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Merge pull request #708 from NCAR/WRF_forward_operators
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Wrf forward operators
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hkershaw-brown authored Aug 15, 2024
2 parents 75cf8dc + b5e8ac1 commit f193ab4
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9 changes: 9 additions & 0 deletions CHANGELOG.rst
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Expand Up @@ -22,6 +22,15 @@ individual files.

The changes are now listed with the most recent at the top.

**August 15 2024 :: WRF fwd operator bug fixes. Tag v11.6.1**

WRF-DART bug-fixes:

- Bug fix for surface temperature observations to use QTY_2M_TEMPERATURE
- Bug fix for conversion of vapor mixing ratio to specific humidity
- Bug fix for diagnostics_obs.csh
- Improved documentation for WRF model_mod and WRF-DART Tutorial

**July 26 2024 :: Library build tools for DART. Tag v11.6.0**

- Buildtools for compiling DART as a shared or a static library.
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2 changes: 1 addition & 1 deletion conf.py
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Expand Up @@ -21,7 +21,7 @@
author = 'Data Assimilation Research Section'

# The full version, including alpha/beta/rc tags
release = '11.6.0'
release = '11.6.1'
root_doc = 'index'

# -- General configuration ---------------------------------------------------
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189 changes: 103 additions & 86 deletions models/wrf/model_mod.f90

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641 changes: 335 additions & 306 deletions models/wrf/readme.rst

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13 changes: 6 additions & 7 deletions models/wrf/shell_scripts/driver.csh
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Expand Up @@ -473,19 +473,18 @@ while ( 1 == 1 )

else if ( $SUPER_PLATFORM == 'derecho' ) then

# Prevent double submission for member 1 only
if ( $n == 1) then
sleep 5
endif

if ( `qstat -wa | grep assim_advance_${n} | wc -l` == 0 ) then

echo "assim_advance_${n} is missing from the queue"
qsub assim_advance_mem${n}.csh
echo "Warning, detected that assim_advance_${n} is missing from the queue"
echo "If this warning leads to missing output from ensemble ${n}"
echo "consider enabling the qsub command within keep_trying while statement in driver.csh"

#qsub assim_advance_mem${n}.csh
endif

endif
sleep 15
sleep 5

end
set start_time = `head -1 start_member_${n}`
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17 changes: 8 additions & 9 deletions models/wrf/shell_scripts/mean_increment.ncl
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@@ -1,7 +1,7 @@
; find the mean state space increment, output the fields to a single mean file
; that can be used to make plots
; G. Romine 2011-12

; Updating for 1 domain only B. Raczka 2024-08
begin

; get the list of files to read in
Expand All @@ -23,9 +23,7 @@ begin
ListSetType(fil, "join")

pull_2D_field_names = (/"T2", "Q2", "U10", "V10", "PSFC"/)
pull_2D_field_names(:) = pull_2D_field_names(:)+"_d01"
pull_3D_field_names = (/"U", "V", "T", "QVAPOR"/)
pull_3D_field_names(:) = pull_3D_field_names(:)+"_d01"
pull_3D_field_names = (/"U", "V", "THM", "QVAPOR"/)
npulls = dimsizes(pull_2D_field_names)

; Below will dump out the data to a file for replotting later
Expand All @@ -34,16 +32,17 @@ begin
do i=0,npulls-1
print(" Extracting 2d variable "+pull_2D_field_names(i))
do fil_num=0,nfils-1
; print(" reading file "+flist(fil_num))
; dimensions are ncljoin, copy, Time, south_north, west_east
; print(" reading file "+flist(fil_num))
; dimensions are ncljoin, Time, south_north, west_east
; copy zero is the ensemble mean
pull_var = fil[fil_num]->$pull_2D_field_names(i)$(:,0,:,:,:)
pull_var = fil[fil_num]->$pull_2D_field_names(i)$(:,:,:,:)
dims = dimsizes(pull_var)
if (fil_num .eq. 0) then ; first iteration, make var
alltimes_var = new ( (/nfils,dims(2),dims(3)/), typeof(pull_var) )
end if
; printVarSummary(pull_var)
alltimes_var(fil_num,:,:) = pull_var(0,0,:,:)
; printVarSummary(alltimes_var)
delete(pull_var)
end do
; average over time (first dimension)
Expand All @@ -69,9 +68,9 @@ begin
print(" Extracting 3d variable "+pull_3D_field_names(i))
do fil_num=0,nfils-1
; print(" reading file "+flist(fil_num))
; dimensions are ncljoin, copy, Time, level, south_north, west_east
; dimensions are ncljoin, Time, level, south_north, west_east
; copy zero is the ensemble mean
pull_var = fil[fil_num]->$pull_3D_field_names(i)$(:,0,:,:,:,:)
pull_var = fil[fil_num]->$pull_3D_field_names(i)$(:,:,:,:,:)
dims = dimsizes(pull_var)
if (fil_num .eq. 0) then ; first iteration, make var
alltimes_var = new ( (/nfils,dims(2),dims(3),dims(4)/), typeof(pull_var) )
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236 changes: 228 additions & 8 deletions models/wrf/tutorial/README.rst
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Expand Up @@ -600,7 +600,7 @@ also want to modify this script to test running a single member first —
just in case you have some debugging to do.

