Articles tagged with Magnetosphere
A study published in Science Advances reveals that Earth's ionosphere contributed to the majority of ring current ions during a record-breaking super geomagnetic storm in May 2024. This finding highlights the importance of understanding how much Earth's ionosphere contributes to the ring current, as it may be essential for accurately p...
New study by University of Southampton confirms the universe's expansion is still accelerating as previously found, debunking 2025 claims that the cosmos was slowing. The team re-evaluated data using Type Ia supernovae to calculate vast cosmic distances and found no error in their methods.
Researchers measured wind speeds on seven hot, Jupiter-like exoplanets and found that magnetic fields govern the winds. The team's findings provide the strongest evidence yet of magnetism on planets outside our Solar System.
A new study suggests Saturn's magnetic field is asymmetrical, with cusps located most often between 13:00 and 15:00. The researchers believe rapid spin and heavy plasma from Enceladus drag the field lines to the right.
A recent study revealed that the solar superstorm caused a dramatic increase in electrons in two distinct layers of Mars' atmosphere at altitudes of around 110 and 130 km. The storm also triggered computer errors for both orbiters, but they recovered quickly due to their radiation-resistant components.
West Virginia University scientists create digital twin models using AI technology to monitor astronaut movements and muscle activity, predicting potential health risks. The system can detect subtle early signs of trouble, providing personalized exercise routines and helping astronauts cope with balance issues upon return to Earth.
A new study reveals how the superstorm compressed Earth's plasmasphere, a protective layer of charged particles that encircles our planet. The plasmasphere normally extends far from Earth, but during the storm, its outer boundary moved from approximately 44,000 km above Earth's surface to just 9,600 km.
Researchers successfully estimated precise altitude distribution of nitrogen molecular ions responsible for blue aurora emissions at high altitudes. The study revealed a peak emission intensity at 200 km altitude, suggesting higher-than-thought density of nitrogen molecular ions in the atmosphere.
Researchers used large-scale simulations to reproduce near-Earth space environment, confirming opposite charge polarities between regions. Plasma motion explains the reversal in equatorial plane.
A team of geophysicists from ETH Zurich and SUSTech, China, used computer models to simulate whether a completely liquid core could generate a stable magnetic field. Their simulations showed that the Earth's magnetic field was generated in the early history of the Earth in a similar way to today.
Researchers propose using soft X-rays to measure reconnection rates and monitor space weather. By analyzing bright X-ray features, they calculated a global reconnection rate of 0.13, closely matching theoretical predictions.
Scientists have discovered a strong correlation between the Earth's magnetic field and atmospheric oxygen levels over the past 540 million years. The study, published in Science Advances, suggests that fluctuations in the magnetic field may be influencing the planet's habitability.
Researchers found that ancient Homo sapiens used tailored clothing and ochre-based sunscreens to protect themselves from harmful UV light during the Laschamps excursion. This period of reduced magnetic field strength allowed more cosmic radiation to reach Earth's surface, potentially contributing to the decline of Neanderthals.
Scientists use FAST to analyze FRB 20201124A and discover 90% circular polarization, a record high. The findings contradict theoretical models, suggesting pulsar-like mechanisms may be more plausible.
The EZIE mission will use a new measurement technique to study the electrojets, which can create large magnetic disturbances and power outages. By mapping the electrojets' structure and evolution, scientists hope to improve predictions of hazardous space weather.
The Lunar Environment Heliospheric X-ray Imager (LEXI) instrument will provide comprehensive views of Earth's magnetosphere, capturing low-energy X-rays emanating from its edges. This could help researchers understand how the planet responds to space weather and potentially damaging solar particles.
Astronomers at MIT used a novel technique to determine the precise location of a fast radio burst, finding it likely originated from the magnetosphere around a rotating neutron star. The study provides conclusive evidence that fast radio bursts can emerge from this highly magnetic environment.
A team of scientists analyzed smartphone videos and amateur photos of a rare blue-dominant aurora in Japan to estimate its area and confirm findings with spectrophotometers. The research revealed longitudinal structures aligned with magnetic field lines, spanning about 1200 km in longitude.
Researchers at the University of Colorado Boulder have discovered a link between lightning storms on Earth and high-energy electrons in space. The team found that lightning strikes can knock these 'killer electrons' out of the inner radiation belt, which could pose a threat to satellites and astronauts.
