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Merge pull request #528 from NCAR/fix-doc-index
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readthedocs build fix #526
mpas constants #251
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hkershaw-brown authored Aug 8, 2023
2 parents f996f26 + c7ef7c1 commit 9729d78
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3 changes: 3 additions & 0 deletions .readthedocs.yaml
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Expand Up @@ -8,3 +8,6 @@ build:
os: ubuntu-22.04
tools:
python: "3.11"

sphinx:
configuration: conf.py
6 changes: 6 additions & 0 deletions CHANGELOG.rst
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Expand Up @@ -22,6 +22,12 @@ individual files.

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

**August 8 2023 :: MPAS-ATM constants and readthedocs fix. Tag v10.8.2**

- MPAS-ATM constants updated to MPAS v5+
- readthedocs build info updated.


**July 27 2023 :: Bug-fixes for MOM6 and WRF. Tag v10.8.1**

- bug-fixes:
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2 changes: 1 addition & 1 deletion assimilation_code/modules/assimilation/filter_mod.rst
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Expand Up @@ -13,7 +13,7 @@ parameter configuration that are driven from its namelist. See the namelist sect
of assimilation steps to be done is controlled by the input observation sequence and by the time-stepping capabilities
of the model being used in the assimilation.

See :doc:`../../../README` for more documentation, including a discussion of the
See :ref:`Welcome page` for more documentation, including a discussion of the
capabilities of the assimilation system, a diagram of the entire execution cycle, the options and features.

Namelist
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2 changes: 1 addition & 1 deletion assimilation_code/programs/filter/filter.rst
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Expand Up @@ -23,7 +23,7 @@ This overview includes these subsections:
- Description of Inflation Options
- Detailed Program Flow

See :doc:`../../../README` for more documentation, including a discussion of the
See :ref:`Welcome page` for more documentation, including a discussion of the
capabilities of the assimilation system, a diagram of the entire execution cycle, the options and features.

Program flow
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4 changes: 2 additions & 2 deletions conf.py
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Expand Up @@ -21,8 +21,8 @@
author = 'Data Assimilation Research Section'

# The full version, including alpha/beta/rc tags
release = '10.8.1'
master_doc = 'README'
release = '10.8.2'
root_doc = 'index'

# -- General configuration ---------------------------------------------------

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2 changes: 1 addition & 1 deletion guide/downloading-dart.rst
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Expand Up @@ -3,7 +3,7 @@ Downloading DART

The DART source code is distributed on the GitHub repository
`NCAR/DART <https://github.com/NCAR/DART>`_ with the documentation
served through :doc:`readthedocs<../README>`.
served through :ref:`readthedocs <Welcome page>`.

Go to https://github.com/NCAR/DART and clone the repository or get the
ZIP file according to your preference. See the `github help page on
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2 changes: 2 additions & 0 deletions README.rst → index.rst
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@@ -1,3 +1,5 @@
.. _Welcome page:

Welcome to the Data Assimilation Research Testbed
=================================================

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2 changes: 1 addition & 1 deletion models/CESM/doc/setup_guidelines.rst
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Expand Up @@ -5,7 +5,7 @@ CESM+DART setup overview
------------------------

If you found your way to this file without reading more basic DART help files,
please read those first. :doc:`Getting Started <../../../README>` is a good place to find pointers to those files.
please read those first. :ref:`Getting Started <Welcome page>` is a good place to find pointers to those files.
Then see :doc:`CESM<../readme>` for an overview of DART's interfaces to CESM.
Finally, see the ../../{your_cesm_component(s)}/readme.html documentation about
the code-level interfaces and namelist values for various CESM component models.
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6 changes: 3 additions & 3 deletions models/clm/tutorial/README.rst
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Expand Up @@ -31,7 +31,7 @@ for CLM-specific assistance.

If you are new to DART, we recommend that you become familiar
by first working through the :doc:`../../../theory/readme` and then
understanding the :doc:`DART getting started <../../../README>` documentation.
understanding the :ref:`DART getting started <Welcome page>` documentation.

This CLM5-DART tutorial is based on a simple example in which we
describe how to:
Expand All @@ -53,8 +53,8 @@ observations that are assimilated, updated model state variables, assimilation t
assimilation frequency, and the model and observation grid resolution.

We encourage users to complete the tutorial and then modify CLM-DART to pursue their own
research questions. We have comprehensive and searchable :doc:`documentation
<../../../README>`, with trained and experienced
research questions. We have comprehensive and searchable :ref:`documentation
<Welcome page>`, with trained and experienced
staff that can help troubleshoot issues ([email protected]).


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16 changes: 8 additions & 8 deletions models/mpas_atm/model_mod.f90
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Expand Up @@ -210,10 +210,10 @@ module model_mod

! Real (physical) constants as defined exactly in MPAS.
! redefined here for consistency with the model.
real(r8), parameter :: rgas = 287.0_r8
real(r8), parameter :: rv = 461.6_r8
real(r8), parameter :: cp = 1003.0_r8
real(r8), parameter :: cv = 716.0_r8
real(r8), parameter :: rgas = 287.0_r8 ! Constant: Gas constant for dry air [J kg-1 K-1]
real(r8), parameter :: rv = 461.6_r8 ! Constant: Gas constant for water vapor [J kg-1 K-1]
real(r8), parameter :: cp = 7.0_r8*rgas/2.0_r8 ! = 1004.5 Constant: Specific heat of dry air at constant pressure [J kg-1 K-1]
real(r8), parameter :: cv = cp - rgas ! = 717.5 Constant: Specific heat of dry air at constant volume [J kg-1 K-1]
real(r8), parameter :: p0 = 100000.0_r8
real(r8), parameter :: rcv = rgas/(cp-rgas)
real(r8), parameter :: rvord = rv/rgas
Expand Down Expand Up @@ -7380,7 +7380,7 @@ function theta_to_tk (ens_size, theta, rho, qv, istatus)

