WG3a+3b: Organization of work related to ConSAT
Chair: Matthias Raschendorfer
All |
Preparation, Welcome |
09:00-09:10 |
Matthias Raschendorfer |
Action-plan and current state of ConSAT |
09:10-09:30 |
Contrasting particular ConSAT-issues (each introduced by Matthias Raschendorfer)
with associated other work, reported by: M. Köhler, L. Schlemmer and JM. Bettems |
Martin Köhler |
Additional Roughness by change of land-use, Special SSO-Tuning (by Günther Zängl) |
09:30-09:45 |
Linda Schlemmer |
Further development of STIC (e.g. Thermal SSO), Parallel development of a TKESV scheme |
09:45-10:00 |
Martin Köhler |
Surface-layer shear amplification: Adaptive Parameter Tuning (by Günther Zängl), Ocean
Coupling and Mixed Upper Ocean
Layer ▼ |
10:00-10:20 |
Jean-Marie Bettems |
Dynamic Surface-Smoothing by snow, possible issue also for follow-up of SAINT? |
10:20-10:30 |
Jean-Marie Bettems |
Closing Water-budget related to vert.-diff. of hydrometeors, possible issue also
of WG3b in general? |
10:30-10:40 |
coffee break |
Linda Schlemmer |
Revised TERRA with implicit treatment of surface processes, Modularization of current
TERRA code (by Roland Wirth) |
11:00-11:15 |
Matthias Raschendorfer, Jean-Marie Bettems |
Prepared implicit mixed phase interception and semi-transparent cover-layer, Related
measures by Günther Zängl (Matthias Raschendorfer), Related planning within WG3b
(Jean-Marie Bettems) |
11:30-11:45 |
Matthias Raschendorfer, Linda Schlemmer |
Modularization and cleaning of turbulence code, BRIDE-project within WG2 |
11:45-11:55 |
All |
Final Discussion about questions like:
- Are there inherent contradictions, and have we ideas towards a harmonization?
- What are the true open problems, and can we arrange all the related efforts under a
leading concept?
- How can we organize a workflow of complementing contributions to the model, avoiding
double work as well as undesired interference?
|
11:55-12:30 |
WG3a+3b: Considering the role of COSMO (as a consortium) regarding development of model physics
in general
Chair: Jean-Marie Bettems, Matthias Raschendorfer
Discussion about the role of COSMO WGs 3a,b (under the roof of COSMO SMC) in
the interplay with ICON authorities, National Services, Research Centers and their
consortia (such as CLM): |
Jean-Marie Bettems, Matthias Raschendorfer |
Introduction and personal perspectives. |
14:00-14:15 |
All |
Discussion about questions like:
- Could the SCM still be a place for
- compiling a coherent and consistent development and implementation plan for short to
longerrange from all desired initiatives for model development?
- coordinating the order and priorities of code-implementations, aiming to minimize
overall work and mutual disturbances, as well as to optimize efficiency of individual
engagement? -
- Should the WG3ab leaders (or delegates) be included into the non-technical gate-keeping
process under GitLab for ICON-nwp as regards a review of content?
- Should, perhaps, new physics WGs be established according thematically connected issues,
which explicitly include developers outside of COSMO/NWP (such as climate people and
ICON developers in general)?
- Should, in contrast, the physics WGs (a part of COSMO-SMC)
- restrict to particular COSMO/NWP issues?
- and provide an overview of other development at the most?
- Should, perhaps, a kind of “core model-development” group be established (dealing with
the matters of our WGs 2,3ab) and should this be closer connected with the already
existing ICON-developer group?