However, be warned that to successfully complete the tutorial, including
running the *driver.csh* script in Step 5, using a smaller ensemble
running the *driver.csh* script in Step 6, using a smaller ensemble
(e.g. < 20 members) can lead to spurious updates during the analysis step,
causing the WRF simulation to fail.

Expand All @@ -617,7 +617,7 @@ Step 3: Prepare observations [OPTIONAL]

The observation sequence files to run this tutorial are already provided
for you. If you want to run with the provided tutorial observations, you
can skip to Step 4 right now. If you are interested in using custom
can skip to Step 5 right now. If you are interested in using custom
observations for a WRF experiment other than the tutorial you should read on.
The remaining instructions provided below in Step 3 are meant as a guideline
to converting raw PREPBUFR data files into the required ``obs_seq`` format
Expand Down Expand Up @@ -807,8 +807,228 @@ you would do the following:
namelist options to consider, and you must provide a *wrfinput* file
for the program to access the analysis domain information.

Step 4: Overview of forward (observation) operators [OPTIONAL]
--------------------------------------------------------------

Step 4: Creating the first set of adaptive inflation files
This section is for informational purposes only and does not include any
instructions to complete the tutorial. It provides a description of
the DART settings that control the forward operator which
calculates the prior and posterior model estimates for the observations.
An introduction to important namelist variables that control the operation of the forward
operator are located in the `WRF namelist documentation.
<../../../models/wrf/readme.html#namelist>`__


The ``obs_seq.out`` file generated as described in Step 3 includes a total
of 30 observation types. Here we examine an exerpt of that file, focusing
on a single temperature observation to describe the process:

::

obs_sequence
obs_kind_definitions
30
41 METAR_TEMPERATURE_2_METER
..
..
num_copies: 1 num_qc: 1
num_obs: 70585 max_num_obs: 70585
NCEP BUFR observation
NCEP QC index
first: 1 last: 70585
OBS 1
288.750000000000
1.00000000000000
-1 2 -1
obdef
loc3d
4.819552185804497 0.6141813398083548 518.0000000000000 -1
kind
41
43200 152057
3.06250000000000
..
..
..


A critical piece of observation metadata includes the observation type
(``METAR_TEMPERATURE_2_METER``) which is linked to the quantity
(``QTY_2M_TEMPERATURE``) through the observation definition file
(``obs_def_metar_mod.f90``). This file is included within the
``&preprocess_nml`` section of the namelist file as:

::

&preprocess_nml
overwrite_output = .true.
input_obs_qty_mod_file = '../../../assimilation_code/modules/observations/DEFAULT_obs_kind_mod.F90'
output_obs_qty_mod_file = '../../../assimilation_code/modules/observations/obs_kind_mod.f90'
input_obs_def_mod_file = '../../../observations/forward_operators/DEFAULT_obs_def_mod.F90'
output_obs_def_mod_file = '../../../observations/forward_operators/obs_def_mod.f90'
quantity_files = '../../../assimilation_code/modules/observations/atmosphere_quantities_mod.f90'
obs_type_files = '../../../observations/forward_operators/obs_def_reanalysis_bufr_mod.f90',
'../../../observations/forward_operators/obs_def_altimeter_mod.f90',
'../../../observations/forward_operators/obs_def_radar_mod.f90',
'../../../observations/forward_operators/obs_def_metar_mod.f90',
..
..
..

During the DART compilation described within Step 1 this information is
included within the ``obs_def_mod.f90``.

