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Merge in NOAA develop head #14

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17a4e32
Bugfix - initialised VD and VS to zero in w3srcemd. (#1037)
ukmo-ccbunney Jul 7, 2023
2514633
More efficient test for binary files in matrix.comp (#1035)
ukmo-ccbunney Jul 7, 2023
4d8c315
Tidy up of pre-processor directives and unused variables in w3srcemd.…
ukmo-ccbunney Jul 11, 2023
02cb72f
Correct typo in w3srcemd.F90 pre-processor directive. (#1039)
ukmo-ccbunney Jul 14, 2023
1cacc43
minor bugfix for matrix grepping on keywords (#1049)
mickaelaccensi Jul 31, 2023
dcafc8c
Stop masking group 1 output where icec > icen (#1019)
benoitp-cmc Aug 4, 2023
2715a9e
Doxygen documentation added, 8th subset.(#1046)
MatthewMasarik-NOAA Aug 7, 2023
b810a89
NC4 ,F90 ,XX0 switches removed from ww3_tp2.19 regtest (#1054)
Ghazal-Mohammadpour Aug 11, 2023
991daf8
CI: Fix for Intel scripts. GNU scripts updated. (#1064)
MatthewMasarik-NOAA Sep 2, 2023
6b9edfa
correct the computation of QP parameter, add QKK output parameter, ch…
mickaelaccensi Sep 14, 2023
8589d12
correct issue with ww3_multi when requesting restart2 and using nml f…
mickaelaccensi Sep 21, 2023
7bbdaca
correct calendar for track netcdf output (#1079)
mickaelaccensi Sep 22, 2023
b1356dd
Fix missing mod_def.ww3 file in multigrid regression tests for track …
ukmo-ccbunney Oct 10, 2023
d22b7bb
STAB3: fix cmake build for ST4 or ST3 (#1086)
MatthewMasarik-NOAA Oct 10, 2023
eff6686
new feature to output out_grd.ww3, out_pnt.ww3 and mod_def.ww3 both i…
mickaelaccensi Oct 12, 2023
d148d09
Update local unit number arrays (NDS, MDS) to be same size of array d…
ukmo-ccbunney Oct 16, 2023
66262f6
Removed code referencing PHIOC in output section for PHICE in ww3_oun…
ukmo-ccbunney Oct 18, 2023
8eb3596
implementation of the GQM (Gaussian Quadrature Method) to replace the…
mickaelaccensi Oct 19, 2023
4cd995d
update logic to ensure you are not accessing uninitialized dates (#1114)
JessicaMeixner-NOAA Oct 31, 2023
c3451a9
Initialised S and D arrays in W3SDB1 before potential early return if…
ukmo-ccbunney Nov 1, 2023
f702a8f
ww3_ounp.F90: x/y units attribute corrected from 'm' to 'km' (#1088)
Biao-Zhao Nov 2, 2023
1f928aa
Bugfix: Assign unit numbers to ASCII gridded/point output in multi-gr…
ukmo-ccbunney Nov 6, 2023
d90078b
correct bugs to run correctly GQM implementation (#1127)
mickaelaccensi Nov 28, 2023
3f35df7
Adding documentation to w3iopo() in preparation for code for #682. (#…
edwardhartnett Nov 30, 2023
ff1b9e9
NCEP regtest module updates: uses spack-stack/1.5.0, includes scotch/…
MatthewMasarik-NOAA Dec 7, 2023
d3ea810
Minor update to ncep regtests (#1138)
JessicaMeixner-NOAA Dec 12, 2023
88c89be
Updated intel workflow to install oneapi compilers from new location.…
edwardhartnett Dec 26, 2023
7bec560
Add unit test for points I/O code. (#1158)
edwardhartnett Jan 4, 2024
63f8270
Update Intel CI (relocate /usr/local; ensure intel-oneapi-mpi; use ub…
AlexanderRichert-NOAA Jan 11, 2024
3952826
remove lookup table for ST4 to speed up computation and clean up the …
mickaelaccensi Jan 16, 2024
026fcdd
initialize USSP_WN for mod_def (#1165)
JessicaMeixner-NOAA Jan 22, 2024
9a718fc
Introduce IC4M8 and IC4M9 to WW3 (#1176)
ErickRogers Jan 23, 2024
ff0358a
clean up and add ST4 variables (#1181)
mickaelaccensi Jan 25, 2024
ba5cd68
w3fld1md.F90: fix divide by zero in CRIT2 parameter (#1184)
MatthewMasarik-NOAA Feb 5, 2024
fd6d559
ww3_prnc.F90: fix out-of-scope grid index write statement (#1185)
MatthewMasarik-NOAA Feb 5, 2024
6d42025
Bugfix: address potential divide-by-zero in APPENDTAIL (#1188)
MatthewMasarik-NOAA Feb 15, 2024
e085bcf
Provide initial drying of cells with depth < ZLIM for SMC grid. (#1192)
ukmo-ccbunney Feb 23, 2024
156a46d
Output OMP threading info to screen when running ww3_shel/ww3_multi c…
ukmo-ccbunney Mar 11, 2024
9d3799f
update run_cmake_test to catch build errors and exit (#1194)
JessicaMeixner-NOAA Mar 12, 2024
027ef77
Merge branch 'develop' of https://github.com/NOAA-EMC/WW3 into ct/mer…
camilleanne Mar 13, 2024
b344d66
fix merge conflicts
camilleanne Mar 13, 2024
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12 changes: 6 additions & 6 deletions .github/workflows/gnu.yml
Original file line number Diff line number Diff line change
Expand Up @@ -7,7 +7,7 @@ concurrency:
cancel-in-progress: true

