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Atmosphere

Simplifying Stellarators with QUADCOIL: A New Computer Code for Fusion Power

Physicists have created a new computer code that could speed up the design of the complicated magnets that shape the plasma in stellarators, making the systems simpler and more affordable to build.

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The development of fusion power has long been hindered by the complexity of its underlying physics. However, a team of researchers at the Princeton Plasma Physics Laboratory (PPPL) has made a significant breakthrough by creating a new computer code called QUADCOIL. This innovative tool promises to simplify the design process for stellarators, a type of twisty fusion system that has been notoriously difficult to build.

QUADCOIL is a game-changer in the field because it enables scientists to quickly and efficiently determine the complexity of magnet shapes required to achieve stable plasmas. By doing so, researchers can focus their efforts on designing stellarators with simple magnet shapes, making the construction process more affordable and efficient.

The code works by predicting the properties of plasma shapes that are both physically desirable and feasible to build. This is achieved through a unique combination of two calculation stages: one that determines the plasma shape itself and another that evaluates the corresponding magnet shape. By communicating between these stages, QUADCOIL can identify potential problems early on and suggest alternative designs that meet both physics and engineering requirements.

“QUADCOIL predicts the complexity of magnets quickly, helping you avoid plasma shapes that are great physics-wise but not helpful for actually building a fusion facility,” explained Frank Fu, lead author of the paper outlining the code. “This research pairs PPPL’s expertise in sophisticated plasma computer codes with its extensive history of developing stellarators, a concept that the Lab originated 70 years ago.”

The benefits of QUADCOIL are numerous. Not only does it reduce the computational time required for magnet design from hours to mere seconds, but it also allows scientists to incorporate engineering specifications into their inputs, generating magnet shapes that are more relevant to their needs.

Moreover, QUADCOIL has three key innovations: it calculates more quickly than traditional programs, predicts properties that other codes cannot, and is flexible enough to accommodate a range of engineering specifications. This flexibility enables researchers to add valuable information about magnet materials and topologies, as well as properties such as curvature and magnetic force.

In short, QUADCOIL has the potential to revolutionize the field of fusion power by simplifying the design process for stellarators. As Elizabeth Paul, an assistant professor at Columbia University, noted: “One of the major challenges in designing stellarators is that the magnets can have complex shapes that are hard to build. This problem tells us that we need to be thinking about magnet complexity at the very beginning.”

The researchers behind QUADCOIL are now working on a new version of the code that not only determines the ease of construction for a particular set of magnets but also provides guidance on how to improve the plasma shape. With the support of the DOE’s Scientific Discovery through Advanced Computing program and the Simons Foundation, this innovative tool is poised to make a significant impact in the pursuit of fusion power.

Atmosphere

Uncovering the Hidden Link: NASA Discovers Connection Between Earth’s Core and Life-Sustaining Oxygen

For over half a billion years, Earth’s magnetic field has risen and fallen in sync with oxygen levels in the atmosphere, and scientists are finally uncovering why. A NASA-led study reveals a striking link between deep-Earth processes and life at the surface, suggesting that the planet’s churning molten interior could be subtly shaping the conditions for life. By comparing ancient magnetic records with atmospheric data, researchers found that these two seemingly unrelated phenomena have danced together since the Cambrian explosion, when complex life first bloomed. This tantalizing connection hints at a single, hidden mechanism — perhaps even continental drift — orchestrating both magnetic strength and the air we breathe.

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The study published in Science Advances by NASA scientists has revealed a significant correlation between the strength of the Earth’s magnetic field and fluctuations in atmospheric oxygen levels over the past 540 million years. This groundbreaking research suggests that processes deep within the Earth’s core might be influencing habitability on the planet’s surface.

At the heart of this phenomenon lies the Earth’s magnetic field, which is generated by the flow of molten material in the planet’s interior. Like a giant electromagnet, this process creates a dynamic field that has been fluctuating over time. The authors of the study point out that the role of magnetic fields in preserving the atmosphere is still an area of active research.

To uncover the hidden link between the Earth’s core and life-sustaining oxygen, scientists have analyzed magnetized minerals that record the history of the magnetic field. These minerals, formed when hot materials rise with magma at gaps between tectonic plates, retain a record of the surrounding magnetic field as long as they are not reheated too severely. By studying these ancient rocks and minerals, researchers can deduce historic oxygen levels based on their chemical contents.

The databases compiled by geophysicists and geochemists have provided valuable information on both the Earth’s magnetic field and oxygen levels over comparable ranges. Until now, no scientists had made a detailed comparison of the records. The findings of this study suggest that the two datasets are remarkably similar, with the planetary magnetic field following similar rising and falling patterns as oxygen in the atmosphere for nearly half a billion years.

The implications of this discovery are profound, suggesting that complex life on Earth might be connected to the interior processes of the planet. Coauthor Weijia Kuang said, “Earth is the only known planet that supports complex life. The correlations we’ve found could help us understand how life evolves and how it’s connected to the interior processes of the planet.”

Further research aims to examine longer datasets to see if the correlation extends farther back in time. The study also plans to investigate the historic abundance of other chemicals essential for life, such as nitrogen. As for the specific causes linking the Earth’s deep interior to life on the surface, scientist Kopparapu said, “There’s more work to be done to figure that out.”

