im_hf_wall_win_waste | K m s-1 | waste heatflux at building walls and windows Only 3D output possible. |
im_t_indoor_mean | K | mean indoor temperature Horizontal building average at each storey. Only 3D output possible. |
im_theta_10cm_roof | K | 10-cm potential temperature above roofs Only 3D output possible. |
im_theta_10cm_wall | K | 10-cm potential temperature at vertical walls Only 3D output possible. |
kc_X | ppm or kg m-3 | concentration of chemical species X Chemistry quantities requires the prefix kc_. X indicates the species name. Only species names belonging to the selected chemistry mechanism are allowed. |
m_soil | m3 m-3 | volumetric soil moisture |
nc | m-3 | cloud drop number density Requires cloud_scheme = morrison. |
ng | m-3 | graupel number density Requires cloud_scheme = 'seifert_beheng' or 'morrison', and microphysics_ice_phase = .T., and snow = .T., and graupel = .T.. |
ni | m-3 | ice crystal number density Requires cloud_scheme = 'seifert_beheng' or 'morrison' and microphysics_ice_phase = .T.. |
nr | m-3 | rain drop number density Requires cloud_scheme = 'seifert_beheng'. |
ns | m-3 | snow number density Requires cloud_scheme = 'seifert_beheng' or 'morrison', and microphysics_ice_phase = .T., and snow = .T., and graupel = .T.. |
p | Pa | perturbation pressure |
pc | number per gridbox | particle/droplet concentration |
pcm_bad | m2 m-3 | basal area density Only 3d-output possible. |
pcm_heatrate | K s-1 | plant canopy heating rate by solar radiation Only 3d-output possible. |
pcm_lad | m2 m-3 | leaf area density Only 3d-output possible. |
pcm_latentrate | K s-1 | plant canopy latent heat flux Only 3d-output possible. |
pcm_transpirationrate | kg kg-1 s-1 | plant canopy transpiration rate by solar radiation Only 3d-output possible. |
pr | m | mean particle/droplet radius |
prr | kg kg-1 m s-1 | total precipitation rate of all cloud species Is allowed for all schemes except of cloud_scheme = 'sat_adjust'. |
prr_cloud | kg kg-1 m s-1 | precipitation rate of cloud droplets (by sedimentation) Is allowed for all schemes except of cloud_scheme = 'sat_adjust', but makes only sense if cloud_water_sedimentation = .T.. |
prr_graupel | kg kg-1 m s-1 | precipitation rate of graupel Requires cloud_scheme = 'seifert_beheng' or 'morrison', and microphysics_ice_phase = .T., and snow = .T., and graupel = .T.. |
prr_ice | kg kg-1 m s-1 | precipitation rate of ice crystals Requires cloud_scheme = 'seifert_beheng' or 'morrison', and microphysics_ice_phase = .T.. |
prr_rain | kg kg-1 m s-1 | precipitation rate of rain droplets Is allowed for all schemes except of cloud_scheme = 'sat_adjust'. |
prr_snow | kg kg-1 m s-1 | precipitation rate of snow Requires cloud_scheme = 'seifert_beheng' or 'morrison', and microphysics_ice_phase = .T., and snow = .T., and graupel = .T.. |
q | kg kg-1 | water vapor mixing ratio (or total water mixing ratio if cloud physics is switched on) Requires humidity = .T.. |
qc | kg kg-1 | cloud water mixing ratio Requires cloud_scheme = 'seifert_beheng' or 'morrison'. |
qg | kg kg-1 | graupel mixing ratio Requires cloud_scheme = 'seifert_beheng' or 'morrison', and microphysics_ice_phase = .T., and snow = .T., and graupel = .T.. |
qi | kg kg-1 | ice crystal mixing ratio Requires cloud_scheme = 'seifert_beheng' or 'morrison', and microphysics_ice_phase = .T.. |
ql | kg kg-1 | liquid water mixing ratio Requires using the bulk cloud model (BCM) or the Lagrangian cloud model (LCM) via setting of cloud_droplets = .T.. |
ql_c | kg kg-1 | change in liquid water mixing ratio due to condensation/evaporation during last time step Requires to switch on the Lagrangian cloud model (LCM) via setting of cloud_droplets = .T.. |
ql_v | m3 per gridpox | volume of liquid water Requires to switch on the Lagrangian cloud model (LCM) via setting of cloud_droplets = .T.. |
ql_vp | 1 | weighting factor Requires to switch on the Lagrangian cloud model (LCM) via setting of cloud_droplets = .T.. |
qr | kg kg-1 | rain water mixing ratio Requires cloud_scheme = 'seifert_beheng'. |
qs | kg kg-1 | snow mixing ratio Requires cloud_scheme = 'seifert_beheng' or 'morrison', and microphysics_ice_phase = .T., and snow = .T., and graupel = .T.. |
qv | kg kg-1 | water vapor mixing ratio Requires using the bulk cloud model (BCM). |
rad_lw_cs_hr | K h-1 | clear-sky longwave radiative heating rate |
rad_lw_hr | K h-1 | longwave radiative heating rate |
rad_lw_in | W m-2 | incoming longwave radiation flux |
rad_lw_out | W m-2 | outgoing longwave radiation flux |
rad_sw_cs_hr | K h-1 | clear-sky shortwave radiative heating rate |
rad_sw_hr | K h-1 | shortwave radiative heating rate |
rad_sw_in | W m-2 | incoming shortwave radiation flux |
rad_sw_out | W m-2 | outgoing shortwave radiation flux |
rh | % | relative humidity Requires humidity = .T.. |
rho_sea_water | kg m-3 | density of sea water Requires ocean module switched on. |
rtm_dif_<d>_<i>_<j>_<k> | 1 | transparency of view factor of the surface to a surface with i,j,k coordinates <d> is one of the directions: up, down, south, north, west, or east. <i>, <j>,<k> are coordinates of pair surfaces. |
rtm_mrt | K | mean radiant temperature |
rtm_mrt_lw | W m-2 | LW fraction of MRT radiation flux |
rtm_mrt_sw | W m-2 | SW fraction of MRT radiation flux |
rtm_rad_inlw_<d> | W m-2 | complete incoming LW radiation at the surface <d> is one of the directions: up, down, south, north, west, or east. |
rtm_rad_inlwdif_<d> | W m-2 | incoming diffuse LW radiation at the surface <d> is one of the directions: up, down, south, north, west, or east. |
rtm_rad_inlwref_<d> | W m-2 | incoming reflected and emitted LW radiation at the surface <d> is one of the directions: up, down, south, north, west, or east. |
rtm_rad_insw_<d> | W m-2 | complete incoming SW radiation at the surface <d> is one of the directions: up, down, south, north, west, or east. |
rtm_rad_inswdif_<d> | W m-2 | incoming diffuse solar SW radiation at the surface <d> is one of the directions: up, down, south, north, west, or east. |
rtm_rad_inswdir_<d> | W m-2 | incoming direct solar SW radiation at the surface <d> is one of the directions: up, down, south, north, west, or east. |
rtm_rad_inswref_<d> | W m-2 | incoming reflected SW radiation at the surface <d> is one of the directions: up, down, south, north, west, or east. |
rtm_rad_net_<d> | W m-2 | net radiation flux at the surface <d> is one of the directions: up, down, south, north, west, or east. |
rtm_rad_outlw_<d> | W m-2 | outgoing LW radiation from the surface <d> is one of the directions: up, down, south, north, west, or east. |
rtm_rad_outsw_<d> | W m-2 | outgoing SW radiation from the surface <d> is one of the directions: up, down, south, north, west, or east. |
rtm_rad_pc_inlw_<d> | W m-2 | LW radiation absorbed by plant canopy <d> is one of the directions: up, down, south, north, west, or east. |
rtm_rad_pc_insw_<d> | W m-2 | SW radiation absorbed by plant canopy <d> is one of the directions: up, down, south, north, west, or east. |
rtm_rad_pc_inswdif_<d> | W m-2 | diffuse solar SW radiation absorbed by plant canopy <d> is one of the directions: up, down, south, north, west, or east. |
