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von Dr. Birgit Quack, GEOMAR Helmholtz-Zentrum für Ozeanforschung Kiel

Es gibt zwei Bereiche in unserer Atmosphäre, in denen das Spurengas Ozon besonders wichtig ist: in der Stratosphäre und in der Grenzschicht an der Erdoberfläche. In der oberen Region unserer Atmosphäre, der Stratosphäre, entsteht Ozon durch den Zerfall von Sauerstoff im Sonnenlicht und wirkt als wichtiger UV-Strahlenschutz für das Leben auf der Erde. Es wird durch Radikalreaktionen von Halogenen wie Chlor, Brom und Jod, die in verschiedenen Formen in unserer Atmosphäre vorkommen, rasch zerstört. In den 1980er Jahren trat ein großes Ozonloch auf, das mit den langlebigen Fluorchlorkohlenwasserstoffen in Verbindung gebracht werden konnte, die in den 1990er Jahren durch das Montrealer Protokoll verboten wurden. Seitdem nehmen das Ozonloch über der Antarktis und das Ozon in der oberen Stratosphäre im Allgemeinen langsam wieder zu. In der unteren Stratosphäre der Tropen nimmt es jedoch weiterhin ab. Das Oberflächenozon hingegen nimmt zu, was auf die Luftverschmutzung zurückzuführen ist, insbesondere auf die Verbrennung fossiler Brennstoffe.

Abb.1: Oberflächenozon am Sonntag, 12. Mai, 14 Uhr Ortszeit (7 Uhr UTC). (windy.com)

Unter windy.com kann jeder weltweit, der Zugang zum Internet hat, eine globale Karte von Oberflächenozon und lokale Werte für jeden Ort der Welt finden (Abbildung 1). Oberflächenozon, das auch ein Treibhausgas ist, wird auf natürliche Weise bis zu einer Hintergrundkonzentration von 10-40 µg/m3 produziert. Da es ein starkes Oxidationsmittel ist, kann es in höheren Konzentrationen Augen und Lunge reizen. Für Städte, in denen die Umgebungskonzentrationen im Sommer über 100 µg/m3 ansteigen und empfindliche Menschen schädigen können, wurden gesetzliche Grenzwerte und Warnsysteme eingerichtet.

Abbildung 1 zeigt die Ozonkonzentration an der Oberfläche in dem Gebiet, in dem unsere Fahrt SO305 im Golf von Bengalen stattfand. Sie ist tagsüber über ganz Indien sehr hoch, und es ist auch offensichtlich, dass die Ozonkonzentrationen an den Küsten und zum offenen Ozean hin stark abnehmen. Dies ist hauptsächlich auf eine aktive Halogenchemie zurückzuführen, die das Ozon über den Ozeanen zerstört, verursacht durch natürliche halogenierte flüchtige Verbindungen, die in den Ozeanen durch Sonnenlicht, Phytoplankton und chemische Reaktionen gebildet werden. Zu diesen Verbindungen gehören Bromoform (CHBr3), Dibrommethan (CH2Br2), Methyljodid (CH3I), Dijodmethan (CH2I2), Jodchlormethan (CH2CII), Dichlorbrommethan (CHBrCl2) und andere. Sie gelangen in die Atmosphäre und setzen dort Halogene frei, die mit Ozon reagieren. Alle Verbindungen haben eine kurze Lebensdauer von Minuten bis zu weniger als sechs Monaten. Die industriellen Lösungsmittel Dichlormethan (CH2Cl2) und Chloroform (CHCl3) aus der Süßwasserchlorierung tragen ebenfalls zum Ozonabbau in der Atmosphäre bei. Die Verbindungen, die durch tiefe Konvektion in den Tropen in die Stratosphäre gehoben werden, setzen ihre Halogene in der unteren Stratosphäre frei, während sie sich zum Nord- und Südpol bewegen. So wirken sich die tropischen Prozesse global aus.

In den letzten vier Wochen waren wir nun im tropischen Golf von Bengalen, der 2001 als Hauptquelle für einige natürliche halogenierte flüchtige Verbindungen für die Atmosphäre entdeckt wurde, mit RV Sonne unterwegs.