env:
cache_key: gnu8
cache_key: gnu11
CC: gcc-10
FC: gfortran-10
CXX: g++-10
Expand All @@ -24,14 +24,14 @@ jobs:
steps:
- name: checkout-ww3
if: steps.cache-env.outputs.cache-hit != 'true'
uses: actions/checkout@v2
uses: actions/checkout@v3
with:
path: ww3
# Cache spack, OASIS, and compiler
# No way to flush Action cache, so key may have # appended
- name: cache-env
id: cache-env
uses: actions/cache@v2
uses: actions/cache@v3
with:
path: |
spack
Expand All @@ -45,7 +45,7 @@ jobs:
run: |
# Install NetCDF, ESMF, g2, etc using Spack
sudo apt install cmake
git clone -c feature.manyFiles=true https://github.com/spack/spack.git
git clone -c feature.manyFiles=true https://github.com/JCSDA/spack.git
source spack/share/spack/setup-env.sh
spack env create ww3-gnu ww3/model/ci/spack_gnu.yaml
spack env activate ww3-gnu
Expand Down Expand Up @@ -77,13 +77,13 @@ jobs:

steps:
- name: checkout-ww3
uses: actions/checkout@v2
uses: actions/checkout@v3
with:
path: ww3

- name: cache-env
id: cache-env
uses: actions/cache@v2
uses: actions/cache@v3
with:
path: |
spack
Expand Down
41 changes: 25 additions & 16 deletions .github/workflows/intel.yml
Original file line number Diff line number Diff line change
@@ -1,3 +1,8 @@
# This is a GitHub actions workflow for WW3.
#
# This workflow builds with the Intel compilers.
#
# Matt Masarik, Alex Richert, Ed Hartnett
name: Intel Linux Build
on: [push, pull_request, workflow_dispatch]

Expand All @@ -8,34 +13,34 @@ concurrency:

# Set I_MPI_CC/F90 so Intel MPI wrapper uses icc/ifort instead of gcc/gfortran
env:
cache_key: intel7
cache_key: intel10-3
CC: icc
FC: ifort
CXX: icpc
I_MPI_CC: icc
I_MPI_F90: ifort