rtm_rad_pc_inswdir_<d> | W m-2 | direct solar SW radiation absorbed by plant canopy <d> is one of the directions: up, down, south, north, west, or east. |
rtm_rad_pc_inswref_<d> | W m-2 | reflected SW radiation absorbed by plant canopy <d> is one of the directions: up, down, south, north, west, or east. |
rtm_rad_reslw_<d> | W m-2 | residuum of LW radiation absorbed in surface after last reflection <d> is one of the directions: up, down, south, north, west, or east. |
rtm_rad_ressw_<d> | W m-2 | residuum of SW radiation absorbed in surface after last reflection <d> is one of the directions: up, down, south, north, west, or east. |
rtm_skyvf_<d> | 1 | sky view factor <d> is one of the directions: up, down, south, north, west, or east. |
rtm_skyvft_<d> | 1 | sky view factor including transparency of plant canopy <d> is one of the directions: up, down, south, north, west, or east. |
rtm_surfalb_<d> | 1 | effective albedo of the surface (weighted average of fractions) <d> is one of the directions: up, down, south, north, west, or east. |
rtm_surfemis_<d> | 1 | effective emissivity of the surface (weighted average of fractions) <d> is one of the directions: up, down, south, north, west, or east. |
rtm_svf_<d>_<i>_<j>_<k> | 1 | view factor of the surface to a surface with i,j,k coordinates <d> is one of the directions: up, down, south, north, west, or east. <i>, <j>, <k> are coordinates of pair surfaces. |
s | kg m-3 or ppm | concentration of passive scalar Requires passive_scalar = .T.. |
sa | psu | salinity of sea water Requires ocean module switched on. |
salsa_g_<gaseous_compound> | m-3 | concentration of <gaseous_compound> <gaseous_compound> is one of H2SO4, HNO3, NH3, OCNV, OCSV |
salsa_LDSA | micro m2 cm-3 | total lung-deposited surface area |
salsa_N_bin<bin number> | m-3 | aerosol number concentration in the aerosol size bin <bin number> is one of the specified aerosol bins |
salsa_N_UFP | m-3 | total aerosol number concentration of particles smaller than 0.1 µm in diameter, i.e. ultrafine particles |
salsa_N_tot | m-3 | total aerosol number concentration |
salsa_PM0.1 | kg m-3 | total mass concentration of particulate matter smaller than 0.1 µm in diameter, i.e. ultrafine particles |
salsa_PM2.5 | kg m-3 | total mass concentration of particulate matter smaller than 2.5 µm in diameter, i.e. ultrafine particles |
salsa_PM10 | kg m-3 | total mass concentration of particulate matter smaller than 10 µm in diameter, i.e. ultrafine particles |
salsa_s_<chemical_compound> | kg m-3 | concentration of <chemical_compound> in the aerosol phase <chemical_compound> is one of BC, DU, NH, NO, OC, SO4, SS, H2O |
silt | kg m-3 | mass concentration of silt-sized particles Particles with a diameter greater than 4.0E-6 m and less than or equal to 63.0E-6 m are considered |
slurb_t_road | K | road layer temperature |
slurb_t_roof | K | roof layer temperature |
slurb_t_wall_a | K | wall A layer temperature |
slurb_t_wall_b | K | wall A layer temperature Same as slurb_t_wall_a if anisotropic_street_canyons = .F.. |
slurb_t_win_a | K | window A layer temperature |
slurb_t_win_b | K | window A layer temperature Same as slurb_t_win_a if anisotropic_street_canyons = .F.. |
t_soil | K | soil temperature |
ta | °C | true air temperature |
theta | K | potential temperature |
thetal | K | liquid water potential temperature Requires using the bulk cloud model (BCM). |
thetav | K | virtual potential temperature Requires humidity = .T.. |
ti | s-1 | curl of velocity vector (magnitude) |
u | m s-1 | u-component of velocity vector |
usm_iwghf_<d> | W m-2 | ground heat flux from indoor surface of wall or roof <d> is one of the directions: up, down, south, north, west, or east. |
usm_iwghf_window_<d> | W m-2 | ground heat flux from indoor surface of window <d> is one of the directions: up, down, south, north, west, or east. |
usm_qsws_<d> | W m-2 | latent heat flux from surface <d> is one of the directions: up, down, south, north, west, or east. |
usm_qsws_liq_<d> | W m-2 | latent heat flux from liquid surface <d> is one of the directions: up, down, south, north, west, or east. |
usm_qsws_veg_<d> | W m-2 | latent heat flux from vegetation surface <d> is one of the directions: up, down, south, north, west, or east. |
usm_surfcat_<d> | 1 | surface category <d> is one of the directions: up, down, south, north, west, or east. |
usm_surfwintrans_<d> | W m-2 | transmissivity window tiles <d> is one of the directions: up, down, south, north, west, or east. |
usm_surfz_<d> | 1 | surface height (z) <d> is one of the directions: up, down, south, north, west, or east. |
usm_swc_<k>_<d> | m3 m-3 | soil water content of k-th layer of green fraction <d> is one of the directions: up, down, south, north, west, or east. <k> is the number of the green layer. |
usm_t_green_<k>_<d> | K | temperature of k-th layer of green fraction <d> is one of the directions: up, down, south, north, west, or east. <k> is the number of the green layer. |
usm_t_surf_green_<d> | K | surface temperature of green surface <d> is one of the directions: up, down, south, north, west, or east. |
usm_t_surf_wall_<d> | K | surface temperature of wall or roof surface <d> is one of the directions: up, down, south, north, west, or east. |
usm_t_surf_window_<d> | K | surface temperature of window surface <d> is one of the directions: up, down, south, north, west, or east. |
usm_t_wall_<k>_<d> | K | temperature of k-th layer of wall fraction <d> is one of the directions: up, down, south, north, west, or east. <k> is the number of the wall layer. |
usm_t_window_<k>_<d> | K | temperature of k-th layer of window fraction <d> is one of the directions: up, down, south, north, west, or east. <k> is the number of the window layer. |
usm_wghf_<d> | W m-2 | ground heat flux from wall or roof surface <d> is one of the directions: up, down, south, north, west, or east. |
usm_wghf_green_<d> | W m-2 | ground heat flux from green surface <d> is one of the directions: up, down, south, north, west, or east. |
usm_wghf_window_<d> | W m-2 | ground heat flux from window surface <d> is one of the directions: up, down, south, north, west, or east. |
usm_wshf_<d> | W m-2 | sensible heat flux from surface <d> is one of the directions: up, down, south, north, west, or east. |
uu_product | m2 s-2 | product of u and u To be used for calculation of resolved-scale transport <u'u'> in case of horizontal inhomogeneity. Output is defined on u-grid. Computation of <u'u'> is possible in post-processing via temporal EC-method, i.e. <u'u'> = <uu> - <u><u>, with < > being the temporal average. For accurate flux calculation the time averaging needs to be sufficiently long (usually 30min) and data from each timestep should enter the average to sample also high-frequency flux contributions (choose dt_averaging_input small enough). |
