Check out this stunning image of a triangular solar prominence captured by Andrea Vanoni on August 26, 2024. Solar prominences like this one are large, bright features extending outward from the Sun's surface, often forming spectacular shapes as they interact with the solar magnetic field. This particular prominence's unique triangular form makes it an especially fascinating sight.
π· Andrea Vanoni, 26 August 2024
@science #sun #solar
π· Andrea Vanoni, 26 August 2024
@science #sun #solar
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3D Simulation of the Sun: Turbulent Flows in Its Upper Layers
Scientists have created a 3D simulation of the Sun, focusing on the turbulent flows in its upper layers. The movement of solar plasma resembles a boiling cauldron or the chaotic swirls of a school of fish, as material rises to the surface or sinks deeper.
βOur simulations use what we call a realistic approach β this means incorporating everything currently known about solar plasma to replicate various phenomena observed by NASAβs space missions,β explained Irina Kitiashvili, a scientist at NASAβs Ames Research Center, who led the study.
Leveraging advanced computational power, the team managed for the first time to simulate fine structures in the subsurface layer, which are also observed by NASAβs Solar Dynamics Observatory.
βCurrently, we lack sufficient computational capacity to create realistic global models of the entire Sun due to its complexity,β noted Kitiashvili. βInstead, we model smaller regions or layers that reveal structures on the Sunβs surface and atmosphere β such as shock waves or tornado-like phenomena just a few miles across. These are far more detailed structures than any spacecraft can capture.β
Such simulations provide invaluable insights into the dynamics of the Sun, offering a glimpse into processes that fuel solar activity and influence space weather.
#science #space #sun
Scientists have created a 3D simulation of the Sun, focusing on the turbulent flows in its upper layers. The movement of solar plasma resembles a boiling cauldron or the chaotic swirls of a school of fish, as material rises to the surface or sinks deeper.
βOur simulations use what we call a realistic approach β this means incorporating everything currently known about solar plasma to replicate various phenomena observed by NASAβs space missions,β explained Irina Kitiashvili, a scientist at NASAβs Ames Research Center, who led the study.
Leveraging advanced computational power, the team managed for the first time to simulate fine structures in the subsurface layer, which are also observed by NASAβs Solar Dynamics Observatory.
βCurrently, we lack sufficient computational capacity to create realistic global models of the entire Sun due to its complexity,β noted Kitiashvili. βInstead, we model smaller regions or layers that reveal structures on the Sunβs surface and atmosphere β such as shock waves or tornado-like phenomena just a few miles across. These are far more detailed structures than any spacecraft can capture.β
Such simulations provide invaluable insights into the dynamics of the Sun, offering a glimpse into processes that fuel solar activity and influence space weather.
#science #space #sun
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A Giant βCanyonβ on the Sun!
On July 15, the Sun unleashed a spectacular coronal mass ejection, creating a plasma structure that looked like a massive rift stretching 400,000 kilometers β about the same distance from Earth to the Moon! π
An incredible phenomenon in our cosmic neighborhood!
#Sun #Astronomy #Space #Science
On July 15, the Sun unleashed a spectacular coronal mass ejection, creating a plasma structure that looked like a massive rift stretching 400,000 kilometers β about the same distance from Earth to the Moon! π
An incredible phenomenon in our cosmic neighborhood!
#Sun #Astronomy #Space #Science
π₯59π25π23π17β‘11π11
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βοΈ A giant solar prominence has just broken away from the Sun β one of the largest this year, according to Russiaβs Space Research Institute (IKI RAS).
This time, we got lucky. Scientists say that if it had happened a day later, Earth would have been grazed by the edge of the blast β and if two days later, weβd have taken a direct hit.
Fortunately, the plasma cloud is heading safely into deep space, missing all planets.
Still, the spectacle was breathtaking β a fiery arch of superheated plasma tens of thousands of kilometers high, briefly suspended above the solar surface before being hurled away into the void.
#Space #Sun #SolarStorm #Science
This time, we got lucky. Scientists say that if it had happened a day later, Earth would have been grazed by the edge of the blast β and if two days later, weβd have taken a direct hit.
Fortunately, the plasma cloud is heading safely into deep space, missing all planets.
Still, the spectacle was breathtaking β a fiery arch of superheated plasma tens of thousands of kilometers high, briefly suspended above the solar surface before being hurled away into the void.
#Space #Sun #SolarStorm #Science
π58π₯41β‘31π26π26
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βοΈ A massive explosion erupted last night on the far side of the Sun (IKI RAS).