The vertical coordinate type is the 4th column beneath the loc3d header within ``obs_seq.out``.
In this example the value -1 indicates the vertical coordinate is ``VERTISSURFACE``. It defines the
vertical units of the observation (e.g. pressure, meters above sea level, model levels etc).
This serves two purposes -- foremost it is required during the vertical spatial interpolation
to calculate the precise location of the expected observation.
A second crtical function is that it defines whether it is a surface observation.
Observations with a vertical coordinate of ``VERTISSURFACE`` are defined as surface
observations. All other coordinates are considered non-surface observations
(e.g. profile observations). Of note is that the vertical coordinate ``VERTISSURFACE`` and
``VERTISHEIGHT`` are functionally identical (i.e. meters above sea level), however
only the ``VERTISSURFACE`` is a surface observation.

For more information on the vertical coordinate metadata see the detailed structure of
an `obs_seq file. <../../../guide/creating-obs-seq-real.html#observation-location>`__

In order to connect this observation to the appropriate WRF output variables
the ``wrf_state_variables`` within ``&model_nml`` defines the *WRF field name* and
the *WRF TYPE* in the 1st and 3rd columns as shown in the tutorial example below:

::

&model_nml
wrf_state_variables = 'T2','QTY_TEMPERATURE','TYPE_T2','UPDATE','999'

..
..

For more information on the ``&model_nml`` variables see the `WRF documentation page
<../../../models/wrf/readme.html#namelist>`__


As described above, the linkage between the observation type and the WRF output field
is defined through the physical quantity, surface variable designation (observation
vertical coordinate), and WRF TYPE. The current design of the WRF ``model_mod.f90``
is such that the quantity is a general classification (e.g. temperature, wind
specific humidity), whereas the WRF TYPE classification is more precisely
mapped to the WRF output field. The table below summarizes the dependency between
the observation type and the WRF output field for a select number of observation types
within the tutorial.

.. Note::

The number of WRF output fields required to support an observation type can vary. For
observation types where there is a direct analog to a WRF output field, the forward
operator consists of only spatial interpolation, thus requires only a single output
variable (e.g. METAR_TEMPERATURE_2_METER). For observation types that require multiple
WRF output fields, the forward operator is more complex than a simple spatial interpolation.
For more information see the notes below the table. A rule of thumb is a surface
observation should use a surface output field (e.g. T2, U10). WRF surface output fields
are appended by a numeric value indicating surface height in meters. It is possible to use
a non-surface WRF output field (3D field) to estimate a surface observation, however, this
requires a vertical interpolation of the 3D WRF field where the observed surface height does
not coincide with the model levels. This either requires a vertical interpolation or an
extrapolation which can be **inaccurate and is not recommended**.




+----------------------------------+---------+-------------------------------+--------------+------------+
| DART Observation Type | Surface | DART Quantity | WRF Type | WRF output |
| | Obs ? | | | field |
+==================================+=========+===============================+==============+============+
| ``METAR_TEMPERATURE_2_METER`` | Yes | ``QTY_2M_TEMPERATURE`` | ``TYPE_T2`` | ``T2`` |
| | | | | |
+----------------------------------+---------+-------------------------------+--------------+------------+
| ``RADIOSONDE_TEMPERATURE`` | No | ``QTY_POTENTIAL_TEMPERATURE`` | ``TYPE_T`` | ``THM`` |
| | | ``QTY_VAPOR_MIXING_RATIO`` | ``TYPE_QV`` | ``QVAPOR`` |
| | | ``QTY_PRESSURE`` | ``TYPE_MU`` | ``MU PH`` |
| | | ``QTY_GEOPOTENTIAL_HEIGHT`` | ``TYPE_GZ`` | |
+----------------------------------+---------+-------------------------------+--------------+------------+
| ``METAR_U_10_METER_WIND`` | Yes | ``QTY_U_WIND_COMPONENT`` | ``TYPE_U10`` | ``U10`` |
| | | ``QTY_V_WIND_COMPONENT`` | ``TYPE_V10`` | ``V10`` |
+----------------------------------+---------+-------------------------------+--------------+------------+
| ``ACARS_U_WIND_COMPONENT`` | No | ``QTY_U_WIND_COMPONENT`` | ``TYPE_U`` | ``U`` |
| | | ``QTY_V_WIND_COMPONENT`` | ``TYPE_V`` | ``V`` |
+----------------------------------+---------+-------------------------------+--------------+------------+
| ``METAR_DEWPOINT_2_METER`` | Yes | ``QTY_DEWPOINT`` | | |
| | | ``QTY_SPECIFIC_HUMIDITY`` | ``TYPE_Q2`` | ``Q2`` |
| | | ``QTY_PRESSURE`` | ``TYPE_PS`` | ``PSFC`` |
+----------------------------------+---------+-------------------------------+--------------+------------+
| ``RADIOSONDE_SPECIFIC_HUMIDITY`` | No | ``QTY_SPECIFIC_HUMIDITY`` | ``TYPE_QV`` | ``QVAPOR`` |
| | | | | |
+----------------------------------+---------+-------------------------------+--------------+------------+



Surface Temperature (e.g. METAR_TEMPERATURE_2_METER)
~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~

WRF output includes a direct analog for sensible temperature surface observations (e.g. T2), thus
the forward operator requires only 1 variable to calculate the expected observation.
The calculation includes a horizontal interpolation of the 2D temperature variable (e.g. T2).