uv_product | m2 s-2 | product of u and v To be used for calculation of resolved scale transport <u'v'> in case of horizontal inhomogeneity. Output is defined on u-grid. Therefore, output of uv is not necessarily identical to output of vu. Output of both quantities, however, can be useful for computation of spatial flux gradients. Computation of <u'v'> is possible in post-processing via temporal EC-method, i.e. <u'v'> = <uv> - <u><v>, with < > being the temporal average. For accurate flux calculation the time averaging needs to be sufficiently long (usually 30min) and data from each timestep should enter the average to sample also high-frequency flux contributions (choose dt_averaging_input small enough). |
uw_product | m2 s-2 | product of u and w To be used for calculation of resolved scale transport <u'w'> in case of horizontal inhomogeneity. Output is defined on u-grid. Therefore, output of uw is not necessarily identical to output of wu. Output of both quantities, however, can be useful for computation of spatial flux gradients. Computation of <u'w'> is possible in post-processing via temporal EC-method, i.e. <u'w'> = <uw> - <u><w>, with < > being the temporal average. For accurate flux calculation the time averaging needs to be sufficiently long (usually 30min) and data from each timestep should enter the average to sample also high-frequency flux contributions (choose dt_averaging_input small enough). |
v | m s-1 | v-component of velocity vector |
vu_product | m2 s-2 | product of v and u To be used for calculation of resolved scale transport <v'u'> in case of horizontal inhomogeneity. Output is defined on v-grid. Therefore, output of vu is not necessarily identical to output of uv. Output of both quantities, however, can be useful for computation of spatial flux gradients. Computation of <v'u'> is possible in post-processing via temporal EC-method, i.e. <v'u'> = <vu> - <v><u>, with < > being the temporal average. For accurate flux calculation the time averaging needs to be sufficiently long (usually 30min) and data from each timestep should enter the average to sample also high-frequency flux contributions (choose dt_averaging_input small enough). |
vv_product | m2 s-2 | product of v and v To be used for calculation of resolved-scale transport <v'v'> in case of horizontal inhomogeneity. Output is defined on v-grid. Computation of <v'v'> is possible in post-processing via temporal EC-method, i.e. <v'v'> = <vv> - <v><v>, with < > being the temporal average. For accurate flux calculation the time averaging needs to be sufficiently long (usually 30min) and data from each timestep should enter the average to sample also high-frequency flux contributions (choose dt_averaging_input small enough). |
vw_product | m2 s-2 | product of v and w To be used for calculation of resolved-scale transport <v'w'> in case of horizontal inhomogeneity. Output is defined on v-grid. Therefore, output of vw is not necessarily identical to output of wv. Output of both quantities, however, can be useful for computation of spatial flux gradients. Computation of <v'w'> is possible in post-processing via temporal EC-method, i.e. <v'w'> = <vw> - <v><w>, with < > being the temporal average. For accurate flux calculation the time averaging needs to be sufficiently long (usually 30min) and data from each timestep should enter the average to sample also high-frequency flux contributions (choose dt_averaging_input small enough). |
w | m s-1 | w-component of velocity vector |
wdir | degree | direction of horizontal wind vector |
wq_product | kg kg-1 m s-1 | product of w and q To be used for calculation of resolved-scale transport <w'q'> in case of horizontal inhomogeneity. Output is defined on w-grid. Requires humidity = .T.. Computation of <w'q'> is possible in post-processing via temporal EC-method, i.e. <w'q'> = <wq> - <w><q>, with < > being the temporal average. For accurate flux calculation the time averaging needs to be sufficiently long (usually 30min) and data from each timestep should enter the average to sample also high-frequency flux contributions (choose dt_averaging_input small enough). |
wspeed | m s-1 | magnitude of the horizontal wind vector |
ws_product | m s-1 | product of w and s To be used for calculation of resolved-scale transport <w's'> in case of horizontal inhomogeneity. Output is defined on w-grid. Computation of <w's'> is possible in post-processing via temporal EC-method, i.e. <w's'> = <ws> - <w><s>, with < > being the temporal average. For accurate flux calculation the time averaging needs to be sufficiently long (usually 30min) and data from each timestep should enter the average to sample also high-frequency flux contributions (choose dt_averaging_input small enough). Requires passive_scalar = .T.. |
wtheta_product | K m s-1 | product of w and theta To be used for calculation of resolved-scale transport <w'theta'> in case of horizontal inhomogeneity. Output is defined on w-grid. Computation of <w'theta'> is possible in post-processing via temporal EC-method, i.e. <w'theta'> = <wtheta> - <w><theta>, with < > being the temporal average. For accurate flux calculation the time averaging needs to be sufficiently long (usually 30min) and data from each timestep should enter the average to sample also high-frequency flux contributions (choose dt_averaging_input small enough). |
wu_product | m2 s-2 | product of w and u To be used for calculation of resolved-scale transport <w'u'> in case of horizontal inhomogeneity. Output is defined on w-grid. Therefore, output of wu is not necessarily identical to output of uw. Output of both quantities, however, can be useful for computation of spatial flux gradients. Computation of <w'u'> is possible in post-processing via temporal EC-method, i.e. <w'u'> = <wu> - <w><u>, with < > being the temporal average. For accurate flux calculation the time averaging needs to be sufficiently long (usually 30min) and data from each timestep should enter the average to sample also high-frequency flux contributions (choose dt_averaging_input small enough). |
wv_product | m2 s-2 | product of w and v To be used for calculation of resolved-scale transport <w'v'> in case of horizontal inhomogeneity. Output is defined on w-grid. Therefore, output of wv is not necessarily identical to output of vw. Output of both quantities, however, can be useful for computation of spatial flux gradients. Computation of <w'v'> is possible in post-processing via temporal EC-method, i.e. <w'v'> = <wv> - <w><v>, with < > being the temporal average. For accurate flux calculation the time averaging needs to be sufficiently long (usually 30min) and data from each timestep should enter the average to sample also high-frequency flux contributions (choose dt_averaging_input small enough). |
ww_product | m2 s-2 | product of w and w To be used for calculation of resolved-scale transport <w'w'> in case of horizontal inhomogeneity. Output is defined on w-grid. Computation of <w'w'> is possible in post-processing via temporal EC-method, i.e. <w'w'> = <ww> - <w><w>, with < > being the temporal average. For accurate flux calculation the time averaging needs to be sufficiently long (usually 30min) and data from each timestep should enter the average to sample also high-frequency flux contributions (choose dt_averaging_input small enough). |