The bright ejection you see in the footage is plasma being hurled away from the Sun β fortunately, in the opposite direction from Earth.
The dark circle and stripe in the frame arenβt mysterious objects β they mark the blind zones of the coronagraphβs optics, used to block direct sunlight and make solar activity visible.
Even though the blast happened on the far side, it shows just how restless our star remains β constantly storing and releasing titanic amounts of magnetic energy.
#Sun #Space #Astronomy #SolarFlare
The bright ejection you see in the footage is plasma being hurled away from the Sun β fortunately, in the opposite direction from Earth.
The dark circle and stripe in the frame arenβt mysterious objects β they mark the blind zones of the coronagraphβs optics, used to block direct sunlight and make solar activity visible.
Even though the blast happened on the far side, it shows just how restless our star remains β constantly storing and releasing titanic amounts of magnetic energy.
#Sun #Space #Astronomy #SolarFlare
π65π₯28β‘20π18π15
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π The Sun Is Waking Up Fast β A Major X-Class Solar Flare Could Happen at Any Moment
Solar activity has accelerated dramatically over the past 48 hours, and space weather scientists are watching closely.
The number of solar flares has surged from 5 per day two days ago, to 8 yesterday, and 17 within the last 24 hours. This morning, the Sun produced its first M-class flares of the current activity spike β leaving only the most powerful category, X-class, yet to appear.
Whatβs making scientists especially cautious is the location of the Sunβs largest active region of 2026. It is currently facing almost directly toward Earth. Surprisingly, despite its enormous size, it has not yet produced a single X-class flare. Earlier this year, another large sunspot group generated five X-class flares, including the yearβs strongest event, X8.1. That makes the current quietness look more like the calm before the storm than a sign of stability.
Space-based observations reveal an even more intriguing picture. Two giant sunspot groups that appear separate on the solar surface are actually connected high above it in the corona, forming a single, highly complex magnetic system. These intertwined magnetic fields continuously exchange energy. On one hand, this can relieve local magnetic stress. On the other, it effectively creates one enormous energy reservoir capable of producing an exceptionally powerful eruption.
Predicting exactly when that energy will be released remains one of the biggest challenges in solar physics. Most of the Sunβs magnetic field lies hidden beneath the visible surface, beyond direct observation, making even the most sophisticated computer models unreliable for systems this complex.
For now, an X-class solar flare could occur at virtually any time. If accompanied by a coronal mass ejection directed toward Earth, it could trigger strong geomagnetic storms, spectacular auroras at unusually low latitudes, and temporary disruptions to satellites, radio communications, and navigation systems.
π The Sun is reminding us that even after centuries of observation, our nearest star can still surprise us.
#Science #Astronomy #Sun #SolarFlare #SpaceWeather #SolarStorm #Heliophysics
Solar activity has accelerated dramatically over the past 48 hours, and space weather scientists are watching closely.
The number of solar flares has surged from 5 per day two days ago, to 8 yesterday, and 17 within the last 24 hours. This morning, the Sun produced its first M-class flares of the current activity spike β leaving only the most powerful category, X-class, yet to appear.
Whatβs making scientists especially cautious is the location of the Sunβs largest active region of 2026. It is currently facing almost directly toward Earth. Surprisingly, despite its enormous size, it has not yet produced a single X-class flare. Earlier this year, another large sunspot group generated five X-class flares, including the yearβs strongest event, X8.1. That makes the current quietness look more like the calm before the storm than a sign of stability.
Space-based observations reveal an even more intriguing picture. Two giant sunspot groups that appear separate on the solar surface are actually connected high above it in the corona, forming a single, highly complex magnetic system. These intertwined magnetic fields continuously exchange energy. On one hand, this can relieve local magnetic stress. On the other, it effectively creates one enormous energy reservoir capable of producing an exceptionally powerful eruption.
Predicting exactly when that energy will be released remains one of the biggest challenges in solar physics. Most of the Sunβs magnetic field lies hidden beneath the visible surface, beyond direct observation, making even the most sophisticated computer models unreliable for systems this complex.
For now, an X-class solar flare could occur at virtually any time. If accompanied by a coronal mass ejection directed toward Earth, it could trigger strong geomagnetic storms, spectacular auroras at unusually low latitudes, and temporary disruptions to satellites, radio communications, and navigation systems.
π The Sun is reminding us that even after centuries of observation, our nearest star can still surprise us.
#Science #Astronomy #Sun #SolarFlare #SpaceWeather #SolarStorm #Heliophysics
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