Mysterious Cold Mass in Atlantic Signals Potential Weakening of AMOC

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The “Cold Blob” in Temperature Visualization

Credit: NASA Scientific Visualization Studio/Goddard Space Flight Center

The Earth’s surface has experienced warming over the past 150 years, with the exception of certain areas in the North Atlantic Ocean. This specific region, found southeast of Greenland, has been termed the “warming hole” or “cold mass,” indicating it is up to 1°C cooler than historical averages.

There is ongoing debate among scientists regarding the reason for the existence of this cold blob. Recent studies suggest it may be linked to the weakening of the Atlantic Meridional Circulation (AMOC), a crucial ocean current that distributes warmth from the tropics to Europe.

<p>The AMOC is responsible for transporting warm, salty water from the Gulf of Mexico to the North Atlantic, where it cools, sinks, and then returns south along the ocean floor. Scientists are concerned that an influx of freshwater from melting ice in Greenland could lower the salinity in this area, potentially slowing the sinking process and weakening the overall circulation.</p>
<p>Recent research indicates that the AMOC may <a href="https://iopscience.iop.org/article/10.1088/1748-9326/adfa3b">cross a tipping point</a> in the coming decades, potentially leading to a complete collapse. This collapse could have severe consequences, causing significant cooling in Europe and disrupting critical monsoon rains vital for agriculture in Africa and Asia. However, current direct observations of AMOC strength span only 22 years, which is insufficient to establish clear trends.</p>
<p>Climate <a href="https://www.nature.com/articles/s41586-018-0006-5">modeling</a> suggests that the slowing AMOC reduces the supply of warm water to the North Atlantic, thereby creating this cold mass. Other models, however, attribute a major portion of the phenomenon to atmospheric changes.</p>
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<p>A <a href="https://agupubs.onlinelibrary.wiley.com/doi/full/10.1029/2022GL100420">2022 study</a> by <a href="https://cos.northeastern.edu/people/chengfei-he/">He Chengfei</a> and researchers from Northeastern University, Boston, found that accelerated warming in the Arctic is diminishing the temperature disparity between the polar regions and tropics. This shift is causing the jet stream to move northward into the cold mass area, resulting in stronger westerly winds that increase evaporation, drawing heat away from the ocean.</p>
<p>As evaporation intensifies, cloud cover also increases. Some research indicates that this cloud cover may further contribute to the cooling of the blob.</p>

<p>Research led by <a href="https://www.pik-potsdam.de/members/stefan/homepage">Stefan Rahmstorf</a> at the Potsdam Institute for Climate Impact Research is closely examining the cold mass through climate reanalysis, utilizing direct weather observations from satellites, buoys, and ships, rather than relying on modeling techniques.</p>
<p>Since 1955, they have discovered that heat loss from the ocean’s surface has diminished in the cold mass area. It appears that the ocean is cooling not just at the surface but also at depths of up to 1,000 meters. This indicates that the AMOC is transporting less heat rather than the atmosphere removing more heat.</p>
<p>According to Rahmstorf, “Wind and clouds can only account for a minor portion of the warming hole. While some models suggest atmospheric influences, the data indicates that oceanic factors are the primary causes.”</p>
<p>This finding highlights that the Atlantic circulation has been undergoing changes for decades, intensifying concerns regarding the potential collapse of not only the AMOC but also the surrounding subpolar circulation, which is vital to the process. If this circulation were to shut down, <a href="https://nyaspubs.onlinelibrary.wiley.com/doi/abs/10.1111/nyas.14659">the UK and neighboring regions may experience even more rapid temperature drops</a> than a full AMOC collapse.</p>
<p>Rahmstorf warns, “The subarctic circulation reaching a tipping point could lead to severe climate impacts in Western Europe as early as the 2040s.”</p>