Non-Surface Temperature (e.g. RADIOSONDE_TEMPERATURE)
~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~

In contrast to surface temperature observations, non-surface temperature observations require 4 WRF
output fields. This is because observations are sensible temperature, whereas the 3D WRF
temperature field is provided in perturbation potential temperature. Thus, the forward
operator first requires a physical conversion between perturbation potential temperature to
sensible temperature, followed by a spatial interpolation (this includes horizontal interpolation
on WRF levels k and k+1, followed by vertical interpolation).

.. Important::

There are two different 3D temperature WRF output fields that can work to calculate non-
surface temperature observations (e.g. T or THM, T=THM when use_theta_m=0). However, and **of
utmost importance** is the variable THM is required to be within the ``&model_nml`` if the
3D temperature field is to be updated in the ``filter`` step. **This is because the WRF field *T*
is a diagnostic variable with no impact on the forecast step, whereas the WRF field *THM* is
a prognostic field which will impact the forecast.**


Surface Wind (e.g. METAR_U_10_METER_WIND)
~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~

Surface winds have a direct WRF output analog (e.g. U10)
and requires horizontal interpolation of the 2D zonal wind field. However, the
meridional wind (e.g. V10) is also required in order to convert from modeled *gridded* winds to
*true* wind observations. This requirement is an artifact of winds measured on a sphere being
mapped on a 2D grid.


Non-Surface Wind (e.g. ACARS_U_WIND_COMPONENT)
~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~

This is identical to surface winds as described above, except the spatial interpolation requires
horizontal interpolation on the k and k+1 WRF levels, followed by vertical interpolation.


Surface Dewpoint (e.g. METAR_DEWPOINT_2_METER)
~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~

The calculation of surface dewpoint requires a physical conversion using both surface
pressure (PSFC) and surface vapor mixing ratio (Q2), follwed by horizontal interpolation.


Non-Surface Specific Humidity (e.g. RADIOSONDE_SPECIFIC_HUMIDITY)
~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~

Specific humidity observations require the (water) vapor mixing ratio (QVAPOR) for the forward operator.
Although specific humidity and vapor mixing ratio are nearly identical, especially in dry
air, they are actually two distinct physical properties -- the ratio of water mass to total air mass
versus ratio of water vapor mass to dry air mass respectively. Therefore the forward operator
includes this physical conversion followed by a spatial interpolation (i.e. horizontal interpolation of k and
k+1 WRF vertical levels followed by vertical interpolation).



Step 5: Creating the first set of adaptive inflation files
----------------------------------------------------------

In this section we describe how to create initial adaptive inflation
Expand Down Expand Up @@ -874,7 +1094,7 @@ cycle.



Step 5: Cycled analysis system
Step 6: Cycled analysis system
------------------------------

While the DART system provides executables to perform individual tasks
Expand Down Expand Up @@ -924,10 +1144,10 @@ continue to cycle until the final analysis time has been reached.



Step 6: Diagnosing the assimilation results
Step 7: Diagnosing the assimilation results
-------------------------------------------

Once you have successfully completed steps 1-5, it is important to
Once you have successfully completed steps 1-6, it is important to
check the quality of the assimilation. In order to do this, DART provides
analysis system diagnostics in both state and observation space.

Expand Down Expand Up @@ -989,7 +1209,7 @@ The tools below provide methods to visualize the spatial patterns, statistics an
failure mode for all observations.

The observation diagnostics use the **obs_epoch*.nc** file as input. This file is
automatically generated by the **obs_diagnostic.csh** script within Step 5 of this
automatically generated by the **obs_diagnostic.csh** script within Step 6 of this
tutorial.

The **obs_epoch*.nc** file is located in the output directory of each time step.
Expand Down Expand Up @@ -1211,7 +1431,7 @@ quite high (>90%). This high acceptance percentage is typical of a high-quality
assimilation and consistent with the strong reduction in RMSE.


The same plot as above is given below except for the observation type:
The same plot as above except for the observation type:
``RADIOSONE_SPECIFIC_HUMIDITY``.

+-------------------------------------------------------------+
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