# Split into a dependency build step, and a WW3 build step which
# builds multiple switches in a matrix. The setup is run once and
# builds multiple switches in a matrix. The setup is run once and
# the environment is cached so each build of WW3 can share the dependencies.

jobs:
setup:
runs-on: ubuntu-20.04
runs-on: ubuntu-latest

steps:

- name: checkout-ww3
if: steps.cache-env.outputs.cache-hit != 'true'
uses: actions/checkout@v2
uses: actions/checkout@v3
with:
path: ww3

# Cache spack, OASIS, and compiler
# No way to flush Action cache, so key may have # appended
- name: cache-env
id: cache-env
uses: actions/cache@v2
uses: actions/cache@v3
with:
path: |
spack
Expand All @@ -51,26 +56,28 @@ jobs:
sudo apt-key add GPG-PUB-KEY-INTEL-SW-PRODUCTS.PUB
echo "deb https://apt.repos.intel.com/oneapi all main" | sudo tee /etc/apt/sources.list.d/oneAPI.list
sudo apt-get update
sudo apt-get install intel-oneapi-mpi-devel intel-oneapi-openmp intel-oneapi-compiler-fortran intel-oneapi-compiler-dpcpp-cpp-and-cpp-classic
sudo apt-get install intel-oneapi-dev-utilities intel-oneapi-mpi-devel intel-oneapi-compiler-fortran-2023.2.1 intel-oneapi-compiler-dpcpp-cpp-and-cpp-classic-2023.2.1 intel-oneapi-openmp

# Build WW3 spack environment
- name: install-dependencies-with-spack
if: steps.cache-env.outputs.cache-hit != 'true'
run: |
sudo mv /usr/local /usr/local_mv
# Install NetCDF, ESMF, g2, etc using Spack
. /opt/intel/oneapi/setvars.sh
sudo mv /usr/local /usrlocal_renamed
sudo apt install cmake
git clone -c feature.manyFiles=true https://github.com/spack/spack.git
git clone -c feature.manyFiles=true https://github.com/JCSDA/spack.git
source spack/share/spack/setup-env.sh
ln -s $(realpath $(which gcc)) spack/lib/spack/env/intel/gcc # spack/make bug in ESMF
spack env create ww3-intel ww3/model/ci/spack_intel.yaml
spack env activate ww3-intel
spack compiler find
spack external find cmake
spack add intel-oneapi-mpi
sudo apt install cmake
spack external find
spack config add "packages:mpi:require:'intel-oneapi-mpi'"
spack config add "packages:all:require:['%intel']"
spack concretize
spack install --dirty -v --fail-fast
spack clean --all

- name: build-oasis
if: steps.cache-env.outputs.cache-hit != 'true'
Expand All @@ -91,17 +98,17 @@ jobs:
strategy:
matrix:
switch: [Ifremer1, NCEP_st2, NCEP_st4, ite_pdlib, NCEP_st4sbs, NCEP_glwu, OASACM, UKMO, MULTI_ESMF]
runs-on: ubuntu-20.04
runs-on: ubuntu-latest

steps:
- name: checkout-ww3
uses: actions/checkout@v2
uses: actions/checkout@v3
with:
path: ww3

- name: cache-env
id: cache-env
uses: actions/cache@v2
uses: actions/cache@v3
with:
path: |
spack
Expand All @@ -112,12 +119,14 @@ jobs:

- name: build-ww3
run: |
sudo mv /usr/local /usr/local_mv
sudo apt install cmake
. /opt/intel/oneapi/setvars.sh
source spack/share/spack/setup-env.sh
spack env activate ww3-intel
cd ww3
export CC=mpicc
export FC=mpif90
export CC=mpiicc
export FC=mpiifort
export OASISDIR=${GITHUB_WORKSPACE}/work_oasis3-mct
mkdir build && cd build
if [[ ${{ matrix.switch }} == "MULTI_ESMF" ]]; then
Expand Down
122 changes: 122 additions & 0 deletions .github/workflows/io_gnu_yml.old
Original file line number Diff line number Diff line change
@@ -0,0 +1,122 @@
name: io_gnu
on: [push, pull_request, workflow_dispatch]