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Acid Rain

Uncovering the Hidden Trigger Behind Massive Floods

Atmospheric rivers, while vital for replenishing water on the U.S. West Coast, are also the leading cause of floods though storm size alone doesn t dictate their danger. A groundbreaking study analyzing over 43,000 storms across four decades found that pre-existing soil moisture is a critical factor, with flood peaks multiplying when the ground is already saturated.

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The West Coast of the United States is no stranger to massive floods caused by atmospheric rivers. These powerful storms bring much-needed moisture to the region, but also pose a significant threat to communities and ecosystems. A new study has shed light on the hidden trigger behind these devastating events: wet soils that cannot absorb more water when a storm hits.

The research, published in the Journal of Hydrometeorology, analyzed over 43,000 atmospheric river storms across 122 watersheds on the West Coast between 1980 and 2023. The findings reveal that flood peaks were 2-4.5 times higher on average when soils were already wet. This means that even weaker storms can generate major floods if their precipitation meets a saturated Earth.

Lead author Mariana Webb, completing her Ph.D. at DRI and the University of Nevada, Reno, explained that flooding from any event is not just a function of storm size and magnitude but also depends on what’s happening on the land surface. The study demonstrates the key role that pre-event soil moisture can have in moderating flood events.

Interestingly, flood magnitudes do not increase linearly as soil moisture increases. There’s a critical threshold of soil moisture wetness above which you start to see much larger flows. This research also untangled the environmental conditions of regions where soil moisture has the largest influence on flooding.

In arid places like California and southwestern Oregon, storms that hit when soils are already saturated are more likely to cause floods. In contrast, in lush Washington and the interior Cascades and Sierra Nevada regions, watersheds tend to have deeper soils and snowpack, leading to a higher water storage capacity. Although soil saturation can still play a role in driving flooding in these areas, accounting for soil moisture is less valuable for flood management because soils are consistently wet or insulated by snow.

The study highlights the importance of integrating land surface conditions into impact assessments for atmospheric rivers. Webb worked with DRI ecohydrologist Christine Albano to produce the research, building on Albano’s extensive expertise studying atmospheric rivers, their risks, and their impacts on the landscape.

While soil saturation is widely recognized as a key factor in determining flood risk, Mari’s work helps to quantify the point at which this level of saturation leads to large increases in flood risk across different areas along the West Coast. Advances in weather forecasting allow us to see atmospheric rivers coming toward the coast several days before they arrive. By combining atmospheric river forecast information with knowledge of how close the soil moisture is to critical saturation levels for a given watershed, we can further improve flood early warning systems.

Increased monitoring in watersheds identified as high-risk, including real-time soil moisture observations, could significantly enhance early warning systems and flood management as atmospheric rivers become more frequent and intense. By tailoring flood risk evaluations to a specific watershed’s physical characteristics and climate, the study could improve flood-risk predictions.

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Atmosphere

Biofilms Hold Key to Stopping Microplastic Build-up in Rivers and Oceans

Where do microplastics really go after entering the environment? MIT researchers discovered that sticky biofilms naturally produced by bacteria play a surprising role in preventing microplastics from accumulating in riverbeds. Instead of trapping the particles, these biofilms actually keep them loose and exposed, making them easier for flowing water to carry away. This insight could help target cleanup efforts more effectively and identify hidden pollution hotspots.

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The accumulation of microplastics in our environment is a growing concern. These tiny particles have been found to harm marine life, contaminate food chains, and even enter our own bodies through various pathways. However, predicting where these particles will accumulate and therefore where remediation efforts should focus has been difficult due to the many factors contributing to their dispersal and deposition.

New research from MIT shows that one key factor in determining where microparticles are likely to build up is related to the presence of biofilms. These thin, sticky biopolymer layers are shed by microorganisms and can accumulate on surfaces, including riverbeds or seashores. The study found that when these particles land on sediment infused with biofilms, they are more likely to be resuspended by flowing water and carried away.

The research involved a flow tank with a bottom lined with fine sand, sometimes mixed with biological material simulating natural biofilms. Water mixed with tiny plastic particles was pumped through the tank for three hours, and then the bed surface was photographed under ultraviolet light that caused the plastic particles to fluoresce, allowing a quantitative measurement of their concentration.

The results revealed two different phenomena affecting how much plastic accumulated on the different surfaces. Immediately around the rods simulating above-ground roots, turbulence prevented particle deposition. Additionally, as the amount of simulated biofilms in the sediment bed increased, the accumulation of particles also decreased.

The researchers concluded that the biofilms filled up the spaces between the sand grains, leaving less room for the microparticles to fit in. The particles were more exposed because they penetrated less deeply into the sand grains, making them easier to resuspend and carry away by the flowing water.

This research provides a “nice lens” to offer guidance on where to find microplastic hotspots versus not-so-hot areas. For example, in mangrove ecosystems, microplastics may accumulate preferentially in the outer edges, which tend to be sandy, while the interior zones have sediment with more biofilm. This suggests that the sandy outer regions may be potential hotspots for microplastic accumulation.

The work was supported by Shell International Exploration and Production through the MIT Energy Initiative. While other factors like turbulence or roughness of the bottom surface complicate this, it provides a framework to categorize habitats and prioritize monitoring and protection efforts.

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