integer, intent(in) :: ens_size
real(r8), dimension(ens_size), intent(in) :: theta ! potential temperature [K]
real(r8), dimension(ens_size), intent(in) :: rho ! dry density
real(r8), dimension(ens_size), intent(in) :: rho ! dry air density [kg/m3]
real(r8), dimension(ens_size), intent(in) :: qv ! water vapor mixing ratio [kg/kg]
integer, dimension(ens_size), intent(inout) :: istatus
real(r8), dimension(ens_size) :: theta_to_tk ! sensible temperature [K]
Expand Down Expand Up @@ -7408,7 +7408,7 @@ function theta_to_tk (ens_size, theta, rho, qv, istatus)
endif
where (istatus == 0)

theta_m = (1.0_r8 + 1.61_r8 * qv_nonzero)*theta
theta_m = (1.0_r8 + rvord * qv_nonzero)*theta

where (theta_m > 0.0_r8 .and. rho > 0.0_r8) ! Check if all the input are positive

Expand Down Expand Up @@ -7441,7 +7441,7 @@ subroutine compute_full_pressure(ens_size, theta, rho, qv, pressure, tk, istatus

integer, intent(in) :: ens_size
real(r8), dimension(ens_size), intent(in) :: theta ! potential temperature [K]
real(r8), dimension(ens_size), intent(in) :: rho ! dry density
real(r8), dimension(ens_size), intent(in) :: rho ! dry air density [kg/m3]
real(r8), dimension(ens_size), intent(in) :: qv ! water vapor mixing ratio [kg/kg]
real(r8), dimension(ens_size), intent(out) :: pressure ! full pressure [Pa]
real(r8), dimension(ens_size), intent(out) :: tk ! return sensible temperature to caller
Expand All @@ -7457,7 +7457,7 @@ subroutine compute_full_pressure(ens_size, theta, rho, qv, pressure, tk, istatus
tk = theta_to_tk(ens_size, theta, rho, qv_nonzero, istatus)

where (istatus == 0) ! We only take non-missing tk here
pressure = rho * rgas * tk * (1.0_r8 + 1.61_r8 * qv_nonzero)
pressure = rho * rgas * tk * (1.0_r8 + rvord * qv_nonzero)
end where

if ( debug > 1 ) then
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10 changes: 9 additions & 1 deletion models/mpas_atm/readme.rst
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Expand Up @@ -7,7 +7,15 @@ Overview
This document describes the DART interface module for the atmospheric component
of the Model for Prediction Across Scales
`MPAS <https://ncar.ucar.edu/what-we-offer/models/model-prediction-across-scales-mpas>`__
(or briefly, MPAS-ATM) global model, which uses an unstructured Voronoi grid mesh,
(or briefly, MPAS-ATM) global model.

The DART interface has constants set to match MPAS v5.0 onwards as defined in
`MPAS-Model/src/framework/mpas_constants.F <https://github.com/MPAS-Dev/MPAS-Model/blob/master/src/framework/mpas_constants.F>`__.
If you need to reproduce work with DART and MPAS v4 you will need to change the model_mod.f90
parameters ``cp``, ``cv`` and ``rvord`` to match MPAS v4.


The mpas-atm model uses an unstructured Voronoi grid mesh,
formally Spherical Centriodal Voronoi Tesselations (SCVTs). This allows for both
quasi-uniform discretization of the sphere and local refinement. The MPAS/DART
interface was built on the SCVT-dual mesh and does not regrid to regular lat/lon
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8 changes: 4 additions & 4 deletions models/wrf/tutorial/README.rst
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Expand Up @@ -27,7 +27,7 @@ forum for WRF-specific assistance.

If you are new to DART, we recommend that you become familiar with DART
by working through the :doc:`../../../theory/readme` and then
understanding the :doc:`DART getting started <../../../README>` documentation.
understanding the :ref:`DART getting started <Welcome page>` documentation.

before attempting the WRF/DART tutorial as you will find many helpful
resources for learning the base DART configuration.
Expand Down Expand Up @@ -109,7 +109,7 @@ needed to perform an experiment.
Build the DART executables.
~~~~~~~~~~~~~~~~~~~~~~~~~~~

If you have not already, see :doc:`Getting Started <../../../README>` to
If you have not already, see :ref:`Getting Started <Welcome page>` to
download the DART software package. Set an environment variable
*DART_DIR* to point to your base DART directory. How to do this will
depend on which shell you are using.
Expand All @@ -135,7 +135,7 @@ might need for an experiment with that model.

1. It is assumed you have successfully configured the
``$DART_DIR/build_templates/mkmf.template`` file for your system. If
not, you will need to do so now. See the :doc:`Getting Started <../../../README>`
not, you will need to do so now. See :ref:`Getting Started <Welcome page>`
for more detail, if necessary.

2. [OPTIONAL] Modify the DART code to use 32bit reals. Most WRF/DART
Expand Down Expand Up @@ -576,7 +576,7 @@ want to run with the example observations, you can skip to Step
4.

However, observation processing is critical to the success of running
DART and was covered in :doc:`getting started <../../../README>`. In
DART and was covered in :ref:`Getting Started <Welcome page>`. In
brief, to add your own observations to WRF/DART you will need to
understand the relationship between observation definitions and
observation sequences, observation types and observation quantities, and
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