Gaschromatographisch-massenspektrometrisches (GC/MS) Spülsystem zur Messung von flüchtigen halogenierten Kohlenwasserstoffen in Meer und Atmosphäre. Jule Ploschke, Julia Mickenbecker und Birgit Quack mit Wasser- und Luftprobenahmegeräten. (Foto: Hendrick Feil)

Jule, die ihre Masterarbeit zu diesem Thema schreibt, Julia, die zum zweiten Mal als studentische Hilfskraft auf der RV Sonne mitfährt und ich, die seit über 30 Jahren auf den Weltmeeren flüchtige Halogenkohlenwasserstoffe untersucht, brachten unser Analysesystem mit an Bord, das seit Beginn der Fahrt rund um die Uhr in Schichten von jeweils 8 Stunden reibungslos lief, wobei das Gerät jede Stunde eine neue Probe erhält. Wir haben Wasser aus der Tiefsee und dem Oberflächenozean und Luft aus der Atmosphäre entnommen (Abbildung 3). Die Luftproben werden von Elliot Atlas in den USA analysiert, mit dem ich seit 2002 in 15 Kampagnen zusammengearbeitet habe. Aus den Konzentrationen im Ozean und in der Atmosphäre berechnen wir den Gasaustausch zwischen Luft und Meer, und versuchen zu verstehen, wie die Verbindungen in der Region mit physikalischen und biogeochemischen Parametern zusammenhängen, und schätzen ab, wie sich die ozeanische Quelle und Senke in Zukunft entwickeln könnten und was dies für Ozon als Treibhausgas und als UV-Schild bedeutet.

Bei jeder Schiffsexpedition in den 30 Jahren, in denen wir die Ozeane bereisten, erforschte ein Team von Wissenschaftlern und Crew an Bord verschiedener Forschungsschiffe den Ozean als ein uraltes Zusammenspiel von Wasser, Chemikalien, Billionen von Bakterien und höheren Organismen, das durch die Schwerkraft, die Erdrotation sowie durch Sonnenlicht und den Mond beeinflusst wird. Die Biologie reagiert auf die Verteilung von nahrhaften Chemikalien im Wasser, das in enger Wechselwirkung mit der Atmosphäre steht, von der Meeresoberfläche bis zur Stratosphäre. Bei jeder Fahrt wurde ein kleiner Teil der Myriaden von globalen und regionalen geheimen Wechselwirkungen, die die Grundlage unseres Lebens bestimmen, entdeckt und veröffentlicht. Das alte Zusammenspiel wird nun durch menschliche Aktivitäten stark beeinflusst. Ich hoffe, dass sie das wechselwirkende Gleichgewicht nicht kippen, so dass künftige Generationen weiterhin die Chance haben, es tiefer zu entschlüsseln, um nachhaltig damit leben zu können.

Die letzte Luftprobe auf SO305. (Foto: Hermann Bange)

Meine letzte Fahrt konnte ich auf der RV Sonne, einem Starschiff der deutschen Forschungsflotte, mit einer professionellen Besatzung durchführen, die durch den reibungslosen Betrieb des Schiffes bis zum Hafen von Singapur wieder sehr gute Datensätze ermöglichte. In den nächsten Jahren werde ich vermutlich meine Datensätze hauptsächlich mit KI erforschen, um das meiste Wissen aus ihnen herauszuholen. Jule und Julia werden hoffentlich mehr Gelegenheiten finden, ihre Karriere mit Entdeckungsreisen auf dem Meer zu verbinden, da diese nicht nur Wissen fördern, sondern auch soziale Fähigkeiten wie Teamarbeit, Disziplin, Ausdauer, Rücksichtnahme und Toleranz entwickeln. Ich werde die täglichen Herausforderungen einer erfolgreichen Forschungsfahrt vermissen.