Masked array quantities#
Name | SI-Unit | Description |
---|---|---|
e | m2 s-2 | SGS turbulence kinetic energy |
kc_X | ppm or kg m-3 | concentration of chemical species X Chemistry quantities requires the prefix kc_. X indicates the species name. Only species names belonging to the selected chemistry mechanism are allowed. |
nr | m-3 | rain drop number density Requires cloud_scheme = 'seifert_beheng'. |
p | Pa | perturbation pressure |
pc | number per gridbox | particle/droplet concentration |
pr | m | mean particle/droplet radius |
q | kg kg-1 | water vapor mixing ratio (or total water mixing ratio if cloud physics is switched on) Requires humidity = .T.. |
qc | kg kg-1 | cloud water mixing ratio Requires cloud_scheme = 'seifert_beheng' or 'morrison'. |
ql | kg kg-1 | liquid water mixing ratio Requires using the bulk cloud model (BCM) or the Lagrangian cloud model (LCM) via setting of cloud_droplets = .T.. |
ql_c | kg kg-1 | change in liquid water mixing ratio due to condensation/evaporation during last time step Requires to switch on the Lagrangian cloud model (LCM) via setting of cloud_droplets = .T.. |
ql_v | m3 per gridpox | volume of liquid water Requires to switch on the Lagrangian cloud model (LCM) via setting of cloud_droplets = .T.. |
ql_vp | 1 | weighting factor Requires to switch on the Lagrangian cloud model (LCM) via setting of cloud_droplets = .T.. |
qr | kg kg-1 | rain water mixing ratio Requires cloud_scheme = 'seifert_beheng'. |
qv | kg kg-1 | water vapor mixing ratio Requires using the bulk cloud model (BCM). |
rho_sea_water | kg m-3 | density of sea water Requires ocean module switched on. |
s | kg m-3 or ppm | concentration of passive scalar Requires passive_scalar = .T.. |
sa | psu | salinity of sea water Requires ocean module switched on. |
ta | °C | true air temperature |
theta | K | potential temperature |
thetal | K | liquid water potential temperature Requires using the bulk cloud model (BCM). |
thetav | K | virtual potential temperature Requires humidity = .T.. |
ti | s-1 | curl of velocity vector (magnitude) |
u | m s-1 | u-component of velocity vector |
v | m s-1 | v-component of velocity vector |
w | m s-1 | w-component of velocity vector |
wdir | degree | direction of horizontal wind vector |
wspeed | m s-1 | magnitude of the horizontal wind vector |
2d-array quantities#
Name | SI-Unit | Description |
---|---|---|
c_liq* | % | coverage of plants with liquid water |
c_soil* | % | coverage of the land surface with bare soil |
c_vef* | % | coverage of the land surface with vegetation |
dust_depo_flux*_bin<b> | kg m-2 s-1 | surface deposition flux of a dust size bin <d> is one of the dust size bin numbers: 1, 2, 3, ... . |
dust_emis_flux*_bin<b> | kg m-2 s-1 | surface emission flux of a dust size bin <d> is one of the dust size bin numbers: 1, 2, 3, ... . |
ghf* | W m-2 | ground (soil) heat flux From energy balance. |
kfd* | m | katabatic flow depth Indicates the top of a katabatic flow characterized by a jet-like structure. To detect a katabatic flow and determine its depth, the flow must show an elevated maximum of shear production and must be roughly aligned with the terrain-slope. |
lai | m2 m-2 | leaf area index |
lwp* | kg m-2 | liquid water path |
m_liq* | m | liquid water level on plants |
ol* | m | Obukhov length in the constant flux layer |
pra* | mm | precipitation amount Requires cloud_scheme = 'kessler' or 'seifert_beheng'. Time interval to which amount refers to is defined by precipitation_amount_interval. |
qsurf* | kg kg-1 | mixing ratio at the surface |
qsws* | kg kg-1 m s-1 or W m-2 | surface latent heatflux Requires humidity = .T.. |
qsws_liq* | W m-2 | surface latent heat flux due to evaporation/condensation of liquid water on plants From energy balance. |
qsws_soil* | W m-2 | surface latent heat flux due to evaporation/precipitation of bare soil From energy balance. |
qsws_veg* | W m-2 | surface latent heat flux due to transpiration of plants From energy balance. |
qv_2m* | kg kg-1 | 2-m water vapor mixing ratio Requires using the buld cloud model. See also description of theta_2m*. |
rad_lw_in* | W m-2 | incoming longwave radiation flux |
rad_lw_out* | W m-2 | outgoing longwave radiation flux |
rad_sw_in* | W m-2 | incoming shortwave radiation flux |
rad_sw_out* | W m-2 | outgoing shortwave radiation flux |
rad_net* | W m-2 | net radiation flux at the surface |
r_a* | s m-1 | aerodynamic resistance |
r_s* | s m-1 | resistance of the surface Soil plus vegetation. |
shf* | K m s-1 or W m-2 | surface sensible heat flux |
slurb_albedo_urb* | 1 | effective urban shortwave albedo |
slurb_c_liq_road* | % | liquid water coverage on the road Requires humidity = .T. and moist_physics = .T.. |
slurb_c_liq_roof* | % | liquid water coverage on the roof Requires humidity = .T. and moist_physics = .T.. |
slurb_emiss_urb* | 1 | effective urban longwave emissivity |
slurb_ghf_road* | K m s-1 or W m-2 | ground heat flux from the road to deep soil |
slurb_ghf_roof* | K m s-1 or W m-2 | ground heat flux from the roof to building indoor air |
slurb_ghf_wall_a* | K m s-1 or W m-2 | ground heat flux from the wall A to building indoor air |
slurb_ghf_wall_b* | K m s-1 or W m-2 | ground heat flux from the wall B to building indoor air Same as slurb_ghf_wall_a* if anisotropic_street_canyons = .F.. |
slurb_ghf_win_a* | K m s-1 or W m-2 | ground heat flux from the window A to building indoor air |
slurb_ghf_win_b* | K m s-1 or W m-2 | ground heat flux from the window B to building indoor air Same as slurb_ghf_wall_b* if anisotropic_street_canyons = .F.. |
slurb_m_liq_road* | m | liquid water reservoir on the road Requires humidity = .T. and moist_physics = .T.. |
slurb_m_liq_roof* | m | liquid water reservoir on the roof Requires humidity = .T. and moist_physics = .T.. |
slurb_ol_canyon* | m | Obukhov length for the constant flux layer between the street canyon air and the first atmospheric grid level |
slurb_ol_road* | m | Obukhov length for the constant flux layer between the road surface and the street canyon air |
slurb_ol_roof* | m | Obukhov length for the constant flux layer between the roof surface and the first atmospheric grid level |
slurb_ol_urb* | m | Obukhov length for the constant flux layer between the urban surface and the first atmospheric grid level Used to compute the momentum flux for aggregate urban surface. |
slurb_q_canyon* | kg kg-1 | mixing ratio of the street canyon air Requires humidity = .T. and moist_physics = .T.. |
slurb_q_road* | kg kg-1 | mixing ratio at the road surface Requires humidity = .T. and moist_physics = .T.. |
slurb_q_roof* | kg kg-1 | mixing ratio at the roof surface Requires humidity = .T. and moist_physics = .T.. |
slurb_qs_road* | kg kg-1 | saturation mixing ratio at the road surface Requires humidity = .T. and moist_physics = .T.. |
slurb_qs_roof* | kg kg-1 | saturation mixing ratio at the roof surface Requires humidity = .T. and moist_physics = .T.. |
slurb_qsws_canyon* | kg kg-1 m s-1 or W m-2 | latent heat flux from the roof to the first atmospheric grid level Requires humidity = .T. and moist_physics = .T.. |