Two lunar magnetic anomalies, Mare Tranquillitatis and Reiner Gamma, attributed to magnetized magma intrusions. The depth to the bottom of magnetic carriers varies at approximately 50 km under Mare Tranquillitatis and 30 km under Reiner Gamma.
The Soft X-ray Imager (SXI) is a wide-field X-ray telescope that will image Earth's magnetospheric boundaries, revealing invisible structures and processes. It is part of the Solar wind Magnetosphere Ionosphere Link Explorer (SMILE) mission, which aims to study the solar winds' impact on our planet's magnetic environment.
Researchers have obtained a detailed spatial distribution of color and a hyperspectral image of the aurora borealis for the first time, revealing new insights into energy transport and electron interactions. The observations will contribute to advancing auroral research and understanding the mechanism of auroral emission.
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.
Research team finds chorus waves suppress ECH waves, leading to dominant role in diffuse auroral precipitation. Chorus waves' effect confirmed through simulations and Japan's Arase satellite data.
New discoveries about Jupiter's magnetosphere shed light on its interaction with the solar wind and Earth's magnetic field. The research, published in AGU Advances, shows that Jupiter has a largely closed magnetic field at its poles but open field lines, which could influence Earth's space weather forecasting.
A new study has challenged existing theories on the behavior of particles in the Van Allen belt, a hazardous region near Earth. The research has implications for predicting and analyzing particle movement, which is crucial for understanding space environments.
Researchers successfully conduct laboratory studies on whistler mode chorus emission using the RT-1 device, a magnetically levitated superconducting coil. The findings reveal that high-temperature electrons drive the generation of chorus emission, while increasing plasma density suppresses its occurrence.
Researchers propose that parallel electric fields in the upper atmosphere could produce the colorful emissions of Steve and the picket fence. This unusual process has implications for understanding energy flow between Earth's magnetosphere and ionosphere.
A study reveals that Earth's ionospheric plasma drives geomagnetic storms, disrupting radio signals and GPS. The research helps predict storm impact and contributes to understanding space weather.
Researchers used seismic data to locate and identify a thin layer of molten silicates overlying Mars' metallic core. The discovery reveals a denser and smaller Martian core, aligning with other geophysical data and analysis of Martian meteorites. This finding provides new insights into how Mars formed, evolved, and became a barren planet.
High-energy electrons from Earth's plasma sheet contribute to weathering processes on the Moon's surface, aiding in the formation of water. The discovery may help explain the origin of lunar water ice and provide insights into the Moon's evolution.
Researchers detected distinct 'dwarf pulses' from PSR B2111+46 using the Five-hundred-meter Aperture Spherical radio Telescope. These narrow, weak pulses exhibit a rare reversed spectrum and are produced by one or a few particles generated by pair production in a fragile gap of the pulsar's magnetosphere.
The BepiColombo mission has successfully observed how electrons raining down on Mercury's surface can trigger high-energy auroras. The observations confirm that the mechanism generating aurorae is the same throughout the Solar System.
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.
Researchers used NASA InSight data to directly measure Mars' core properties, finding a completely liquid iron-alloy core with high percentages of sulfur and oxygen. This discovery provides new insights into Martian formation and geological differences between Earth and Mars, potentially impacting planetary habitability.
A team of researchers has successfully modeled the complex fluctuations in soft X-ray signals detected by satellites using numerical methods. They were able to capture how the signal varied with the orbital motion of the satellite and reproduce it up to a factor of two, an impressive feat in the field.
Scientists from Southwest Research Institute (SwRI) used data from NASA's Juno spacecraft to observe magnetic reconnection between Ganymede and Jupiter. The study found accelerated electrons traveling along the magnetic field at Ganymede's magnetopause, indicating the presence of reconnection.
A team of scientists from Tokyo Metropolitan University created unprecedentedly lightweight optics for X-ray space telescopes by employing Micro Electro-Mechanical System (MEMS) technology. By refining the patterning and annealing process, they achieved ultra-sharp features that rival existing telescopes in performance while significan...
Researchers develop experimental platform to study mini-magnetospheres, observing effects of magnetic field on magnetopause and bow shocks. The platform combines Large Plasma Device with lasers and magnetic dipoles, allowing for controlled variation of parameters.
Researchers discovered Mercury has geomagnetic storms triggered by a ring current, similar to those on Earth. The findings were made possible by the Messenger space probe's data and a solar coronal mass ejection.
