Reports

Research Stay in Perth by Mira Schmitt (Oct 23)

At the end of last year, I spent two months in Perth, Western Australia, to work on a collaborative project with Jen-Ping Peng, who was a PhD in TRR181’s first phase and is now a PostDoc in the working group of Nicole Jones at the Indian Ocean Marine Research Centre of the University of Western Australia. For the most part, my stay in Perth was covered by the Australia–Germany Joint Research Cooperation Scheme, with the TRR kindly providing some additional financial support. The above scheme is an initiative of Universities Australia and the German Academic Exchange Service (DAAD) for the support of international academic cooperation. Early-career researchers from Australia and Germany are encouraged to hand in proposals for a joint research topic, and, if approved, the grant covers the expenses for a research stay at the partner institute. For our project, Jen-Ping and I decided that we want to combine our two fields of research and investigate the interactions of diurnal warm layers, submesoscale fronts and other turbulent processes in the surface mixed layer. For this, we firstly extended the 1D turbulence model GOTM to include 3D frontal effects and validated our model results by comparing them to published LES studies. Then, we used our model to recreate measurements taken previously during two campaigns in the Baltic Sea and the Indian Ocean and use the results to understand the governing processes involved. We found nice agreements between the measurements and our simple model and are planning on publishing two joint papers on these topics.

But besides the work aspect, Western Australia was also a great place to explore and spend time. Jen-Ping was an excellent host (I think we went to every great Asian restaurant in all of Perth) and the weather was pleasant from beginning to end (basically nothing but sunshine for two months). I stayed in a researcher accommodation on campus, which is located a few kilometres away from the city centre directly at the Swan river estuary with lots of green areas and beautiful old trees. Moreover, I got to go on two nice road trips up and down the coast, explore the Margaret River wine region, see quokkas on Rottnest Island and snorkel in the beautiful Ningaloo Reeve national reserve with an infinite amount of fish, stingrays and even a big sea turtle. I also got to see a living colony of stromatolites, microorganisms that are believed to be the oldest form of life on earth dating back 3 billion years, and that can only survive in hypersaline estuaries like Shark Bay in Western Australia. And while there were a few snake and spider sightings, I didn’t have the heart to look up their level of toxicity, so I like to believe it was all safe and sound.

I can definitely recommend looking into the Joint Research Cooperation Scheme (it exists not only between Germany and Australia, but also other countries) and would strongly encourage others to take the opportunity to extend their network and travel, maybe to Perth, it’s a lovely corner of the world. I would like to thank Jen-Ping, Nicole Jones and all other members of this working group for hosting me, showing interest in my research and teaching me about their fields of research.

Diurnal Warm Layers and Rain Layers: Dynamics, Turbulence and Atmospheric Feedbacks

My work so far has been to simulate idealized cases using a 1D turbulence model.

Mira Schmitt, PhD L4

Hello everyone, my name is Mira, I am a PhD at the Institute for Baltic Sea Research in Warnemünde and working in subproject L4, supervized by Lars Umlauf. To start off with something about myself: I studied physics at the University of Göttingen with a focus on Astro- and Geophysics during my masters. After an internship on sea ice physics at the University of Otago in New Zealand, I studied double-diffusive convection during my master thesis.

I love hiking and backpacking, so before, during and after my studies I spent a lot of time abroad, travelling, discovering new countries and meeting interesting people. When the pandemic started I had to change my plans and, by a chain of coincidences, started this phd position, which I am very happy about. I very much enjoy to live this close to the ocean and I spend a lot of time by the beach.

The focus of my project is on diurnal warm layers and rain layers on the ocean surface. These thin, stratified layers influence air-sea fluxes and turbulence in the ocean interior, but are usually not resolved in climate models. My work so far has been to simulate idealized cases using a 1D turbulence model. With that I can identify the non-dimensional parameters that govern these processes and perform parameter space studies, which can be the basis for a parameterization. I also work in close collaboration with Mira Shevchenko and Cathy Hohenegger, who study diurnal warm layers and their effect on the atmosphere using the coupled ICON model.

An In-Depth Study of Diurnal Warm Layers: Quantification of Air-Sea Interactions

I am fascinated by such theoretical results but also by their various fields of application.

Mira Shevchenko, Postdoc, L4

In July 2021 I joined the TRR 181 as a postdoctoral researcher in the project L4, “Energy-Consistent Ocean-Atmosphere Coupling”. Within this project I am studying the phenomenon of diurnal warm layers (DWLs) in the ocean. It describes the warming of the sea surface in certain areas during daytime (by up to 2K, though in particular cases also higher fluctuations have been observed) compared to the surrounding ocean that usually keeps an almost constant surface temperature.

From the point of view of air-sea interactions the appearance of DWLs is of particular interest, since such differential heating can promote a sea breeze like convective movement and, as a result, serve as a cloud building mechanism. Moreover, as such warm spots appear due to solar radiation, one can also expect a feedback behaviour caused by an increase in the cloud cover. 