Birgit Quack, Singapur 18.05.2024

Hallo Halos in und über der Bay of Bengal

Ocean Acidification

New Friends, New Addresses

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The JOIDES Resolution (JR) was a renowned, international, scientific research ship. It was home to over 190 expeditions, each sailing for 60 days at a time without docking. Scientists and crew members from all over the world met to discover Earth’s secrets through studying ocean cores. Every two months the JR would get a new crew, sailing to an entirely new place. This once in a lifetime experience forms special and unforgettable social connections.

Since working on the JR I’ve kept those connections strong with snail mail. I have always been an avid penpal, so meeting new friends means new addresses to send my letters and postcards to. Experiences like sailing on the JOIDES Resolution or participating in programs like OCEAN CORE Academy is one of the ways I’ve met people from all over the world.

Now that the JR is retired, there is no more scientific research drilling being done through the International Ocean Discovery Program (IODP). But, there is still plenty to learn from ocean cores, and plenty of people to meet through programs like OCEAN CORE Academy (OCA). OCA is an annual summer opportunity from the U.S. Scientific Support Program (USSSP) that hosts undergraduates interested in geoscience related careers. Students can apply to this program for a chance to research and study data recovered from cores originally brought up by the JR, now located at the Gulf Coast Repository (GCR) in College Station, Texas. Students also practice forms of science communication with the guide of mentors. As a science communicator and fan of snail mail, I ran a craft night teaching students how to make and send science-themed postcards.

Fig. 1) students using watercolor to paint onto 4 by 6 inch board paper, a photo of a thin section slide is in the background. Photo by Dr. Leah Joseph.

For this project, we based the cover image of the postcards off of rock thin section slides. These slides are a slice of a hard rock or mineral that’s been glued to a microscope slide, sanded to 0.03 millimeter thickness, and polished. Thin section slides are used to identify grain size, shape, color, and other physical properties. This helps scientists understand the textural relationships between the rocks and determine the origin or evolution of the parent rock. Thin sections can also be helpful for identifying minerals using cross polarized light (XPL). XPL reduces light reflection and glare, commonly used for sunglasses and professional photography, but in a polarizing microscope, XPL is used to create a dark field causing certain minerals to appear brighter and more visible. Different colors are associated with different minerals, and as the stage of the microscope rotates, light passes through the slide in unique ways aiding scientists with identification. Identifying minerals can help scientists in understanding more about where the rocks came from and how old they are. These thin sections are not only informative, but are incredibly beautiful, making unique and stunning postcard covers.

     

Fig. 2) Examples of thin section slides under a XPL microscope, bronzitite (left) and gabbro (right). Sourced from here.

After the OCA students finished their paintings, my home-made “post card” stamps go on the back, a stamp gets added, and they’re ready to be mailed out. Although most OCA participants this year were U.S. based, they came from all over, ranging from Staten Island to San Francisco to Arizona to Connecticut. In addition to one mentor from New Zealand!  For many of these students this was their first time traveling on their own, and their first time forming long-distance connections. With these scientific postcards, OCA students can stay connected by reminding each other of the science they learned together. My experience on the JR taught me great things about geological research, but it also gave me life long connections that I cherish. Although the JR is gone, its legacy lives on in our memories and the ways we stay connected with friends. I’m grateful to know that even without an international ship, I’m still able to add friends to my address book.

     

Fig. 3) Examples of participant made postcards

Written by Kellan Moss

New Friends, New Addresses

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Ocean Acidification

Color Traditions with Munsell Soil-Color Charts

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Fig. 1) an open page of the Munsell Soil-Color Chart book

The Munsell Color Chart has been the national standard and official color system for soil research in the U.S. since the 1930s. For nearly 100 years, geologists and soil scientists have taken these color chip pages into the field to better understand the Earth they are studying, so it comes as no surprise that it is the standard for recording ocean cores brought up by the JOIDES Resolution.

Upon first glance, these charts may look like a page of free paint sample strips you can find at your local hardware store, but they are critical to classifying sediment and understanding the environments they came from and can cost several hundred dollars. The Munsell Color System is a method of numerically describing colors. It specifies colors based on hue, value, and chroma and measures them in a three dimensional space. Hue refers to the dominant color of the soil, value is the lightness of the color (scaled 0-10; 0 being black and 10 being white), and chroma is the intensity or saturation of the color.

