Articles tagged with Astrophysical Plasmas
The Blavatnik Awards recognize exceptional early-career achievements in Life Sciences, Chemical Sciences, and Physical Sciences & Engineering. The 2026 Laureates are Maxie M. Roessler, Thi Hoang Duong Nguyen, and Paola Pinilla.
A University of Arizona-led research team has measured the dynamics and ever-changing hot gas shell from where the solar wind originates. The study helps scientists answer fundamental questions about energy and matter moving through the heliosphere, affecting space weather events and planetary orbits.
Astronomers have created a naturally occurring space weather station around complex periodic variable M dwarf stars to study the environment of planets. This discovery sheds new light on how stars affect their planets' makeup and might provide clues about the habitability of distant worlds.
Researchers from Tel Aviv University predict that detecting radio waves from the cosmic dark ages can help resolve the nature of dark matter. The study uses computer simulations to show that dense clumps of dark matter formed throughout the Universe, pulling in hydrogen gas and causing it to emit intense radio waves.
Researchers identified 33 plasma proteins that differ significantly in patients with ALS, suggesting the disease could be detected up to 10 years before symptoms appear. Machine learning models showed strong performance in separating ALS cases from non-ALS cases, with an accuracy of over 98.3%.
Researchers observed a flare caused by a star falling onto a black hole and surviving the encounter. The discovery suggests that these flares may be part of a longer, more complex story about supermassive black holes.
A team of researchers has successfully described warm dense matter, a state of matter combining solid, liquid, and gaseous phases, using a new computational method. This breakthrough advances laser fusion research and helps in the synthesis of new high-tech materials.
Arati Dasgupta, a leading atomic and plasma physicist at NRL, has been elevated to IEEE Fellow for her groundbreaking research in high-energy density plasmas, atomic physics, and radiation materials. Her work has significantly advanced our understanding of extreme environments and their applications.
The EHT Collaboration unveils a new analysis of the supermassive black hole at the heart of galaxy M87, combining observations from 2017 and 2018. The study confirms the presence of a luminous ring with a shifted brightest region, indicating turbulent accretion disk dynamics.
A team led by Sayak Bose has made significant progress in understanding the underlying heating mechanism of coronal holes. They found that reflected plasma waves can cause turbulence and heat coronal holes, providing the first experimental verification of Alfvén wave reflection.
Scientists at the DOE's Princeton Plasma Physics Laboratory have directly observed magneto-Rayleigh Taylor instabilities in plasma, which could aid in understanding how black holes produce vast intergalactic jets. The observation confirms that magnetic fields play a crucial role in forming these jets.
The study found that chaotic movements in magnetic fields heat plasma and make it radiate, explaining the observed X-ray radiation from accretion disks. The simulation also showed that plasma can exist in two distinct equilibrium states, depending on external radiation field.
Scientists at European XFEL have developed a new method to study warm dense matter, allowing for unprecedented insights into its structure and properties. This breakthrough enables the investigation of plasmons in ambient aluminum with ultra-high-resolution X-ray Thomson scattering.
Scientists have developed a machine learning program that can identify blobs of plasma in outer space known as plasmoids. The program will analyze data from NASA's Magnetospheric Multiscale (MMS) mission to better understand magnetic reconnection and its effects on the electrical grid.
Researchers at University of Rochester's Laboratory for Laser Energetics have developed a novel way to experimentally produce plasma 'fireballs' on Earth, generating high-density relativistic electron-positron pair plasmas. This breakthrough enables follow-up experiments that could yield fundamental discoveries about the universe.
A new study suggests that the sun's magnetic field could arise from instabilities in the outermost layers of the sun, rather than deep within. This finding may enable scientists to better forecast solar activity and space weather.
Researchers uncover possible origins of sun's engine, the solar dynamo, which drives sunspots and solar storms. The study reveals that the dynamo may begin in the sun's outermost layers, contradicting decades-old theories.
Researchers used a powerful framework called THEMIS to generate clear images of the Sagittarius A* (Sgr A*) black hole, revealing its plasma ring and magnetic field lines. The study provides strong evidence for the need of strong magnetic fields in the accretion disk to push accreting plasma around.
