With this blog post, we would like to introduce and launch our new cooperation with FYORD! FYORD is a joint network by CAU and GEOMAR initiated to connect and support Early Career Researchers of the marine sciences from Master’s to PostDoc level. After occasional exchanges in the past (see our blog here), we are very happy to establish a closer, long-term cooperation with FYORD.
One example of the support provided by FYORD is the Travel Grant. Any FYORD member can apply for funding to travel to conferences, workshops, and summer schools, or visit project partners or institutes. After returning from a funded trip, the FYORD members provide a short report about the event they participated in, to inspire and motivate others and share their experiences. As part of the newly established cooperation, OceanVoices will publish these reports on behalf of FYORD. Below you can find the first two reports, where Helene, Sayoni, and Xiaoqi share their experiences at the largest European geoscientific conference. Enjoy!
My experience of participating in the EGU assembly for the first time
I am Xiaoqi Xu, an exchange PhD student in GEOMAR, from the Institute of Atmospheric Physics, Chinese Academy of Sciences. My major is meteorology, and my research is about the atmosphere-ocean-sea ice interaction over the Southern Ocean as well as the development of an ocean-sea ice coupled model.
Since starting my PhD studies, I have believed that academic communication is a crucial part of scientific research. With the scholarship supported by the University of Chinese Academy of Sciences, I had an opportunity to go to GEOMAR for a one-year exchange program. Under the guidance of Torge Martin, a scientist in the Ocean Dynamics group in GEOMAR, I am studying the mechanism of the atmospheric response to freshwater input around Antarctica based on FOCI (the fully coupled climate model developed by GEOMAR).
I am delighted to have received funding from FYORD and was pleasantly surprised that guest students like me are eligible for the same benefits. I applied for funding to participate in the General Assembly of the European Geosciences Union (EGU). EGU General Assembly is a fantastic event in the geoscience community, held annually in Vienna. This year, the conference featured 18,896 presentations, with early-career scientists accounting for 57%, making it an excellent platform for young researchers. Six months before the conference, I decided to organize my research with Torge and present it at this international event to promote our work. Since we didn’t have project funding related to this topic at the time, I learned about FYORD and applied for funding with the help and advice of colleagues, receiving a positive response quickly, which was a pleasant surprise.
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Xiaoqi Xu giving her talk -

A crowded meeting room -

The exhibition hall
A month before the conference, I spent a lot of time and effort perfecting my presentation. The EGU venue is vast, with a lot of sessions and a tight schedule, so to attend the talks of interest, it’s essential to plan and bookmark them in advance. I gave an 8-minute oral presentation (plus 2 minutes for discussion), requiring careful management of my content due to the time constraints. Oral presentations provide an opportunity to systematically convey my research and enhance my presentation skills. For researchers, it’s crucial not only to conduct research but also to articulate it logically.
In addition to oral presentations, the poster sessions were a pleasant surprise for me because they allowed for more extended discussions (1-2 hours) with other scientists in similar fields. If given the chance, I would consider presenting a poster in the future.
During the conference, my days were filled with attending talks and visiting the poster sessions, where I could chat over coffee. This intense exchange of ideas, both giving and receiving, is a highlight. Although we cannot remember every detail of each talk, the main goal of such conferences is to know about what scientists worldwide are working on and what improvements are needed. Additionally, it’s a large social platform where you can meet your old friends, make new ones, and learn about various institutions, which can help in future career decisions.
The overall experience of the conference was very positive, and the venue was modern and well-organized. I highly recommend attending EGU. Of course, one small gripe is that lunchtime can be extremely crowded, with lines for food stalls exceeding 40 minutes, so bringing your own lunch might be a good idea to avoid missing out on sessions.
Xiaoqi Xu
Sayoni’s experience at EGU 2024
Hello, I am Sayoni Bhattacharya and I am currently working as a Ph.D. student in GEOMAR, Kiel. My topic of research is to develop an autonomous sensor for measuring Dissolved Inorganic Carbon (DIC) in seawater.
I applied for a travel grant from FYORD to attend the EGU 2024 conference. The conference was held in Vienna, Austria from 14-19th April 2024. EGU is considered one of the biggest conferences in Europe in the field of Earth Science. According to this year’s survey, almost 20,000 people attended from all over the world. EGU is a successful concoction of ocean, land, and space science, where curious scientists can develop a network with peers from similar expertise, or they can expose themselves to other genres of science to get a new flavour. There were parallel sessions of talks and posters for consecutive days. With the help of the EGU24 app, a curious person can navigate through all the sessions and choose to attend specific sessions. Moreover, several companies, and publishing houses e.g., Pyroscience, ThermoScientific, and Elsevier showcased their products in company booths. I was particularly interested in sensors which were commercially available to measure gases or liquids using different working principles.
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Sayoni at EGU 2024 -