Fig. 2) A 3D model representation of the Munsell Color System

There are five primary hues, red, yellow, green, blue, and purple, and five intermediate hues, which are a combination of primary hues such as yellow-red (YR) or green-yellow (GY). The hue of a color is represented as a ring and as the rings go up and down a vertical axis, the value of the color changes. As the color moves horizontally from the vertical axis, chroma or saturation becomes stronger or weaker. A color is specified by listing the three numbers or letters for hue, value, and chroma in that order. In the soil color chart, these number letter combinations correspond with a color. For instance, in figure 1, a 7.5YR 5/6 is also called “strong brown” (seen on the left page, bottom right). The names of colors used in weekly expedition reports are not arbitrary or subjective, they are specific and can be easily and accurately charted by anyone with a Munsell Chart reading the report.

Useful or Just Tradition?

The Munsell Color System has limitations. There are a distinct number of samples and the spacing between colors are large, making it difficult to measure thresholds. This inspired new color measuring methods to develop like CIELAB. Read more about CIELAB and what it means here (blog post “Color Science and Ocean Cores”). Changes to the Munsell system were made, doubling the number of hues in Munsell’s original book from 20 to 40, but CIELAB was already on its way to mainstream.

However, it’s still true that Munsell has been the soil color standard for nearly 100 years. That’s 100 years of geological and earth science research using this method of recording color. If scientists were to change to a system like CIELAB, it would mean having to constantly convert units when comparing previous research. Scientists compare and reference previous work all the time. Comparing sediment core colors from different sites can help support their own scientific findings. So switching to a different color recording method would mean converting all previous research. But is that a good enough reason to stick to tradition?

CIELAB creates a standard observer, which is an averaging of color matching that helps set a base value for recordings. This helps create the most accurate color reading on something such as an ocean core. Using color charts opens up the possibility for disagreements as no two human eyes see colors the same. And this really happens! In 2024 while aboard the JOIDES Resolution, EXP401 sedimentologists held long discussions about shades of grey they were recording differently.

Fig. 3) Photos of “The Great Grey Debate” on EXP401 by Dr. Patty Standring

Machines can record accurately and consistently, so why not switch to CIELAB? Well, expensive machines that use CIELAB, like the Section Half Multi-Sensor Logger (SHMSL) take anywhere from seven minutes to hours, recording only one core at a time. When on a two month cruise, pulling up hundreds of meters of core, time is crucial. Cores dry out and potentially change color as they dry, so it’s important to record fresh colors.

The color of a core can tell scientists so much information so quickly.

“Gradual color changes helped us to identify where we saw facies changes on a larger scale. There were very obvious cyclical color changes at Site U1385 that helped establish that the cores preserved a really good orbitally-driven sediment record. Color differences are also really useful when looking at different grain sizes that help identify turbidites and other sedimentary structures, and burrows from bioturbating organisms,” (Standring)

It’s important that scientists record these fresh colors as quickly and efficiently as possible. Although debates about the color grey can happen, these color discussions and international collaborations are what scientific research is all about. After 100 years, Munsell will stay the golden standard, not because it’s what we’ve always done, but because it’s still the best.

Written by Kellan Moss

Thank you to Dr. Patty Standring and Natacha Fabregas for help with this research

Sources:

Berns, R. S. (2016). Color science and the visual arts a guide for conservators, curators, and the curious. Los Angeles Getty Conservation Institute.

EXP 401 Sedimentologists: Dr. Patty Standring ad Natacha Fabregas

Featured Image: MerlinOne Archive

Fig. 1 Image: Here

Fig. 2 Image: Here

Fig. 3 Images: Dr. Patty Standring from EXP401

Color Traditions with Munsell Soil-Color Charts

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Ribbegople, Rippenqualle or Comb Jelly: Whatever You Call Mnemiopsis leidyi, You Should Be Concerned

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In early July at Kerteminde, most of the individuals I observed were longer than 10 cm, including one close to 15 cm. Their size, and their timing, deserve immediate attention.