slurb_qsws_road* | kg kg-1 m s-1 or W m-2 | latent heat flux from the road surface to street canyon air Requires humidity = .T. and moist_physics = .T.. |
slurb_qsws_lsm* | kg kg-1 m s-1 or W m-2 | latent heat flux from natural surfaces to the first atmospheric grid level as modelled by PALM-LSM With SLUrb enabled, the surface latent heat flux output qsws* becomes the aggregated flux from both urban and natural surfaces. With slurb_qsws_urb* and slurb_qsws_lsm*, it is possible to output the urban and natural partitions separately. The output is not weighted by surface fraction. Requires humidity = .T. and moist_physics = .T.. |
slurb_qsws_urb* | kg kg-1 m s-1 or W m-2 | latent heat flux from urban surfaces to the first atmospheric grid level as modelled by PALM-LSM With SLUrb enabled, the surface latent heat flux output qsws* becomes the aggregated flux from both urban and natural surfaces. With slurb_qsws_urb* and slurb_qsws_lsm*, it is possible to output the urban and natural partitions separately. The output is not weighted by surface fraction. Requires humidity = .T. and moist_physics = .T.. |
slurb_rad_lw_net_road* | W m-2 | net longwave radiation flux at the road surface |
slurb_rad_lw_net_roof* | W m-2 | net longwave radiation flux at the roof surface |
slurb_rad_lw_net_urb* | W m-2 | aggregated net longwave radiation flux of the urban surface |
slurb_rad_lw_net_wall_a* | W m-2 | net longwave radiation flux at the wall A surface |
slurb_rad_lw_net_wall_b* | W m-2 | net longwave radiation flux at the wall B surface Same as slurb_rad_lw_net_wall_a* if anisotropic_street_canyons = .F.. |
slurb_rad_lw_net_win_a* | W m-2 | net longwave radiation flux at the window A surface |
slurb_rad_lw_net_win_b* | W m-2 | net longwave radiation flux at the window B surface Same as slurb_rad_lw_net_win_a* if anisotropic_street_canyons = .F.. |
slurb_rad_sw_net_roof* | W m-2 | net shortwave radiation flux at the roof surface |
slurb_rad_sw_net_urb* | W m-2 | aggregated net shortwave radiation flux of the urban surface |
slurb_rad_sw_net_wall_a* | W m-2 | net shortwave radiation flux at the wall A surface |
slurb_rad_sw_net_wall_b* | W m-2 | net shortwave radiation flux at the wall B surface Same as slurb_rad_sw_net_wall_a* if anisotropic_street_canyons = .F.. |
slurb_rad_sw_net_win_a* | W m-2 | net shortwave radiation flux at the window A surface |
slurb_rad_sw_net_win_b* | W m-2 | net shortwave radiation flux at the window B surface Same as slurb_rad_sw_net_win_a* if anisotropic_street_canyons = .F.. |
slurb_rad_sw_net_road* | W m-2 | net shortwave radiation flux at the road surface |
slurb_rad_sw_tr_win_a* | W m-2 | transmitted shortwave radiation flux through the window A to building indoor air |
slurb_rad_sw_tr_win_b* | W m-2 | transmitted shortwave radiation flux through the window B to building indoor air Same as slurb_rad_sw_tr_win_a* if anisotropic_street_canyons = .F.. |
slurb_rah_canyon* | s m-1 | aerodynamic resistance for heat for the constant flux layer between the street canyon air and the first atmospheric grid level |
slurb_rah_facade* | s m-1 | aerodynamic resistance for heat between a facade surface and the street canyon air Available only if facade_resistance_parametrization is either 'krayenhoff&voogt' or 'rowley'. These parametrizations do not differentiate between wall and window surfaces or facade A and B. |
slurb_rah_road* | s m-1 | aerodynamic resistance for heat for the constant flux layer between the road surface and the street canyon air |
slurb_rah_roof* | s m-1 | aerodynamic resistance for heat for the constant flux layer between the road surface and the street canyon air |
slurb_rah_wall_a* | s m-1 | aerodynamic resistance for heat between the wall A surface and the street canyon air Available only if facade_resistance_parametrization is 'doe-2'. |
slurb_rah_wall_b* | s m-1 | aerodynamic resistance for heat between the wall B surface and the street canyon air Available only if facade_resistance_parametrization is 'doe-2'. |
slurb_rah_win_a* | s m-1 | aerodynamic resistance for heat between the window A surface and the street canyon air Available only if facade_resistance_parametrization is 'doe-2'. |
slurb_rah_win_b* | s m-1 | aerodynamic resistance for heat between the window B surface and the street canyon air Available only if facade_resistance_parametrization is 'doe-2'. |
slurb_ram_urb* | s m-1 | aerodynamic resistance for momentum for the constant flux layer between the urban surface and the first atmospheric grid level Used to compute the momentum flux for aggregate urban surface. |
slurb_rib_canyon* | s m-1 | bulk Richardson number for the constant flux layer between the street canyon air and the first atmospheric grid level |
slurb_rib_road* | s m-1 | bulk Richardson number for heat for the constant flux layer between the roof surface and the street canyon air |
slurb_shf_canyon* | K m s-1 or W m-2 | sensible heat flux from the street canyon air to the first atmospheric grid level |
slurb_shf_external* | K m s-1 or W m-2 | sensible heat flux from external sources to the first atmospheric grid level |
slurb_shf_road* | K m s-1 or W m-2 | sensible heat flux from the road to the street canyon air |
slurb_shf_roof* | K m s-1 or W m-2 | sensible heat flux from the roof to the first atmospheric grid level |
slurb_shf_traffic* | K m s-1 or W m-2 | sensible heat flux from traffic to the street canyon air |
slurb_shf_lsm* | K m s-1 or W m-2 | sensible heat flux from natural surfaces to the first atmospheric grid level With SLUrb enabled, the surface latent heat flux output shf* becomes the aggregated flux from both urban and natural surfaces. With slurb_shf_urb* and slurb_shf_lsm*, it is possible to output the urban and natural partitions separately. |
slurb_shf_urb* | K m s-1 or W m-2 | sensible heat flux from urban surfaces to the first atmospheric grid level With SLUrb enabled, the surface latent heat flux output shf* becomes the aggregated flux from both urban and natural surfaces. With slurb_shf_urb* and slurb_shf_lsm*, it is possible to output the urban and natural partitions separately. |
slurb_shf_wall_a* | K m s-1 or W m-2 | sensible heat flux from the wall A to the street canyon air |
slurb_shf_wall_b* | K m s-1 or W m-2 | sensible heat flux from the wall B to the street canyon air Same as slurb_shf_wall_a* if anisotropic_street_canyons = .F.. |
slurb_shf_win_a* | K m s-1 or W m-2 | sensible heat flux from the window A to the street canyon air |
slurb_shf_win_b* | K m s-1 or W m-2 | sensible heat flux from the window B to the street canyon air Same as slurb_shf_win_a* if anisotropic_street_canyons = .F.. |
slurb_t_canyon* | K | street canyon air temperature Defined at street canyon half-height. |
slurb_t_rad_urb* | K | radiative temperature of the urban surface Computed from outgoing longwave radiation and effective urban surface temperature. |
slurb_t_surf_road* | K | road surface temperature |
slurb_t_surf_roof* | K | roof surface temperature |
slurb_t_surf_wall_a* | K | wall A surface temperature |