Researchers discovered a new class of plasma oscillations that can exhibit extraordinary features, enabling innovative advancements in particle acceleration and fusion. This finding has significant implications for achieving clean-burning commercial fusion energy.
The H.E.S.S. Observatory detected gamma-ray emission from the outer jets of SS 433, revealing a shift in energy-dependent morphology. This suggests strong shock acceleration, where high-energy particles collide with photons, producing x-ray radiation and explaining the X-ray reappearance of the jets.
A team of Princeton astrophysicists has conclusively determined that the energy close to the event horizon of black hole M87* is pushing outward, not inward. This finding resolves a longstanding debate within the field and provides new insights into the behavior of black holes.
Researchers discovered a massive structure, Hoʻoleilana, with a diameter of one billion light years, which is larger than predicted by the Big Bang theory. The bubble-like structure encompasses several well-known galaxy clusters and voids, including the Boötes Supercluster.
Scientists have long debated the source of magnetic fields in the universe. New research by Columbia University researchers suggests that turbulent plasma can spontaneously generate these fields, which then amplify and spread across vast distances.
An international team of scientists has detected a quasi-periodic oscillation (QPO) signal in the radio band from a Galactic black hole system, revealing features that have never been seen before. The QPO signal may provide the first evidence of activity from a jet launched by a Galactic stellar-mass black hole.
Researchers at Breakthrough Listen project have devised a new technique for finding and vetting possible radio signals from other civilizations. The technique eliminates the possibility of signal being mere radio interference from Earth, boosting confidence in future detection of alien life.
The Vlasiator model demonstrated that two central theories on plasma eruptions in near-Earth space are simultaneously valid: magnetic reconnection and kinetic instabilities. This finding helps understand how these events occur and improves the predictability of space weather.
A group of scientists from the JIHT, HSE and MIPT have developed a novel solution: OpenDust, a fast, open-source code that performs calculations ten times faster than existing analogues. The algorithm uses multiple GPUs simultaneously to accelerate computations.
Researchers create a hydrogen plasma with known temperature anisotropy, demonstrating the Weibel instability and its potential to seed galactic dynamo magnetic fields. The study uses a novel experimental platform to measure the complex topology of generated magnetic fields.
The Butterfly Nebula's unique shape is caused by a second star orbiting the central star, creating wing-like lobes. New research reveals powerful winds are altering the material within these lobes, contradicting existing models of planetary nebulae formation and evolution.
A research team proposes that magnetic reconnection around black holes energizes plasma, producing copious electron-positron pairs loaded into radio jets. This explanation aligns with M87 observations and predicts short-term X-ray emission when plasma is loaded.
Scientists Luca Comisso and Lorenzo Sironi used supercomputers to simulate the origin of high-energy particles in turbulent environments like the sun's atmosphere. Their research provides a clear pattern of when and how these particles form, paving the way for more accurate predictions of space weather events.
Scientists have simulated a way to create and observe the early stages of fast radio bursts, a mysterious phenomenon that releases enormous energy in space. The proposed experiment uses a strong laser to produce pair plasma, which is then shifted to a higher frequency, demonstrating the prospects for laboratory production and observation.
Researchers propose multiple plasmoids could bridge the vast range of scales in magnetic reconnection, enabling more credible simulations and high-fidelity experiments. The coming experiments will use exascale supercomputers and multiscale laboratory facilities to study reconnection in nature more faithfully.
A new experimental setup provides precise calibration references for soft X-ray transition energies in neon, carbon dioxide, and sulfur hexafluoride gases. This improves the accuracy of astrophysical plasma analysis, enabling scientists to access techniques currently not available.
A team of researchers used the National Ignition Facility (NIF) to create a laboratory replica of galaxy-cluster plasmas, discovering strong suppression of heat conduction in these turbulent environments. The experiments provide insight into complex physics processes and raise additional questions that may be answered in future studies.
Researchers at the DOE's Princeton Plasma Physics Laboratory discovered a process in plasma swirling around black holes that causes previously unexplained emissions of light and heat. The process, known as magnetic reconnection, also jettisons huge plumes of plasma billions of miles in length.