⚠ One out of many large speciments I got from Kerteminde (Javidpour, July 2026)

It does not matter whether you call it ribbegople in Danish, Rippenqualle in German or comb jelly in English. The species is the same: Mnemiopsis leidyi. And what I have observed in Kerteminde this summer should concern us. During our current summer field course at the Marine Research Centre, I have repeatedly seen unusually large individuals of M. leidyi around the pier. Most of the animals I observed were longer than 10 cm, even bigger than the one I photographed.

Yes, yes, a pier observation is not a formal population survey….I know. We still need systematic sampling to determine the abundance, distribution and size structure of the population. Nevertheless, the observation is striking because both the size of the animals and the timing of their appearance are unusual, said by someone who is studying this species for the last 20 years.

This is happening earlier than expected

In previous years, the maximum population size of M. leidyi generally occurred several weeks later, mainly during August and early September. Our previous research, including work based on daily sampling, showed a clear seasonal development of the population. The timing varies among years and is influenced by environmental conditions, including winter temperature. Temperature is particularly important because it strongly affects the metabolism of M. leidyi. At warmer temperatures, individuals use their carbon reserves much faster and therefore require more food to maintain themselves and grow. This year, however, the pattern appears to be different. We are seeing very large individuals already in early July. We do not yet know whether this is a local aggregation, an unusually early bloom, transport from another area, particularly favourable feeding conditions or a combination of these factors. But it is a signal that deserves attention.

What does it take to grow by one centimetre?

It is tempting to ask how much energy an individual needs to add one centimetre to its body. The answer is not straightforward because one centimetre of length is not a fixed amount of biomass. Growing from 5 to 6 cm is not the same as growing from 14 to 15 cm…OK? However, we can make a rough carbon-budget calculation using a published relationship between the length and body-carbon content of M. leidyi:

Body carbon in milligrams = 0.0017 × body length in millimetres²·⁰¹³⁸

According to this relationship, an individual measuring 10 cm contains approximately 18.1 mg of carbon. At 11 cm, it contains about 21.9 mg. Adding this single centimetre therefore represents an increase of approximately 3.8 mg of body carbon. If we assume that the animal assimilates approximately 40% of the carbon it consumes, it would need to ingest at least ~10 mg of prey carbon to produce this additional tissue. Using an approximate value of 1 micrograms of carbon for a small copepod, this would correspond to more than 10,000 copepods.

For an already large individual growing from 14 to 15 cm, the estimated increase is approximately 5.3 mg of body carbon. At the same assimilation efficiency, that would require at least 13.3 mg of prey carbon: the equivalent of roughly 15,000 small copepods.

These calculations are only rough, conservative estimates. They are not complete energy budgets. They do not include the food needed for respiration, movement, reproduction, mucus production, excretion or unsuccessful feeding. The real prey requirement would therefore be considerably higher. The important point is that an individual measuring 15 cm represents a substantial transfer of material from the surrounding planktonic food web into gelatinous biomass. One additional centimetre is not “just” one centimetre.

Our students are tracing the food web

The timing of these observations coincides with our summer field course. The students are now collecting M. leidyi, fish, other gelatinous organisms and potential prey for stable-isotope analysis. By comparing carbon and nitrogen isotope values, we hope to obtain a rough picture of the relationships within the local food web. Carbon isotopes can help us trace the original sources of the material entering the food web, while nitrogen isotopes can provide information about relative trophic position.

This will not give us a direct photograph of one organism eating another. Stable-isotope values represent assimilated food over time, and their interpretation depends on appropriate baselines and turnover rates. Nevertheless, combined with information about size, abundance, prey availability and experimental feeding, they can help us understand where M. leidyi is obtaining its biomass and which organisms may be affected. …In simple terms, we are trying to determine who might be eating whom, and where this unusually large population fits into the food web.

Competition with fish is only part of the problem

The concern is not limited to competition for zooplankton. Mnemiopsis leidyi consumes copepods and other small planktonic animals that are also important food for pelagic fish. When the ctenophores are abundant, they can therefore compete directly with fish for prey. Our experiments have also demonstrated that M. leidyi can potentially feed directly on the early life stages of fish. In the study by my previous PhD student, the ctenophores captured and digested Baltic herring yolk-sac larvae. Predation was related to ctenophore size and was not simply eliminated when alternative copepod prey were available. This means that M. leidyi may/can affect fish populations in two ways: by consuming the food needed by fish and by consuming fish eggs or larvae directly.