slurb_t_surf_wall_b* | K | wall B surface temperature Same as slurb_t_surf_wall_a* if anisotropic_street_canyons = .F.. |
slurb_t_surf_win_a* | K | window A surface temperature |
slurb_t_surf_win_b* | K | window B surface temperature Same as slurb_t_surf_win_a* if anisotropic_street_canyons = .F.. |
slurb_t_c_urb* | K | complete urban surface temperature Urban surface temperature computed by area-weighting of surface temperatures from roof, walls, windows and road. |
slurb_t_h_urb* | K | effective urban surface temperature Urban surface temperature based on conservation of local heat flux contributions of surfaces. |
slurb_t_2m_urb* | K | urban 2-meter air temperature Diagnostic urban 2-meter air temperature using stability-corrected logarithmic extrapolation from the first atmospheric grid level. Extrapolation typically underestimates the true air temperature within the urban canopy during daytime. |
slurb_theta_canyon* | K | street canyon air potential temperature Defined at street canyon half-height. |
slurb_theta_road* | K | road surface potential temperature |
slurb_theta_roof* | K | roof surface potential temperature |
slurb_theta_wall_a* | K | wall A surface potential temperature |
slurb_theta_wall_b* | K | wall B surface potential temperature Same as slurb_theta_wall_a* if anisotropic_street_canyons = .F.. |
slurb_theta_win_a* | K | window A surface potential temperature |
slurb_theta_win_b* | K | window B surface potential temperature Same as slurb_theta_win_a* if anisotropic_street_canyons = .F.. |
slurb_thetav_canyon* | K | street canyon air virtual potential temperature Defined at street canyon half-height. Requires humidity = .T. and moist_physics = .T.. |
slurb_thetav_road* | K | road surface virtual potential temperature Requires humidity = .T. and moist_physics = .T.. |
slurb_thetav_roof* | K | roof surface virtual potential temperature Requires humidity = .T. and moist_physics = .T.. |
slurb_wspeed_canyon* | m s-1 | street canyon horizontal wind speed Defined at street canyon half-height. |
slurb_wspeed_eff_canyon* | m s-1 | street canyon effective horizontal wind speed Defined at street canyon half-height. Includes the effect of turbulent and convective velocity scales. |
slurb_us_canyon* | m s-1 | friction velocity in the constant flux layer between the street canyon air and the first atmospheric grid level |
slurb_us_road* | m s-1 | friction velocity in the constant flux layer between the road surface and the street canyon air |
slurb_us_roof* | m s-1 | friction velocity in the constant flux layer between the roof surface and the first atmospheric grid level |
slurb_us_urb* | m s-1 | friction velocity in the constant flux layer between the urban surface and the first atmospheric grid level Computed for the aggregate urban surface. |
slurb_usws_urb* | m-2 s-2 | u-component of the urban vertical turbulent momentum flux Computed for the aggregate urban surface. |
slurb_vsws_urb* | m-2 s-2 | v-component of the urban vertical turbulent momentum flux Computed for the aggregate urban surface. |
ssurf* | kg kg-1 | surface scalar concentration Requires passive_scalar = .T.. |
ssws* | kg m-2 s-1 or ppm m s-1 | surface scalarflux Requires passive_scalar = .T.. |
t* | K | (near surface) characteristic temperature |
ta_2m* | °C | true air temperature at 2m above surface Estimated from logarithmic interpolation if the 2m level is below the first prognostic grid point, else interpolated between two vertical levels. |
theta_2m* | K | potential temperature at 2m above surface Estimated from logarithmic interpolation if the 2m level is below the first prognostic grid point, else interpolated between two vertical levels. |
tsurf* | K | surface temperature |
us* | m s-1 | (near surface) friction velocity |
uv_ewir1* | mW m-2 | wavelength integrated and erythemally weighted UV irradiance The UV radiance is calculated based on a sky-view factor approach (LOD1). Requires setting of parameter uv_integration_method = 'from_irradiance'. |
uv_ewir2* | mW m-2 | wavelength integrated and erythemally weighted UV irradiance The UV radiance is calculated based on a spherical obstruction approach (LOD2). Requires setting of parameter uv_integration_method = 'from_radiance'. |
uv_ir1* | W m-2 | wavelength integrated UV irradiance The UV radiance is calculated based on a sky-view factor approach (LOD1). Requires setting of parameter uv_integration_method = 'from_irradiance'. |
uv_ir2* | W m-2 | wavelength integrated UV irradiance The UV radiance is calculated based on a spherical obstruction approach (LOD2). Requires setting of parameter uv_integration_method = 'from_radiance'. |
vf25m* | m3 s-1 | volume-flux rate integrated up to 25m above surface |
vf50m* | m3 s-1 | volume-flux rate integrated up to 50m above surface |
vf75m* | m3 s-1 | volume-flux rate integrated up to 75m above surface |
vf100m* | m3 s-1 | volume-flux rate integrated up to 100m above surface |
vfxxm* | m3 s-1 | volume-flux rate integrated up to detected katabatic flow depth See also remarks for kfd*. |
vfd25m* | m3 m-1 s-1 | volume-flux density integrated up to 25m above surface Volume flux per second through a 1m wide column with height of 25m. |
vfd50m* | m3 m-1 s-1 | volume-flux density integrated up to 50m above surface Volume flux per second through a 1m wide column with height of 50m. |
vfd75m* | m3 m-1 s-1 | volume-flux density integrated up to 75m above surface Volume flux per second through a 1m wide column with height of 75m. |
vfd100m* | m3 m-1 s-1 | volume-flux density integrated up to 100m above surface Volume flux per second through a 1m wide column with height of 100m. |
vfdxxm* | m3 m-1 s-1 | volume-flux density integrated up to detected katabatic flow depth Volume flux per second through a 1m wide column with height of 75m. See also remarks for kfd*. |
wdir_10m* | degree | direction of horizontal wind vector at 10 m above surface Calculated based on the horizontal wind vector components, which are estimated from logarithmic interpolation if the 10m level is below the first prognostic grid point, else interpolated between two vertical levels. |
wspeed_10m* | m s-1 | 10-m wind speed Estimated from logarithmic interpolation if the 10m level is below the first prognostic grid point, else interpolated between two vertical levels. |
z0* | m | roughness length |
z0h* | m | roughness length for scalar quantities |
DET quantities#
Name | SI-Unit | Description |
---|---|---|
clay | kg m-3 | mass concentration of clay-sized particles Particles with a diameter less than or equal to 4.0E-6 m are considered |
dust | kg m-3 | mass concentration of dust-sized particles Particles with a diameter less than or equal to 63.0E-6 m are considered |
dust_depo_flux*_bin<b> | kg m-2 s-1 | surface deposition flux of a dust size bin <d> is one of the dust size bin numbers: 1, 2, 3, ... . |
dust_emis_flux*_bin<b> | kg m-2 s-1 | surface emission flux of a dust size bin <d> is one of the dust size bin numbers: 1, 2, 3, ... . |
dust_mc_bin<b> | kg m-3 | mass concentration of a dust size bin <d> is one of the dust size bin numbers: 1, 2, 3, ... . |