# Cancel in-progress workflows when pushing to a branch
concurrency:
group: ${{ github.workflow }}-${{ github.event.pull_request.number || github.ref }}
cancel-in-progress: true

env:
cache_key: gnu11-1
CC: gcc-10
FC: gfortran-10
CXX: g++-10


# Split into a steup step, and a WW3 build step which
# builds multiple switches in a matrix. The setup is run once and
# the environment is cached so each build of WW3 can share the dependencies.

jobs:
setup:
runs-on: ubuntu-latest

steps:
- name: checkout-ww3
if: steps.cache-env.outputs.cache-hit != 'true'
uses: actions/checkout@v3
with:
path: ww3
# Cache spack, OASIS, and compiler
# No way to flush Action cache, so key may have # appended
- name: cache-env
id: cache-env
uses: actions/cache@v3
with:
path: |
spack
~/.spack
work_oasis3-mct
key: spack-${{ runner.os }}-${{ env.cache_key }}-${{ hashFiles('ww3/model/ci/spack_gnu.yaml') }}

# Build WW3 spack environment
- name: install-dependencies-with-spack
if: steps.cache-env.outputs.cache-hit != 'true'
run: |
# Install NetCDF, ESMF, g2, etc using Spack
sudo apt install cmake
git clone -c feature.manyFiles=true https://github.com/JCSDA/spack.git
source spack/share/spack/setup-env.sh
spack env create ww3-gnu ww3/model/ci/spack_gnu.yaml
spack env activate ww3-gnu
spack compiler find
spack external find cmake
spack add [email protected]
spack concretize
spack install --dirty -v

- name: build-oasis
if: steps.cache-env.outputs.cache-hit != 'true'
run: |
source spack/share/spack/setup-env.sh
spack env activate ww3-gnu
export WWATCH3_DIR=${GITHUB_WORKSPACE}/ww3/model
export OASIS_INPUT_PATH=${GITHUB_WORKSPACE}/ww3/regtests/ww3_tp2.14/input/oasis3-mct
export OASIS_WORK_PATH=${GITHUB_WORKSPACE}/ww3/regtests/ww3_tp2.14/input/work_oasis3-mct
cd ww3/regtests/ww3_tp2.14/input/oasis3-mct/util/make_dir
cmake .
make VERBOSE=1
cp -r ${GITHUB_WORKSPACE}/ww3/regtests/ww3_tp2.14/input/work_oasis3-mct ${GITHUB_WORKSPACE}

io_gnu:
needs: setup
runs-on: ubuntu-latest

steps:
- name: install-dependencies
run: |
sudo apt-get update
sudo apt-get install doxygen gcovr valgrind

- name: checkout-ww3
uses: actions/checkout@v3
with:
path: ww3

- name: cache-env
id: cache-env
uses: actions/cache@v3
with:
path: |
spack
~/.spack
work_oasis3-mct
key: spack-${{ runner.os }}-${{ env.cache_key }}-${{ hashFiles('ww3/model/ci/spack_gnu.yaml') }}

- name: build-ww3
run: |
source spack/share/spack/setup-env.sh
spack env activate ww3-gnu
set -x
cd ww3
export CC=mpicc
export FC=mpif90
export OASISDIR=${GITHUB_WORKSPACE}/work_oasis3-mct
mkdir build && cd build
export LD_LIBRARY_PATH="/home/runner/work/WW3/WW3/spack/var/spack/environments/ww3-gnu/.spack-env/view/:$LD_LIBRARY_PATH"
cmake -DSWITCH=${GITHUB_WORKSPACE}/ww3/regtests/unittests/data/switch.io -DCMAKE_BUILD_TYPE=Debug -DCMAKE_Fortran_FLAGS="-g -fprofile-abs-path -fprofile-arcs -ftest-coverage -O0 -Wall -fno-omit-frame-pointer -fsanitize=address" -DCMAKE_C_FLAGS="-g -fprofile-abs-path -fprofile-arcs -ftest-coverage -O0 -Wall -fno-omit-frame-pointer -fsanitize=address" ..
make -j2 VERBOSE=1
./bin/ww3_grid
mv mod_def.ww3 regtests/unittests
ctest --verbose --output-on-failure --rerun-failed
gcovr --root .. -v --html-details --exclude ../regtests/unittests --exclude CMakeFiles --print-summary -o test-coverage.html &> /dev/null

