Machine learning unlocks greener pathway to urea production
Peer-Reviewed Publication
Updates every hour. Last Updated: 28-Apr-2026 16:15 ET (28-Apr-2026 20:15 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.
Endowing and controlling topologically structured emission in microlasers is highly desired yet remains challenging. Toward this goal, researchers at Fudan University developed a compound topological microcavity design for vectorial lasing with designable topological charges. Leveraging quasi-BIC Möbius-like correspondence, they establish a direct, predictive link between cavity morphology and topological charge of emitted lasing profile. Experimentally, they demonstrate vectorial lasing with topological charges from −5 to +5, representing a substantial advance toward compact topological light sources.
A UNSW-led study demonstrates how a new tool can detect blue whale calls with almost 100% accuracy, despite only being trained on one sample song. The tool has the potential to transform how scientists analyse rare and elusive species.
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.