Freediving with Nik Linder, world record holder in freediving under ice and dynamic apnea
Today I was honoured to step into a discussion with Bauer crew experts about the risks of ice diving and polar scientific research from their past expeditions.
Bauer Compressors, founded in Munich in 1946 is recognised as the world’s foremost innovative designer and manufacturer of high and low pressure systems, including air and gas treatment and measurement technology for all industrial applications. Bauer is the main supplier for the diving activities in Düsseldorf Boot 2023. The tower consists of slim steel struts and large acrylic glass surfaces, and has a capacity of 200,000 liters of water.
Bauer Compressors supports institutions in marine research with the provision of compressor systems and compressor maintenance, including the University of Rostock, marine biology research as part of the Polarstern missions, the research and media ship Aldebaran and the Australian NGO “Great Barrier Reef Legacy”, which researches coral death on the Great Barrier Reef.
Polarstern, Europe’s largest scientific vessel and icon of German polar research, is celebrating its fortieth anniversary since it started its first expeditions with polar research ships worldwide. It has carried out over 130 successful expeditions in the Arctic and Antarctic and has been a temporary home for thousands of researchers from Germany and around the world.
The use of new underwater technologies also plays a major role in planning the successor to the Polarstern. After the federal budget was passed in 2022, the BMBF enabled the AWI to start the Europe-wide tender for the construction of a new research icebreaker, scheduled to start the service in 2027. Polarstern is also intended to become an ambassador for sustainable shipbuilding and energy supply based on hybrid diesel-electric propulsion.
The energy of a closed system is steady until converted into other forms, such as when kinetic energy is transferred into thermal energy or vice versa, but it is never lost. However, this fundamental principle of natural science is often still a problem for climate research.
For example, in the case of the calculation of ocean currents, where small-scale vortices as well as mixing processes they induce need to be considered, without fully understanding where the energy for their creation originates from. Waves on a larger scale can disintegrate into small structures driving large movements. All these processes are important for the Earth’s climate and determine how temperatures will rise in the future.
Expedition M180 SONETT (Synoptic Observations – a Nested approach to study Energy Transfer & Turbulence in the ocean) is a key part of the ocean observations in the second phase of TRR181 ‘Energy transfers in Atmosphere and Ocean’. The expedition take scientists to an ocean region where they can observe many processes that affect energy fluxes in the ocean and the ocean’s exchange with the atmosphere.
Researchers from MARUM – Center for Marine and Environmental Sciences at the University of Bremen, the University of Bremen, the University of Hamburg, the Institute for Baltic Sea Research Warnemünde (IOW) and the Helmholtz Center Hereon are involved.
The working area is located southeast of the Walvis Ridge in the eastern South Atlantic. In this region, the so-called Agulhas eddies, which are formed at the southern tip of Africa and migrate northward through the Atlantic, meet internal tides generated at the Walvis Ridge, and affect the propagation of internal tidal waves. The eddies form fronts and so-called filaments at their edges. Filaments are structures that form where different water masses meet. They look like elongated fingers on satellite images. The planned observations include surface fluxes and waves, surface layer processes, mesoscale and submesoscale variability, horizontal mixing, internal wave energy fluxes, the interaction between internal waves and eddies circular current, and the energy dissipation in the ocean interior.
The observations will be complemented by runs of a high-resolution ocean circulation model with tidal forcing (ICON SMT-WAVE) from the Max Planck Institute for Meteorology in Hamburg, Germany, which will allow to contextualize the observations, understand processes, and characterize the energy balance of this ocean region.
The expedition started on February 23, 2022 in Montevideo (Uruguay), on April 14 the team returned with METEOR in Cape Town (South Africa). Here, the researchers reported life and work on board in a logbook. Reference: https://www.marum.de/en/Discover/Logbuch-M180.html
Excerpts from the M180 SONETT logbook:
15 March 2022: A Drifting Passenger
“On Wednesday at the CTD station, we pulled up a catch: a worm-like animal out of the water. The semi-transparent tube looked almost plastic and had interesting nubs of different sizes growing on its mantle. No one knew what we had unknowingly caught there. The first idea was that it could be a sea-cucumber. After a while, however, it was discovered that it was called a ”Pyrosome”, a colony consisting of several thousand individual animals. Because the individual tunicates can reproduce via cloning, the colony can regenerate injured parts or continue growing after being broken apart. Pyrosomes form an important biological substrate in the water column that other animals use for settlement.
Especially during the night watches we noticed that these tunicates can often be seen close to the water surface. Pyrosomes migrate up and down the water column daily to feed in the productive upper marine layers at night. At dusk, they migrate back to deeper water layers. During this migration, they actively transport their feces to these depths, while also releasing carbon through respiration.
Pyrosomes have an elongated shape with one open and one closed side. Credits: Nikos Lymperis
11 March 2022: Little Things, Big Impact
Attached to the bottom of the ship and running constantly: the vessel- mounted ADCP fires pulses of sound down into the ocean and listens for any echoes coming back. Based on how long an echo takes to return, and if the sound of it changed on the way, the speed and direction can be calculated of water movements at different depths below the ship. If anything other than the water returns an echo measures aren’t accurate.
Shortly after sunrise (yellow dashed line) a large gap in our signal grows around 300 metres depth then closes shortly after sunset (black dashed line). At the same time our strongest signals (anything above the dark line) move closer to the surface. This is due to the movement of plankton. Graph: Ryan Mole
By looking at the strength of the signal a strange pattern emerges. During the night, from down to 600 meters the echo becomes too quiet to hear. During the day, a gap in our signal starts to emerge just after sunrise and closes just after sunset. The strength of our signal increases near the surface whilst at the same time we get no echoes bouncing back from deeper waters, particularly around 300 meters.
Due to the movement of microscopic plants and animals known as plankton, which are almost too small to see with the eye but are excellent for bouncing back an echo. Every day they migrate for hundreds of meters: to the surface 100 meters where there is light and they can feed and photosynthesise by day, and down in deep water by night hide from predators and get rid of waste. This migration happens every day across much of the ocean and globally is an important route for getting nutrients and carbon into deeper waters.
Microorganisms in sea ice and the water column are cornerstones of this ecosystem and play critical roles in providing feedback to climate and maintaining food chains that are central to protection and ecosystem services. Due to their rapid adaptability to environment, marine microorganisms are biological indicators of the environment.
From Düsseldorf Boot 2023, the world’s largest water sports trade fair with 1,900 exhibitors from 60 countries, presenting their products and the most important awards for sailing and motor yachts in Europe.