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 |