<p>However, direct measurements of ocean surface heat fluxes are currently lacking, making it challenging to accurately estimate them through modeling. A 2021 study, which used data from Rahmstorf's research, found that winds <a href="https://link.springer.com/article/10.1007/s00382-021-06003-4">may account for the majority</a> of the cold blob's formation.</p>
<p>According to He, “Inferring the energy budget of a cold mass using reanalysis poses significant challenges.”</p>
<p>While recent research provides valuable insights, experts like <a href="https://profiles.ucl.ac.uk/38605-david-thornalley">David Thornalley</a> from University College London caution that definitive conclusions about the causes of cold blobs remain elusive.</p>
<p>Limited data prevents us from entirely ruling out alternative explanations. For instance, <a href="https://www.sams.ac.uk/people/researchers/fraser-dr-neil/">Neil Fraser</a> from the Scottish Marine Science Society notes that a tributary of the AMOC, known as the Norwegian Current, may be strengthening and transporting additional heat away from the cold mass regions.</p>
<p>In conclusion, while the existence of the cold mass aligns with AMOC weakening, conclusive evidence remains to be established.</p>
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Source: www.newscientist.com

Signs of Potentially Weakening Dark Energy

Slice of the universe's largest 3D map showing the fundamental structure of matter

A collaboration between Leah Raman and DESI. Custom colormap package with cmastro

The largest 3D map of the universe ever created offers hints about the evolution of the universe and suggests we may be wrong about the behavior of dark energy, which makes up most of the universe. I am. This mysterious power may weaken over time.

“If it can be maintained, this is a very big deal,” he says Adam Rees Johns Hopkins University in Maryland discovered the first evidence of dark energy 25 years ago. That's because the standard model of cosmology, called the lambda CDM, suggests that the intensity of dark energy should not change over time.

Dark energy is thought to cause the accelerated expansion of the universe. If it is not static, it could also have major implications for our ideas about the universe's beginning, its size, and ultimate fate. Mr. Reese, who was not involved in the new work, said the impact was that “we… [our understanding of] “Gravity and Field”.

This strange finding comes from the Dark Energy Spectroscopy Instrument (DESI) in Arizona, where even DESI collaborators say data suggests dark energy may be weakening in recent times. I don't really know what to make of that fact. A DESI spokesperson said: “Whether this is interesting or not, this is all we have been talking about in this collaboration for months.” Kyle Dawson at the University of Utah.

DESI researchers investigated the strength of dark energy by measuring the large-scale structure and distribution of galaxies in the universe, revealing how the universe has expanded over time. The researchers then combined this information with three sets of data about supernovae. Supernovae act as so-called “standard candles” that determine the distance to cosmic objects thanks to their predictable brightness.

Surprisingly, each of the three supernova samples gave a different answer to the changing rate of expansion of the universe over time. All three suggest that the influence of dark energy may have declined in recent years, but the strength of these suggestions varies, so researchers wonder how to interpret the data. I don't really understand.

“Two of the supernova samples don't match each other, but they are very similar,” Dawson said. “We don't know which one is correct. The truth may lie somewhere in between, but the real difference seems to be in the method.” [the supernova researchers] We evaluated the data. ”

Model discrepancy is indicated by a coefficient called sigma. Sigma measures the likelihood that similar collisions will occur by chance when the models do not match each other. “About 3 sigma is the level at which we typically sit and pay attention and call it a 'sign' of something,” Reese says. Values ​​lower than that are usually not of particular interest to researchers. It would be too likely a simple coincidence.

The discrepancies between the lambda CDM and combined supernova and DESI measurements ranged from 2.5 sigma to 3.9 sigma. “Both opinions are true. There's enough tension and it's interesting. And there's not enough tension to say that something is definitely there,” says Dawson.

Dark energy makes up nearly 70 percent of the universe, so errors in our understanding of its properties can have far-reaching implications for physics. However, more precise measurements will be needed in the coming years to prove whether the error really exists.

“if [this is] “Certainly, this is the first real clue we've had about the nature of dark energy in 25 years,” says Rees.

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Source: www.newscientist.com