Discussion research during the poster session
In EGU 2024, I applied for a short talk but in the end, my abstract was selected for a poster presentation and I presented my Ph.D.-related work. I communicated with many scientists, from early career scientists like myself to well-known professors. In each interaction, I felt that I explored a new way of thinking about my own work and I can translate that idea to my next discussion. I felt that the poster sessions were more active and dynamic than talks.
My overall feeling about EGU 2024 is bittersweet. I like the idea of connecting scientists of different backgrounds from any corner of the world and making it a successful event without any visible problems. On the other hand, it felt robotic, as from getting the ID badge to hovering around a session is all done without any human interaction. Finally, from my very personal feeling, I would like to say that the cost to attend EGU is very expensive and no food was served (except for drinks at a few specific times).
Sayoni Bhattacharya
A short report on visiting Europe’s largest geoscience conference
My name is Helene-Sophie Hilbert and I am a doctoral researcher at GEOMAR Helmholtz Centre for Ocean Research Kiel. My research belongs to the field of marine geophysics, a discipline which studies the physical processes and the physical properties of the Earth within the marine environment. My main work focuses on the back-arc basin and active volcanic island arc in the Mariana Subduction zone in the north-western Pacific. I am fascinated by these geologic settings because they are regarded as highly dynamic regions encompassing oceanic and continental domains. While island arcs are considered prime locations for the growth of continental crust, back-arc basins play a major role in the opening and closure of ocean gateways. To gain information about the structures in the crust and upper mantle in the Marianas, I use ocean bottom seismometers that record seismic signals on the seafloor and analyse these signals by generating a seismic tomography (a bit more abstract version of computer tomography, you may know from your doctor).
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Some FYORD travel grand recipients -

Helene presenting her Poster
From 14-19 April 2024, I now had the opportunity to present my research about the youngest back-arc basin, the Mariana Trough, at the European Geoscience Union (EGU) General Assembly in Vienna. The EGU General Assembly is Europe’s largest and most prominent geoscience event with more than 20,000 participants this year from all over the world. I presented my research results in the form of a scientific poster in a session focusing on the geological processes inside subduction zones during their initiation and later evolution. This presentation format gave me the chance to have in-depth discussions with other experts on the individual aspects of my interpretation. Due to the nearly 19,000 presentations during the EGU General Assembly, it was possible to get a wide overview of the current hot topics in the geoscience community and to meet scientists from all kinds of disciplines and institutes. Although the programme was very tightly scheduled, there was still plenty of time for networking. For me personally, it was quite extraordinary and sometimes overwhelming due to the sheer flood of information. But I would still recommend to every geoscientist to have this experience and benefit from the direct exchange with the community. I am therefore grateful that I was given this opportunity thanks to the support in the form of the FYORD Travel Grant.
Helene
FYORD Travel Grant Reports: Impressions from the largest European geoscientific conference
Ocean Acidification
New Friends, New Addresses
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
Ocean Acidification
Color Traditions with Munsell Soil-Color Charts

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