silt | kg m-3 | mass concentration of silt-sized particles Particles with a diameter greater than 4.0E-6 m and less than or equal to 63.0E-6 m are considered |
SLUrb quantities#
Name | SI-Unit | Description |
---|---|---|
slurb_albedo_urb* | 1 | effective urban shortwave albedo |
slurb_c_liq_road* | % | liquid water coverage on the road Requires humidity = .T. and moist_physics = .T.. |
slurb_c_liq_roof* | % | liquid water coverage on the roof Requires humidity = .T. and moist_physics = .T.. |
slurb_emiss_urb* | 1 | effective urban longwave emissivity |
slurb_ghf_road* | K m s-1 or W m-2 | ground heat flux from the road to deep soil |
slurb_ghf_roof* | K m s-1 or W m-2 | ground heat flux from the roof to building indoor air |
slurb_ghf_wall_a* | K m s-1 or W m-2 | ground heat flux from the wall A to building indoor air |
slurb_ghf_wall_b* | K m s-1 or W m-2 | ground heat flux from the wall B to building indoor air Same as slurb_ghf_wall_a* if anisotropic_street_canyons = .F.. |
slurb_ghf_win_a* | K m s-1 or W m-2 | ground heat flux from the window A to building indoor air |
slurb_ghf_win_b* | K m s-1 or W m-2 | ground heat flux from the window B to building indoor air Same as slurb_ghf_wall_b* if anisotropic_street_canyons = .F.. |
slurb_m_liq_road* | m | liquid water reservoir on the road Requires humidity = .T. and moist_physics = .T.. |
slurb_m_liq_roof* | m | liquid water reservoir on the roof Requires humidity = .T. and moist_physics = .T.. |
slurb_ol_canyon* | m | Obukhov length for the constant flux layer between the street canyon air and the first atmospheric grid level |
slurb_ol_road* | m | Obukhov length for the constant flux layer between the road surface and the street canyon air |
slurb_ol_roof* | m | Obukhov length for the constant flux layer between the roof surface and the first atmospheric grid level |
slurb_ol_urb* | m | Obukhov length for the constant flux layer between the urban surface and the first atmospheric grid level Used to compute the momentum flux for aggregate urban surface. |
slurb_q_canyon* | kg kg-1 | mixing ratio of the street canyon air Requires humidity = .T. and moist_physics = .T.. |
slurb_q_road* | kg kg-1 | mixing ratio at the road surface Requires humidity = .T. and moist_physics = .T.. |
slurb_q_roof* | kg kg-1 | mixing ratio at the roof surface Requires humidity = .T. and moist_physics = .T.. |
slurb_qs_road* | kg kg-1 | saturation mixing ratio at the road surface Requires humidity = .T. and moist_physics = .T.. |
slurb_qs_roof* | kg kg-1 | saturation mixing ratio at the roof surface Requires humidity = .T. and moist_physics = .T.. |
slurb_qsws_canyon* | kg kg-1 m s-1 or W m-2 | latent heat flux from the roof to the first atmospheric grid level Requires humidity = .T. and moist_physics = .T.. |
slurb_qsws_road* | kg kg-1 m s-1 or W m-2 | latent heat flux from the road surface to street canyon air Requires humidity = .T. and moist_physics = .T.. |
slurb_qsws_lsm* | kg kg-1 m s-1 or W m-2 | latent heat flux from natural surfaces to the first atmospheric grid level as modelled by PALM-LSM With SLUrb enabled, the surface latent heat flux output qsws* becomes the aggregated flux from both urban and natural surfaces. With slurb_qsws_urb* and slurb_qsws_lsm*, it is possible to output the urban and natural partitions separately. The output is not weighted by surface fraction. Requires humidity = .T. and moist_physics = .T.. |
slurb_qsws_urb* | kg kg-1 m s-1 or W m-2 | latent heat flux from urban surfaces to the first atmospheric grid level as modelled by PALM-LSM With SLUrb enabled, the surface latent heat flux output qsws* becomes the aggregated flux from both urban and natural surfaces. With slurb_qsws_urb* and slurb_qsws_lsm*, it is possible to output the urban and natural partitions separately. The output is not weighted by surface fraction. Requires humidity = .T. and moist_physics = .T.. |
slurb_rad_lw_net_road* | W m-2 | net longwave radiation flux at the road surface |
slurb_rad_lw_net_roof* | W m-2 | net longwave radiation flux at the roof surface |
slurb_rad_lw_net_urb* | W m-2 | aggregated net longwave radiation flux of the urban surface |
slurb_rad_lw_net_wall_a* | W m-2 | net longwave radiation flux at the wall A surface |
slurb_rad_lw_net_wall_b* | W m-2 | net longwave radiation flux at the wall B surface Same as slurb_rad_lw_net_wall_a* if anisotropic_street_canyons = .F.. |
slurb_rad_lw_net_win_a* | W m-2 | net longwave radiation flux at the window A surface |
slurb_rad_lw_net_win_b* | W m-2 | net longwave radiation flux at the window B surface Same as slurb_rad_lw_net_win_a* if anisotropic_street_canyons = .F.. |
slurb_rad_sw_net_roof* | W m-2 | net shortwave radiation flux at the roof surface |
slurb_rad_sw_net_urb* | W m-2 | aggregated net shortwave radiation flux of the urban surface |
slurb_rad_sw_net_wall_a* | W m-2 | net shortwave radiation flux at the wall A surface |
slurb_rad_sw_net_wall_b* | W m-2 | net shortwave radiation flux at the wall B surface Same as slurb_rad_sw_net_wall_a* if anisotropic_street_canyons = .F.. |
slurb_rad_sw_net_win_a* | W m-2 | net shortwave radiation flux at the window A surface |
slurb_rad_sw_net_win_b* | W m-2 | net shortwave radiation flux at the window B surface Same as slurb_rad_sw_net_win_a* if anisotropic_street_canyons = .F.. |
slurb_rad_sw_net_road* | W m-2 | net shortwave radiation flux at the road surface |
slurb_rad_sw_tr_win_a* | W m-2 | transmitted shortwave radiation flux through the window A to building indoor air |
slurb_rad_sw_tr_win_b* | W m-2 | transmitted shortwave radiation flux through the window B to building indoor air Same as slurb_rad_sw_tr_win_a* if anisotropic_street_canyons = .F.. |
slurb_rah_canyon* | s m-1 | aerodynamic resistance for heat for the constant flux layer between the street canyon air and the first atmospheric grid level |
slurb_rah_facade* | s m-1 | aerodynamic resistance for heat between a facade surface and the street canyon air Available only if facade_resistance_parametrization is either 'krayenhoff&voogt' or 'rowley'. These parametrizations do not differentiate between wall and window surfaces or facade A and B. |
slurb_rah_road* | s m-1 | aerodynamic resistance for heat for the constant flux layer between the road surface and the street canyon air |
slurb_rah_roof* | s m-1 | aerodynamic resistance for heat for the constant flux layer between the road surface and the street canyon air |
slurb_rah_wall_a* | s m-1 | aerodynamic resistance for heat between the wall A surface and the street canyon air Available only if facade_resistance_parametrization is 'doe-2'. |
slurb_rah_wall_b* | s m-1 | aerodynamic resistance for heat between the wall B surface and the street canyon air Available only if facade_resistance_parametrization is 'doe-2'. |
slurb_rah_win_a* | s m-1 | aerodynamic resistance for heat between the window A surface and the street canyon air Available only if facade_resistance_parametrization is 'doe-2'. |
slurb_rah_win_b* | s m-1 | aerodynamic resistance for heat between the window B surface and the street canyon air Available only if facade_resistance_parametrization is 'doe-2'. |