- name: upload-test-coverage
uses: actions/upload-artifact@v3
with:
name: ww3-test-coverage
path: |
ww3/build/*.html
ww3/build/*.css


6 changes: 6 additions & 0 deletions CMakeLists.txt
Original file line number Diff line number Diff line change
Expand Up @@ -58,3 +58,9 @@ if(NOT CMAKE_BUILD_TYPE MATCHES "^(Debug|Release|RelWithDebInfo|MinSizeRel)$")
endif()

add_subdirectory(model)

# Turn on unit testing.
include(CTest)
if(BUILD_TESTING)
add_subdirectory(regtests/unittests)
endif()
3 changes: 3 additions & 0 deletions manual/defs.tex
Original file line number Diff line number Diff line change
Expand Up @@ -94,6 +94,9 @@
\newcommand{\cR}{{\cal R}}
\newcommand{\cS}{{\cal S}}

\newcommand{\rd}{{\mathrm d}}


\newcommand{\marbox}[1]{\marginpar{\fbox{{\small #1}}}}

\newcommand{\proddefH}[3]{
Expand Down
16 changes: 15 additions & 1 deletion manual/eqs/ICE4.tex
Original file line number Diff line number Diff line change
Expand Up @@ -52,6 +52,20 @@ \subsubsection{~$S_{ice}$: Empirical/parametric damping by sea ice} \label{sec:I

{\code IC4M7}: This is a formula for dissipation from \cite{art:Dob15}, developed for a mixture of pancake and frazil ice, using data collected in the Weddell Sea (Antarctica). The formula depends on wave frequency and ice thickness:
\begin{equation}\label{eq:ice7}
{\alpha=0.2T^{-2.13}h} \:\:\: .
{\alpha=2k_i=0.2h^1f^{2.13}} \:\:\: .
\end{equation}
This method is described in \cite{rep:RPLA18}.

{\code IC4M8}: Like {\code IC4M7}, this method is in the general form of
\begin{equation}\label{eq:ice8}
{k_i=C_{hf}h^mf^n} \:\:\: .
\end{equation}
The formula is taken from \cite{Meylan2018}, where it is described as a ``Model with Order 3 Power Law''. It is applied by \cite{Liu2020}, where it is referred to as the ``M2'' model. The model specifies $m=1$ and $n=3$, and $C_{hf}$ is a user-specified calibration coefficient. \cite{Liu2020} provide calibration to two field cases and \cite{rep:RYW2021} provides a calibration to a third field case, \cite{art:RMK2021}. The third calibration is set as the default for {\code IC4M8}, $C_{hf}=0.059$, but can be changed in using the namelist parameter (constant and uniform) {\code IC4CN}, or using the spatially and/or temporally variable parameter ${C_{ice,2}}$ . Further details on the calibrations are available in the inline documentation in {\file w3sic4md.F90}. This method is functionally the same as the ``{\code M2}'' model in {\code IC5} (i.e., {\code IC5} with {\code IC5VEMOD=3}) and is redundantly included here as {\code IC4M8} because it is in the same ``family'' as {\code IC4M7} and {\code IC4M9}, being in the form of Eq. (\ref{eq:ice8}).

For an example of setting the namelist parameter, see {\file /regtests/ww3\_tic1.1/input\_IC4\_M8}.