A team of scientists successfully visualized the propagation path of electromagnetic waves from space to ground, revealing a 'straw-shaped' pathway. The study used data from multiple spacecraft and ground-based observatories to clarify the origin and spatial extent of these waves.
Researchers have discovered a new technique to locate the diffusion wake's signal in the quark-gluon plasma, a subatomic soup that flowed like a friction-free fluid after the Big Bang. This breakthrough may help scientists understand how matter emerged from this perfect fluid.
Recent studies suggest that cosmic rays, originating from supernova remnants and pulsars, have a significant impact on galactic dynamics and star formation. The streaming instability triggered by cosmic rays in the interstellar medium can create plasma waves that heat and scatter gas, influencing the formation of planets and stars.
A team of researchers from the Flatiron Institute and Princeton University has found that the magnetic field around a black hole quickly decays when surrounded by plasma. This process, known as 'magnetic reconnection,' rapidly drains the magnetic field and could explain flares seen near supermassive black holes.
Scientists have discovered a novel way to classify magnetized plasmas, which could lead to advances in harvesting fusion energy on Earth. The discovery reveals that a magnetized plasma has 10 unique phases, with transitions between them supporting localized wave excitations.
A new study assesses the dynamics of positron acoustic waves in electron-positron-ion plasmas under magnetic fields, finding compressive and rarefactive solitary waves. The team's results provide insight into magnetoplasma behavior in astrophysical contexts, such as solar winds and auroral acceleration regions.
Researchers at the University of Michigan have discovered a method to stabilize plasma compression using twisted magnetic fields. The technique reduced escaping plasma tentacles by 70% and improved conditions for studying extreme plasma states.
The Plasma Liner Experiment is testing a novel plasma fusion concept while providing insights into the physics of colliding plasma jets. Experiments are also helping to validate simulations crucial for understanding and developing other controlled fusion schemes.
Researchers from the Technion Israel Institute of Technology used exploding electrical wires underwater to generate shock waves, revealing a slower decay rate than predicted by previous models. The findings support a simplified model that accurately describes the relationship between shock wave evolution and wire expansion.
Researchers at the Princeton Plasma Physics Laboratory found that plasma turbulence could amplify magnetic fields to dynamical strengths in a hot, dilute plasma, such as those residing within clusters of galaxies. This discovery provides a possible answer to one of the most important unsolved problems in plasma astrophysics.
Davidovits won the award for his outstanding thesis research on turbulence in compressing fluids and plasma, with a focus on novel mechanisms and applications in inertial-confinement-fusion and astrophysical plasmas. His work has significant implications for plasma physics research.
Researchers in India used numerical computations to investigate the role of chaotic magnetic field lines in generating intense electric current sheets, which are potential sites for extreme heating of the sun's corona. The simulations found a direct proportionality between the intensity of the current sheet and chaoticity.
A new experiment reproduces nature's patterns with a specially designed system called an H-shaped dielectric barrier discharge system. The system produces filaments of discharge plasma that can assume vast ranges of patterns in 3D, allowing scientists to explore complex mechanisms behind nature's diverse designs.
Researchers at Princeton Plasma Physics Laboratory have discovered a new mechanism that speeds up magnetic reconnection, providing new insights into this complex astrophysical process. The model predicts a novel regime in which fast reconnection rates appear independent of system resistivity.
Researchers at the University of Warwick have confirmed a longstanding prediction that high-energy alpha particles will be key to generating fusion power in next-generation tokamaks. They found that LH waves, often used externally, can occur naturally in fusion plasmas and help exploit alpha particle energy.
Researchers observed the onset and stagnation of 3D magnetic reconnection in a lab experiment. The study reveals unexpected features not considered in 2D models, including asymmetric reconnection fields and forces.
Caltech researchers use magnetic forces to create jet-like structures in a hydrogen plasma experiment, shedding light on the formation of astrophysical jets. The study involves running high electrical currents through a cylindrical metal chamber, producing spiral-shaped plumes similar to those observed in space.