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The non‐conservation of potential vorticity by a dynamical core compared with the effects of parametrized physical processes

Abstract:
Numerical models of the atmosphere combine a dynamical core, which approximates solutions to the adiabatic, frictionless governing equations for fluid dynamics, with tendencies arising from the parametrization of other physical processes. Since potential vorticity (PV) is conserved following fluid flow in adiabatic, frictionless circumstances, it is possible to isolate the effects of non‐conservative processes by accumulating PV changes in an air‐mass‐relative framework. This ‘PV tracer technique’ is used to accumulate separately the effects on PV of each of the different non‐conservative processes represented in a numerical model of the atmosphere. Dynamical cores are not exactly conservative because they introduce, explicitly or implicitly, some level of dissipation and adjustment of prognostic model variables which acts to modify PV. Here, the PV tracers technique is extended to diagnose the cumulative effect of the non‐conservation of PV by a dynamical core and its characteristics relative to the PV modification by parametrized physical processes. Quantification using the Met Office Unified Model reveals that the magnitude of the non‐conservation of PV by the dynamical core is comparable to those from physical processes. Moreover, the residual of the PV budget, when tracing the effects of the dynamical core and physical processes, is at least an order of magnitude smaller than the PV tracers associated with the most active physical processes. The implication of this work is that the non‐conservation of PV by a dynamical core can be assessed in case‐studies with a full suite of physics parametrizations and directly compared with the PV modification by parametrized physical processes. The non‐conservation of PV by the dynamical core is shown to move the position of the extratropical tropopause while the parametrized physical processes have a lesser effect at the tropopause level.
Publication status:
Published
Peer review status:
Peer reviewed

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Publisher copy:
10.1002/qj.2729

Authors

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Institution:
University of Oxford
Division:
MPLS
Department:
Physics
Sub department:
Atmos Ocean & Planet Physics
Role:
Author
ORCID:
0000-0002-6744-7785


Publisher:
Royal Meteorological Society
Journal:
Quarterly Journal of the Royal Meteorological Society More from this journal
Volume:
142
Issue:
696
Pages:
1265-1275
Publication date:
2016-02-05
Acceptance date:
2015-12-16
DOI:
EISSN:
1477-870X
ISSN:
0035-9009


Keywords:
Pubs id:
pubs:734264
UUID:
uuid:52c6908f-154c-4eb8-b405-8bc22e5f6951
Local pid:
pubs:734264
Source identifiers:
734264
Deposit date:
2018-03-20
ARK identifier:

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