New global model reveals how biochar can boost climate-smart agriculture
Peer-Reviewed Publication
Updates every hour. Last Updated: 25-Apr-2026 20:16 ET (26-Apr-2026 00:16 GMT/UTC)
As is well known, the Earth behaves like a “giant magnet” (that is, it possesses a dipole magnetic field*1), and this magnetic field is thought to be generated by a dynamo process*2 driven by thermal convection of liquid iron in the Earth’s outer core. Paleomagnetism studies have shown that the Earth’s magnetic field reverses its polarity at irregular intervals, ranging from several hundred thousand to about ten million years. However, the physical mechanism responsible for these reversals remains unresolved. In particular, it is still not well understood how the polarity of the magnetic field - northward or southward - is determined.
Focusing on this polarity-determination mechanism, a research team at the National Institute for Fusion Science (NIFS) and the Graduate University for Advanced Studies, SOKENDAI, carried out a detailed study of a convective dynamo arising in a spherical-shell plasma having the same geometry as the Earth’s outer core, using three-dimensional magnetohydrodynamic simulations*3. As a result, they showed for the first time that, in an Earth-like dynamo, the polarity of the magnetic field (northward or southward) is determined randomly, not by the direction of convection, but by extremely weak magnetic perturbations present initially. Moreover, depending on subtle differences in the imposed magnetic perturbations, the system settles into either a northward - or southward- polarity state and remains there (bi-stability of the dipole polarity). Thus, the polarity of the Earth’s magnetic field may likewise have been determined by tiny fluctuations present when the geodynamo first emerged some four billion years ago. That polarity would then be expected to persist, yet in reality the geomagnetic field undergoes repeated reversals. This suggests that geomagnetic reversals may be caused by physical effects not included in the present computational model.
Beavers are spreading northwards into the Arctic and a new study provides detailed evidence of their expansion by dating the changes they have been making to the tundra landscape. The research, which combines tree ring analysis (looking at beaver browsing scars) with satellite imagery of surface water (highlighting dams), has allowed scientists to track and date beaver movements in remote areas of the Canadian Arctic.
The top ocean predators during the Cretaceous were primarily giant marine reptiles and sharks, or so researchers have thought. Now, a new study suggests colossal “kraken-like” octopuses once hunted Late Cretaceous seas, growing as large as 19 meters in length and competing with – and perhaps even preying upon – large ocean apex predators like mosasaurs. For hundreds of millions of years, marine ecosystems were thought to be dominated by large vertebrate apex predators. Invertebrates served as smaller prey. However, unlike shelled invertebrates, octopuses followed a unique evolutionary trajectory. Instead of protective shells, these creatures evolved soft-bodies, which gave them unprecedented mobility, vision, and intelligence. Some of these species grew to enormous sizes, too, and have functioned as top-tier predators, yet their precise ecological role has remained uncertain due to limited fossil evidence.
To aim to fill this gap, Shin Ikegami and colleagues evaluated the patterns of wear on fossilized jaws of ancient octopus relatives. Wear on the jaw – produced when biting into hard, skeletal prey – leaves characteristic damage similar to the damage seen in modern shell-crushing cephalopods. Measurements of an octopus jaw can also be used to estimate their overall body size. Ikegami et al. reexamined 15 large fossil jaws from ancient octopus relatives and identified clear signs of wear on particularly well-preserved specimens. Using advanced digital fossil-mining techniques, they uncovered 12 additional jaws of finned octopuses from Late Cretaceous sediments (~100 to 72 million years ago). In analyzing them, they identified two main species – Nanaimoteuthis jeletzkyi and N. haggarti. These finned octopuses, N. haggarti in particular, grew to exceptional sizes, say the authors, ranging from ~7 to 19 meters, rivaling the size of contemporaneous giant marine reptiles and potentially representing the largest invertebrates currently described. Moreover, in the largest individuals, the jaws showed extensive wear, with once-sharp features in small juveniles becoming blunted and rounded over time. The wear patterns suggest that these creatures were active carnivores that routinely crushed hard shells and bones with powerful bites, and used their long, flexible arms to seize sizable prey while dismantling it with their strong beaks, a behavior that has been linked to advanced intelligence. According to Ikegami et al., the findings indicate that N. jeletzkyi and N. haggarti were not merely prey but highly active participants in shaping marine ecosystems while occupying roles previously attributed only to large vertebrates.
New high-altitude measurements have revealed a hidden population of extremely small, organic-rich aerosol particles in the lower stratosphere. The findings suggest that these ultrafine aerosols, likely lofted from the underlying troposhpere, are far more abundant and chemically influential than previously understood. The stratospheric aerosol layer, extending from roughly 8 to 35 kilometers above Earth’s surface, plays a crucial role in regulating climate by reflecting sunlight and enabling chemical reactions that influence atmospheric composition. Yet, despite its importance, our understanding of its constituent particles remains incomplete, largely because existing instruments struggle to detect the smallest particles, which fall below their sensitivity thresholds. It’s thought that extremely small particles from the lower atmosphere are transported into the stratosphere through processes such as tropical uplift, atmospheric mixing, intense storm systems, wildfire-driven convection, and even aircraft emissions. However, detailed information about their size distribution, which is critical for determining their volume, surface area, and role in chemical processes, has remained scarce.
Using data collected by a high-altitude research aircraft during the NASA Stratospheric Aerosol Processes, Budget, and Radiative Effects (SABRE) project in 2023, Ming Lyu and colleagues report detailed measurements of stratospheric particles ranging from 0.003 to 2.4 microns, capturing both their distribution and chemical compositions in regions up to 19 kilometers above Earth. In their analysis, Lyu et al. reveal notably high concentrations of extremely small, organic-rich aerosol particles, particularly in atmospheric regions influenced by recently transported air and within the polar vortex. Despite being exceptionally small, these particles dominate the surface area available for heterogeneous atmospheric chemistry and act as a significant condensation sink. Lyu et al. confirmed that many of these fine organic-rich particles originate from the lower atmosphere and subsequently interact with larger sulfur-based aerosols, including those formed from volcanic emissions. This interaction produces a complex, bimodal particle size distribution that current climate models fail to accurately reproduce.