The presence of DWLs as well as their influence on the cloud amount is well documented in the literature, at least in the qualitative sense. Moreover, this phenomenon has been confirmed in idealised simulation studies. However, most modern global coupled simulations do not capture this mechanism, since it requires a high vertical resolution of the sea levels in order to correctly represent the heat transport (involving only about 20m in the vertical), but also a high horizontal resolution in the atmosphere that would permit to directly resolve convection. My work in the project consists in implementing a simulation that would incorporate both these features. This has been made possible thanks to recent model development advances for the ICON models at the Max Planck Institute for Meteorology. A subsequent analysis of the output will improve the understanding of the phenomenon itself, in particular permitting to quantify the feedback mechanisms, but it will also clarify how significant of an influence the correct representation of DWLs has on the global cloud amount, and, as a consequence, on the climate described by the simulation. Such results would, moreover, enable a parametrisation of this phenomenon such that it can be included in lower resolution models in order to improve their performance.

Within the project L4 I work under supervision of Cathy Hohenegger at the MPI for Meteorology and collaborate mainly with Nils Brüggemann, Lars Umlauf and Mira Schmitt who already implemented a set of thin layer ocean simulations and contributed significantly to my understanding of the mechanisms involved. 

Prior to joining the TRR 181 I spent several years doing research in Probability Theory. After obtaining my Master’s degree at the HU Berlin I went on to complete my PhD at the TU Dortmund with a research stay at the University of Lille. During my doctorate I studied stochastic (partial) differential equations driven by random processes or fields with long memory, i.e. such that the increment correlation decays only slowly over time. An example is the fractional Brownian motion. Using techniques from the Malliavin-Stein toolkit (providing a definition for multiple stochastic integrals with respect to Gaussian processes and many limiting results for those) I proved in several collaborations limit theorems for certain functionals of the solutions of such equations. From the practical point of view, this enabled me to derive results in mathematical statistics and provide estimators for different quantities in such equations as well as show their asymptotic properties.

After defending my dissertation I stayed at the TU Dortmund as a postdoctoral researcher. During this time I studied (in another collaboration) random fields on a sphere. Such objects are used in cosmology to describe cosmic microwave background, but they can also be applied to analyse other random spherical observations such as, for instance, temperature defects.

I am fascinated by such theoretical results but also by their various fields of application. I hope to be able to use some of the models that I studied in order to assess the impact of DWLs and/or to describe other phenomena in the atmosphere and ocean that would help advance the understanding and modelling of physical processes on different scales.

The Impact of Submesoscales on the Air-Sea Exchange

I will investigate on the potential impact of submesoscale dynamics on the sea surface temperature or the influence of wind on instabilities at ocean fronts.

Moritz Epke, PhD, L4

Hello everyone, my name is Moritz Epke and I am pleased to give you a small impression of my work at TRR. I am part of the subproject L4 „Energy consistent ocean atmosphere coupling”, which investigates small scale and balanced processes and their impact on feedback mechanism between atmosphere and ocean. Before I go into more detail, maybe a few words about my background. I moved to Hamburg to study theoretical mechanical engineering at the Hamburg University of Technology. My interest in the physics of fluids grew and grew through my studies and drove me to focus on this topic and related numerical solution approaches. In my thesis I developed and implemented a lattice Boltzmann scheme to efficiently simulate non-isothermal flows, which I benchmarked on standard testcases like Rayleigh-Bénard convection in a cavity and which I used to simulate the internal cooling of a turbine blade by a turbulent flow.

While most engineering applications have setups with scales from less than a centimeter as in a pipe flow, or up to a few hundred meters as in a large ship, the ocean and the atmosphere have scales that are orders of magnitude higher. Even if we make use of clever approximation techniques to simplify the governing equations in order to reduce the computational effort, we can only carry out coupled climate simulations with roughly tenkilometer (ocean) grid spacing on a modern supercomputer. In such a simulation an 80km ocean eddy would only be coarsely resolved. The computational surplus to resolve more scales in long-term simulations is simply too high. What cannot be resolved is usually parameterized or neglected. If parameterized, a model is developed which is based at best on a physical relationship between the relevant parameters. These parameterizations are then tested and optimized in idealized or regional setups. If now such parameterizations or insufficient parameterizations are used, the model is most likely subject to biases. These types of biases might have a strong impact on the energy consistency.

In the first phase of my PhD I am using an ICON submesoscale telescope simulation, which is based on an unstructured grid and allows us (for a short time period) to use an extremely fine spatial resolutions of up to 600m in the focus region. If we look again at an 80km ocean eddy, which is now well resolved, we can see small scale coherent structures that we associate with the submesoscale (see figure) and define to be smaller than the first baroclinic Rossby radius of deformation. It is an objective to understand and quantify the impact of submesoscale dynamics like baroclinic and symmetric instabilities on the downward heat and energy transfer and their role for ocean-atmosphere interactions. Here, I will investigate on the potential impact of submesoscale dynamics on the sea surface temperature or the influence of wind on instabilities at ocean fronts. Therewith, I aim to obtain a better understanding of submesoscale dynamics and their role in the coupled ocean-atmosphere system. This improved understanding might ultimately lead to improved parameterizations and therewith less biases in the coupled climate models.