A recent study by Lucila Sobrero and colleagues in Argentina, within the native range of M. leidyi, found a similar pattern. Their experiments showed size-dependent predation on fish eggs and larvae. Larger ctenophores consumed more eggs. Some eggs were later regurgitated, but many were no longer viable, while fish larvae were retained and digested. These findings are particularly relevant to what we are observing in Kerteminde. The size of an individual is not merely an interesting measurement. It can influence what that individual is capable of capturing and how strongly it affects the surrounding ecosystem. A population consisting of fewer but much larger individuals may still exert substantial pressure on zooplankton, fish eggs and fish larvae.

We need to investigate use, not only control

For several years, I have tried to obtain funding to investigate innovative approaches to this invasive species.

Once M. leidyi is well established, we may not be able to control its regional spread or completely prevent its blooms. But that does not mean that we have no options. We should investigate whether at least part of this recurring biomass can be collected and converted into something useful.

This is not a proposal for a miracle solution. Any utilisation strategy would have to be tested carefully. It must not encourage the further spread of the species, create damaging bycatch or provide an economic incentive to maintain an invasive population. We also need to understand the environmental costs of collection, transport and processing.

But these are exactly the questions that research funding should allow us to answer.

So far, my attempts to secure support for this work have been unsuccessful. Funding agencies do not seem to sense the urgency of studying approaches whose benefits may not be immediate or easily visible. and EPAs do not have any resource to invest in this part. The contrast with events on land is striking. This week, the oak processionary moth, the so-called “larva from hell”, has attracted considerable attention in Odense. Its microscopic hairs can cause rashes and allergic reactions, residents have reported serious discomfort, and a kindergarten has reportedly had to close temporarily. Those concerns are real and deserve a response.

But the case also illustrates how differently we react to environmental threats.

When the impact appears visibly on human skin, the urgency is immediately understood. When ecological damage develops below the surface of the sea, in the form of disappearing zooplankton, altered food webs, consumed fish eggs or reduced larval survival, it is much easier to overlook.

Marine ecosystem changes are often gradual, underwater and largely invisible to the public. By the time their consequences become obvious, the opportunity for early and relatively inexpensive action may already have passed.

Concern does not mean panic

One photograph and a series of observations from one pier do not prove that an ecological crisis is underway. I am not suggesting that they do. But science should not have to wait for undeniable damage before investigation becomes urgent.

The unusually large M. leidyi appearing in Kerteminde this July give us an opportunity to act early. We need systematic monitoring of their abundance and size distribution. We need to measure the available prey field. We need to determine their trophic position and investigate possible consequences for fish recruitment. And we need to explore whether biomass that we may be unable to prevent could be collected and used responsibly.

Whatever language we use and whatever name we give it, the message is the same:

We should measure early, investigate early and support innovative solutions while the warning is still only a warning, not after it has become a crisis.

Relevant publications

Javidpour, J. et al. (2009). “Seasonal changes and population dynamics of the ctenophore Mnemiopsis leidyi after its first year of invasion in the Kiel Fjord, Western Baltic Sea.” Biological Invasions.

Javidpour, J. et al. (2020). “Cannibalism makes invasive comb jelly, Mnemiopsis leidyi, resilient to unfavourable conditions.” Communications Biology.

Stoltenberg, I. et al. (2024). “Predation on Baltic Sea yolk-sac herring larvae (Clupea harengus) by the invasive ctenophore Mnemiopsis leidyi.” Fisheries Research.

Sobrero, L. et al. (2025). “Predatory impact on ichthyoplankton by Mnemiopsis leidyi is size-dependent: an experimental approach.” Marine Ecology Progress Series.

Ribbegople, Rippenqualle or Comb Jelly: Whatever You Call Mnemiopsis leidyi, You Should Be Concerned

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