slurb_ram_urb* | s m-1 | aerodynamic resistance for momentum for the constant flux layer between the urban surface and the first atmospheric grid level Used to compute the momentum flux for aggregate urban surface. |
slurb_rib_canyon* | s m-1 | bulk Richardson number for the constant flux layer between the street canyon air and the first atmospheric grid level |
slurb_rib_road* | s m-1 | bulk Richardson number for heat for the constant flux layer between the roof surface and the street canyon air |
slurb_shf_canyon* | K m s-1 or W m-2 | sensible heat flux from the street canyon air to the first atmospheric grid level |
slurb_shf_external* | K m s-1 or W m-2 | sensible heat flux from external sources to the first atmospheric grid level |
slurb_shf_road* | K m s-1 or W m-2 | sensible heat flux from the road to the street canyon air |
slurb_shf_roof* | K m s-1 or W m-2 | sensible heat flux from the roof to the first atmospheric grid level |
slurb_shf_traffic* | K m s-1 or W m-2 | sensible heat flux from traffic to the street canyon air |
slurb_shf_lsm* | K m s-1 or W m-2 | sensible heat flux from natural surfaces to the first atmospheric grid level With SLUrb enabled, the surface latent heat flux output shf* becomes the aggregated flux from both urban and natural surfaces. With slurb_shf_urb* and slurb_shf_lsm*, it is possible to output the urban and natural partitions separately. |
slurb_shf_urb* | K m s-1 or W m-2 | sensible heat flux from urban surfaces to the first atmospheric grid level With SLUrb enabled, the surface latent heat flux output shf* becomes the aggregated flux from both urban and natural surfaces. With slurb_shf_urb* and slurb_shf_lsm*, it is possible to output the urban and natural partitions separately. |
slurb_shf_wall_a* | K m s-1 or W m-2 | sensible heat flux from the wall A to the street canyon air |
slurb_shf_wall_b* | K m s-1 or W m-2 | sensible heat flux from the wall B to the street canyon air Same as slurb_shf_wall_a* if anisotropic_street_canyons = .F.. |
slurb_shf_win_a* | K m s-1 or W m-2 | sensible heat flux from the window A to the street canyon air |
slurb_shf_win_b* | K m s-1 or W m-2 | sensible heat flux from the window B to the street canyon air Same as slurb_shf_win_a* if anisotropic_street_canyons = .F.. |
slurb_t_canyon* | K | street canyon air temperature Defined at street canyon half-height. |
slurb_t_rad_urb* | K | radiative temperature of the urban surface Computed from outgoing longwave radiation and effective urban surface temperature. |
slurb_t_surf_road* | K | road surface temperature |
slurb_t_surf_roof* | K | roof surface temperature |
slurb_t_surf_wall_a* | K | wall A surface temperature |
slurb_t_surf_wall_b* | K | wall B surface temperature Same as slurb_t_surf_wall_a* if anisotropic_street_canyons = .F.. |
slurb_t_surf_win_a* | K | window A surface temperature |
slurb_t_surf_win_b* | K | window B surface temperature Same as slurb_t_surf_win_a* if anisotropic_street_canyons = .F.. |
slurb_t_c_urb* | K | complete urban surface temperature Urban surface temperature computed by area-weighting of surface temperatures from roof, walls, windows and road. |
slurb_t_h_urb* | K | effective urban surface temperature Urban surface temperature based on conservation of local heat flux contributions of surfaces. |
slurb_t_2m_urb* | K | urban 2-meter air temperature Diagnostic urban 2-meter air temperature using stability-corrected logarithmic extrapolation from the first atmospheric grid level. Extrapolation typically underestimates the true air temperature within the urban canopy during daytime. |
slurb_theta_canyon* | K | street canyon air potential temperature Defined at street canyon half-height. |
slurb_theta_road* | K | road surface potential temperature |
slurb_theta_roof* | K | roof surface potential temperature |
slurb_theta_wall_a* | K | wall A surface potential temperature |
slurb_theta_wall_b* | K | wall B surface potential temperature Same as slurb_theta_wall_a* if anisotropic_street_canyons = .F.. |
slurb_theta_win_a* | K | window A surface potential temperature |
slurb_theta_win_b* | K | window B surface potential temperature Same as slurb_theta_win_a* if anisotropic_street_canyons = .F.. |
slurb_thetav_canyon* | K | street canyon air virtual potential temperature Defined at street canyon half-height. Requires humidity = .T. and moist_physics = .T.. |
slurb_thetav_road* | K | road surface virtual potential temperature Requires humidity = .T. and moist_physics = .T.. |
slurb_thetav_roof* | K | roof surface virtual potential temperature Requires humidity = .T. and moist_physics = .T.. |
slurb_wspeed_canyon* | m s-1 | street canyon horizontal wind speed Defined at street canyon half-height. |
slurb_wspeed_eff_canyon* | m s-1 | street canyon effective horizontal wind speed Defined at street canyon half-height. Includes the effect of turbulent and convective velocity scales. |
slurb_us_canyon* | m s-1 | friction velocity in the constant flux layer between the street canyon air and the first atmospheric grid level |
slurb_us_road* | m s-1 | friction velocity in the constant flux layer between the road surface and the street canyon air |
slurb_us_roof* | m s-1 | friction velocity in the constant flux layer between the roof surface and the first atmospheric grid level |
slurb_us_urb* | m s-1 | friction velocity in the constant flux layer between the urban surface and the first atmospheric grid level Computed for the aggregate urban surface. |
slurb_usws_urb* | m-2 s-2 | u-component of the urban vertical turbulent momentum flux Computed for the aggregate urban surface. |
slurb_vsws_urb* | m-2 s-2 | v-component of the urban vertical turbulent momentum flux Computed for the aggregate urban surface. |
slurb_t_road | K | road layer temperature |
slurb_t_roof | K | roof layer temperature |
slurb_t_wall_a | K | wall A layer temperature |
slurb_t_wall_b | K | wall A layer temperature Same as slurb_t_wall_a if anisotropic_street_canyons = .F.. |
slurb_t_win_a | K | window A layer temperature |
slurb_t_win_b | K | window A layer temperature Same as slurb_t_win_a if anisotropic_street_canyons = .F.. |
UV quantities#
Name | SI-Unit | Description |
---|---|---|
uv_ewir1* | mW m-2 | wavelength integrated and erythemally weighted UV irradiance The UV radiance is calculated based on a sky-view factor approach (LOD1). Requires setting of parameter uv_integration_method = 'from_irradiance'. |
uv_ewir2* | mW m-2 | wavelength integrated and erythemally weighted UV irradiance The UV radiance is calculated based on a spherical obstruction approach (LOD2). Requires setting of parameter uv_integration_method = 'from_radiance'. |
uv_ir1* | W m-2 | wavelength integrated UV irradiance The UV radiance is calculated based on a sky-view factor approach (LOD1). Requires setting of parameter uv_integration_method = 'from_irradiance'. |
uv_ir2* | W m-2 | wavelength integrated UV irradiance The UV radiance is calculated based on a spherical obstruction approach (LOD2). Requires setting of parameter uv_integration_method = 'from_radiance'. |