- Should SMC also organize general aid for special problems or burden related to model
development in the sense of a proper division of work?
|
14:15-15:30 |
WG3a+3b: Organization of technical support for coding of new physics development (e.g. related
to BuildBot-testing and GPU-porting)
Chair: Jean-Marie Bettems, Matthias Raschendorfer
Towards developing a common understanding of model developers about the
current needs and shortcomings regarding the process of finally getting a larger development
on top of already operational code into the master-code, facing the
- large and further developing technical overhead of the ICON code, e.g., due to
GPU-facilities
- high and still increasing update rate of the master code and the BuildBot
test-infrastructure
- implementation of not tunable (particularly empirical) extensions apart from consistent
parameterization strategies
- large formal code reorganization, running in parallel (organized and planned by
ICON groups)
- growing list of coding standards (formulated and agreed by ICON groups)
- obligatory readiness of the code for various computer systems, methods of parameter
variation or applications apart from NWP
- alternative non-operational parameterization schemes for the same purpose with all their
overhead and special requirements
|
Jean-Marie Bettems, Matthias Raschendorfer |
Introduction and report about personal experiences |
16:00-16:15 |
all |
Other individual reports about related experiences |
16:15-16:30 |
all |
Discussion about wishes like:
- Alternative parameterizations → Single, consistent code with upgrade options
- Empirical extensions: Hard-coded with fix numbers → Adapting to new, more
advanced parameterizations.
- Better arrangement with running code-development, when introducing extensive
modifications of technical overhead (such as ACC-directives) into the related
master-code
- Adaptation of related review/gate-keeping
- Taking-over of related modification in development branches by those actions as well,
if desired
- Technical support: mandatory part of future action-planning
- Better division of work to associated experts within the community:
- Support at using GitLab efficiently
- Support, if debugging is necessary on external machines
- Support at achieving readiness of new development for GPU
- Adaptation of too sensible BB-tests, failing due to pure difference of rounding
errors.
- Providing tools helping to prescind from minor modifications (such as blanks and
comments) for review with GitLab
- Support of non-technical gate-keeping by factual experts of related matters
|
16:30-17:30 |
ALL |
Time-buffer or possibility to join (at least the final discussion of) the parallel WG6
session just about technical issues (ICON-SCA/C) |
17:30-18:00 |
WG5
Chair: Flora Gofa
F. Fundel |
Presentation of FFV2 updates, conditional verification with roughness length |
10:00-10:15 |
F. Fundel |
Spatial verification update from
SINFONY ▼ |
10:15-10:30 |
P.Kaufman |
Performance differences between COSMO-1E and
ICON-CH1-EPS ▼ |
10:30-10:45 |
coffee break |
M. S. Tesini |
Model performances during the flood events of May 2023 in Emilia-Romagna
region ▼ |
11:00-11:25 |
F. Fundel |
ML Weather Fronts
Prediction ▼ |
11:25-11:50 |
N. Vela |
Precipitation FSS for COSMO
CP ▼ |
11:50-12:15 |
F.Sudati |
Comparing Cosmo-IT and
ICON‐IT ▼ |
12:15-12:25 |
coffee break |
J. Linkowska |
Comparing ICON-PL/COSMO-CE- PL |
14:00-14:10 |
F. Gofa, D. Boucouvala |
ICON-GR 2mT and heat stress
forecasts ▼ |
14:10-14:20 |
P. Khain |
IMS verification
report ▼ |
14:20-14:30 |
M. Bogdan, B. Maco |
NMA verification report |
14:30-14:40 |
WG5/EPOCS
Chair: Joanna Linkowska
J. Linkowska |
Introduction to PT EPOCS ▼ |
16:00-17:10 |
Marcin Grzelczyk |
PWS databases survey and
exploitation ▼ |
17:10-17:25 |
Francesco Sudati, Massimo Milelli |
Analysis of the mobile PWS sensors: testing QC proprieties of a new mobile weather sensors
from Meteotracker (FS ▼
and MM ▼ |
17:25-17:40 |
Katarzyna Ośródka, Jan Szturc, Anna Jurczyk |
Development and testing automatic QC methods based on the RainGaugeQC algorithms
developed at IMGW‐PIB ▼ |
17:40-17:55 |
Elena Oberto |
Testing and application of the open source software package TITAN for a quality
control of ground data ▼ |
17:55-18:10 |
Anna Jurczyk, Jan Szturc, Katarzyna Ośródka |
Processing different rainfall data sources |
18:10-18:25 |