{\code IC4M9}: This formula is taken from the ``monomial power fit'' given in section 2.2.3 of \cite{rep:RYW2021}. Like {\code IC4M7} and {\code IC4M8}, it is a specific case of the general form of Eq. (\ref{eq:ice8}). The specificity is the constraint that $m=n/2-1$. This constraint is derived by \cite{rep:RYW2021} by invoking the scaling from \cite{art:YRW2019}, which is based on Reynolds number with ice thickness as the relevant length scale. This is also given as equation 2 in \cite{art:YRW2022}. The default namelist settings are $C_{hf}=2.9$ and $n=4.5$, from calibration by \cite{rep:RYW2021} to \cite{art:RMK2021}. Further details, including alternative calibrations such as \cite{art:Yu2022}, are available in the inline documentation in {\file w3sic4md.F90}. Constant values can be set using namelist parameters, where $C_{hf}$ and $n$ are {\code IC4CN(1)} and {\code IC4CN(2)}, respectively. Spatially and/or temporally versions of the same can be specified as ${C_{ice,2}}$ and ${C_{ice,3}}$, respectively.

The namelist default $C_{hf}$ values in {\code IC4M8} and {\code IC4M9} are consistent with those of identical formulae implemented in \cite{man:SWAN4145A}.


4 changes: 2 additions & 2 deletions manual/eqs/ICE5.tex
Original file line number Diff line number Diff line change
Expand Up @@ -25,7 +25,7 @@ \subsubsection{~$S_{ice}$: Damping by sea ice (effective medium models)} \label{
\begin{align}
k_i^{EFS} &\propto \eta h_i^3 \sigma^{11},\label{eq:fspw}\\ k_i^{RP} &\propto \frac{\eta}{\rho_w g^2} \sigma^3,\label{eq:rppw}
\end{align}
whereas previous field measurements \citep[e.g.,][]{Meylan2018, Rogers2021} support a power law $k_i \propto \sigma^n$, with $n$ between 2 and 4. Eqs.~(\ref{eq:fspw}) and (\ref{eq:rppw}) indicate at certain regimes (i.e., $k_r \approx k_0$ and low $k_i$), $k_i$ of the EFS model is too sensitive to wave frequency and $k_i$ of the RP model shows no dependence on ice thickness.
whereas previous field measurements \citep[e.g.,][]{Meylan2018, RMK21} support a power law $k_i \propto \sigma^n$, with $n$ between 2 and 4. Eqs.~(\ref{eq:fspw}) and (\ref{eq:rppw}) indicate at certain regimes (i.e., $k_r \approx k_0$ and low $k_i$), $k_i$ of the EFS model is too sensitive to wave frequency and $k_i$ of the RP model shows no dependence on ice thickness.

The third model included in the {\code IC5} module is based on the ``Model with Order 3 Power Law'' proposed by \citet[][their section 6.2; hereafter the M2 model]{Meylan2018}, which assumes the loss of wave energy is proportional to the horizontal ice velocity squared times the ice thickness. The attenuation rate is given by
\begin{equation}
Expand All @@ -52,4 +52,4 @@ \subsubsection{~$S_{ice}$: Damping by sea ice (effective medium models)} \label{
%
\cit{IC5VEMOD} {the sea ice model to be selected: 1 - {\code EFS}, 2 - {\code RP}, 3 - {\code M2}; Default=3 (i.e., \textbf{the {\code M2} model is chosen}).}
\end{clist}
The first 6 parameters were introduced to improve the stability of the numerical solver for the EFS model \citep[the solver may fail for small wave periods in some rare cases, particularly for shallow water depth $d$ and low $G$; see][]{Liu2020}. Nonetheless, since version 7.12, the M2 model becomes the default option and these limiters are therefore not used by default.
The first 6 parameters were introduced to improve the stability of the numerical solver for the EFS model \citep[the solver may fail for small wave periods in some rare cases, particularly for shallow water depth $d$ and low $G$; see][]{Liu2020}. Nonetheless, since version 7.12, the M2 model becomes the default option and these limiters are therefore not used by default.
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