A new simulation suggests that energy released near a black hole's event horizon during magnetic field line reconnection powers the intense flares. The process involves interactions between the magnetic field and material falling into the black hole, releasing hot plasma particles that radiate away as photons.
Researchers discovered a complex relationship between Jupiter's magnetic field, volcanic activity on its moon Io, and the planet's powerful aurorae. The study revealed an electromagnetic 'tug-of-war' lights up aurorae in Jupiter's upper atmosphere.
The Parker Solar Probe has entered the solar corona and spent five hours in direct contact with the sun's plasma, measuring phenomena previously estimated. The probe discovered that the Alfvén critical surface is wrinkled, suggesting a potential new era for understanding coronal heating.
Researchers are using a multi-disciplinary approach to study the habitability of exoplanets, with Mars serving as a key example. The team is analyzing the atmospheres of different planets and how they might retain them under various conditions.
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 use NASA's MMS data to study micro-scale physics in the Earth's magnetotail, revealing a key component missing from existing models: an ambipolar electric field. This discovery challenges existing understanding of thin current sheets and provides new insights into space weather
The LSXI will use a lunar platform to continuously observe the global images of the Earth's magnetosphere, providing unprecedented observational coverage and innovations in magnetospheric physics research. The instrument combines space-based and ground-based detection results to predict and mitigate space weather disasters.
Researchers at the University of Rochester found that lunar samples do not show signs of magnetization from a magnetic shield. The lack of magnetization suggests that the moon has never had a prolonged dynamo field. Without this protection, solar wind implanted volatiles like helium 3 in the lunar soil.
A Korean research team has identified the origin of bifurcated current sheets in the Earth's magnetosphere through theoretical analysis and simulations. The study reveals that these sheets naturally bifurcate during equilibration, resolving a long-standing mystery.
Researchers at George Mason University are developing Python tools to facilitate the exploration of heliophysics data in 3D. The project aims to create a suite of functions that can read in measurements and simulation output, produce 3D renderings, and perform basic data reduction and manipulation.
Scientists discovered that electrons in Van Allen Radiation Belts are accelerated to extreme high speeds locally, reaching ultra-relativistic energies. This process is extremely efficient and may help understand acceleration processes in the universe.
Scientists have discovered that auroral beads are caused by turbulence in the plasma surrounding Earth, which precedes substorms and triggers auroras. The new models provide a broader picture of the near-space environment, helping researchers better understand swirling structures seen in auroras.
Scientists at Rice University have developed new methods to characterize the influence of turbulence on space weather. They discovered that bursty bulk flows cause big ripples in plasma, leading to oscillations called buoyancy waves. These waves play a role in the formation of auroral structures and magnetospheric substorms.
Researchers studied EMIC waves to reveal plasma characteristics and temperature/density within the magnetosphere. This knowledge could provide insights into space weather effects on our planet and aid fusion energy development.
Researchers measured Jupiter's electric current system and found that alternating currents play a crucial role in generating the aurora. The study used data from NASA's Juno spacecraft to derive electric currents and found a total of approximately 50 million amperes, significantly lower than expected values.
Researchers found that when a plasma jet strikes the magnetopause, it creates drum-like vibrations on its surface, producing standing waves that echo back and forth. These waves can penetrate deep into the magnetosphere, triggering other types of waves and affecting radiation belts, auroras, and ionospheres.
Researchers successfully captured chorus wave packets and transient auroral flashes simultaneously, revealing details of wave-particle interaction regions. The observation confirms geomagnetic north-south asymmetry and suggests rapid precipitation of energetic electrons into the atmosphere.
Researchers have found that the regions in the Earth's magnetosphere that energize the polar aurora are remarkably calm and nonturbulent. The study revealed intense electron jets associated with magnetic reconnection, which dump energy into Earth's atmosphere, exciting auroras.
Researchers have found an extremely hot magnetosphere around a white dwarf, a remnant of a star like our Sun. This discovery sheds light on the origin of highly ionised metals in some white dwarfs, which were previously a puzzle. The study reveals that the magnetic field traps material flowing from the surface, heating it up dramatically.
Researchers at Kanazawa University used satellite data to study the Earth's inner magnetosphere, gaining a better understanding of charged particles and electric fields. This knowledge can help protect satellites from damage caused by particle bursts, enabling more accurate space weather forecasts.