A comparison between vertical mixing parameterizations in the Levantine Sea

The goal of this thesis was the study of an optimal vertical mixing parameterization scheme in a mesoscale dominated field characterized from a strong vorticity and the presence of a layer of colder, less saline water at about 100 m depth (Atlantic Waters); in these conditions we compared six different experiments, that differ by the turbulent closure schemes, the presence or not of an enhanced diffusion parameterization and the presence or not of a double diffusion mixing parameterization. To evaluate the performance of the experiments and the model we compared the simulations with the ARGO observations of temperature and salinity available in our domain, in our period of interest. The conclusions were the following: • the increase of the resolution gives better results in terms of temperature in all the considered cases, and in terms of salinity. • The comparisons between the Pacanovski-Philander and the TKE turbulent closure schemes don’t show significant differences when the simulations are compared to the observations. • The removing of the enhanced diffusion parameterization in presence of the TKE turbulent closure submodel doesn’t give positive results, and show limitations in the resolving of gravitational instabilities near the surface • The k-ϵ turbulent closure model utilized in all the GLS experiments, is the best performing closure model among the three considered, with positive results in all the salinity comparison with the in situ observation and in most of the temperature comparisons. • The double mixing parameterization utilized in the k-ϵ closure submodel improves the results of the experiments improving both the temperature and salinity in comparison with the ARGO data.

Submesoscale features in regions with different baroclinic deformation radius

In questo studio, un modello nidificato "child" ad alta risoluzione (risoluzione 1/48°) è ottenuto attraverso la piattaforma SURF. Il modello "child" è ottenuto tramite "downscaling" dei campi medi giornalieri dal modello globale "parent" (1/12°). Questo permette di osservare le caratteristiche della sottomesoscala in due regioni dell'oceano Atlantico settentrionale, Azzorre e Bermuda, dal 4 al 12 gennaio 2021. Questa tesi si propone di condurre un'analisi preliminare della relazione fra il raggio di deformazione baroclino e l'esordio dell'attività di sottomesoscala, nelle regioni di interesse. A questo scopo, vengono effettuati molti confronti fra i campi risultanti dal "parent" e dal "child". In particolare, ci concentriamo sulla Mixed-Layer Instability (MLI) studiata attraverso variabili come la Mixed-Layer Depth (MLD), la vorticità relativa, le velocità orizzontali e verticali, l'energia cinetica e la frequenza di Brunt-Vaisala. Dai risultati, mentre il modello "parent" sembra inadeguato, quello "child" è in grado di rilevare la MLI e la presenza di filamenti e scie topografiche in entrambe le regioni, riproducendo meglio le correnti orizzontali e verticali alla sottomesoscala. Ciò fornisce una connessione tra mesoscala e sottomesoscala: mentre nelle Azzorre la MLI sembra svolgere un ruolo chiave nella ristratificazione della colonna d'acqua, lo stesso non sembra nelle Bermuda dove i vortici di mesoscala sono più ampi, influendo maggiormente sulla stratificazione verticale. Qui, i processi di ristratificazione sembrerebbero correlati alle mesoscale piuttosto che alle sottomesoscale. La MLI giocherebbe comunque un ruolo nella generazione di correnti alla sottomesoscala, insieme ad altri processi come la frontogenesi e le scie topografiche. In conclusione, il valore del raggio di deformazione baroclino non sembra influenzare l'attivazione dei processi di sottomesoscala, mentre sembrerebbe determinare l'importanza della MLI nel processo di ristratificazione.

Analysis of evening and morning transitions in complex terrain: MATERHORN campaign 2013

A field study of thermal circulation over very gentle slope is described for a specific day characterised by weak synoptic conditions. The emphasis was on morning and evening transitions, but measurements cover the entire day; therefore a brief analysis is performed to represent the general thermal circulation pattern. Both transition periods are characterised by complex dynamic behaviours. During evening transition, the upslope flow has got through a stagnation condition characterised by wind velocity U<0:5 m=s. Only when the stagnating air has become negative buoyant, the flow is allowed to pour downslope like a slab. Some features of front formation has been found during the transition development, such as delay time of downslope flow start up along the slope, and the presence of positive turbulent kinetic energy at the onset of the motion. Eventually the observed evening transition has followed a mixed mechanisms, with features from different models. Therefore the Rayleigh number seems not to be a good criterion by which parametrise evening transition itself. Morning transition is characterised by destruction of nocturnal temperature inversion and the onset of upslope flow. Inversion destruction can be described in terms of CBL growth at surface and inversion decent from the top of the layer. KH has found to be a good indicator of inversion breakup, if used as parameter to study the inversion breakup in terms of temperature reversal. After the inversion breakup, buoyancy and mechanical productions supply the flow with the necessary energy to start the upslope wind. More quantitative analysis are provided by the study of stability parameters and turbulent kinetic energy budgets. Gradient Richardson number has been used in this terms, finding that a mixed SBL-CBL behaviour dominates the most of the observed layers. Tke budget has shown high turbulent behaviour during morning transition while the evening transition has developed entirely in laminar condition, apart from short intermittent turbulent events.