Sun releases a powerful solar flare. But don't expect unusual northern lights in US
The sun has emitted a powerful solar flare that has the capability to interfere with technology on Earth.
The explosive burst of radiation peaked on the evening of Tuesday, June 17, matching the intensity of the first of two solar flares detected in May.
This particular flare wasn't accompanied by a geomagnetic storm that can strike Earth's magnetic field and trigger the northern lights. But because the flare occurred on the sun's Earth-facing side, a potential exists for things like radio communications, electric power grids and navigation signals to be disrupted, according to the National Oceanic and Atmospheric Administration.
Reports have already surfaced of a shortwave radio blackout centered over the Pacific Ocean that was especially strong over Hawaii, according to NOAA.
NASA also captured an image of the sun's bright energy burst, which it shared in a blog post.
Considered our solar system's largest explosive events, solar flares occur when magnetic energy associated with sunspots is released into space, creating intense bursts of radiation. These flares are often associated with solar magnetic storms known as coronal mass ejections and can sometimes be as strong as a billion hydrogen bombs.
Solar flares can last mere minutes, or can drag on for hours, depending on their intensity. NASA classifies solar flares based on their strength, with A-class being the smallest and X-class – which is what was recently detected – being the largest.
Each letter represents a ten-fold increase in energy output and includes a scale of 1 to 9 in each class. The exception is the X-class since there are flares that have been recorded exceeding 10 times the power of an X-1.
In May 2024, the largest solar flare since 2017 was detected, ranking at an X-8.7 magnitude. Then in 2025, a May 13 flare was classified as an X-1.2 flare, while another the following day was listed as an X-2.7 flare.
But the most powerful flare measured with modern methods was in 2003. The event was so powerful that it overloaded the sensors measuring it, cutting out at X-28, according to NASA.
Solar flares and other solar activity, such as solar storms, increase every 11 years as the sun reaches the height of its 11-year cycle, the solar maximum, which last occurred in late 2024.
The flare detected recently was also classified as an X-1.2 magnitude, according to NOAA's Space Weather Prediction Center.
NASA's Solar Dynamics Observatory, which observes the sun, was able to capture an image of the event, which the agency said peaked at around 5:49 p.m. ET Tuesday, June 17.
Solar flares emit radiation, mostly in the form of ultraviolet light and X-rays, that can hurtle toward Earth at the speed of light. Some of these flares can be accompanied by coronal mass ejections, or clouds of plasma and charged particles, that emerge from the sun's outermost atmosphere, the corona.
These ejections can collide with Earth's magnetosphere, the barrier protecting humanity from the harshest impacts of space weather, to produce geomagnetic storms that not only pose a hazard to Earthly technologies, but play a role in unleashing northern lights.
But because this powerful flare was not accompanied by a coronal mass ejection, don't expect any unusual aurora activity. The Space Weather Prediction Center tracks the northern lights through an online dashboard.
Weaker solar flares won't be noticeable here on Earth.
But those with enough energy output to rank as an X-class have the potential to disrupt satellites, communications systems, and even ground-based technologies like electric power grids if directed at our planet. In extreme cases, powerful flares even pose risks to spacecraft and astronauts, according to NASA.
About a year ago in May 2024, a historically powerful geomagnetic storm was responsible for some reports of power grid irregularities and interference with GPS signals – even farming equipment. On the bright side, it also unleashed spectacular views of the northern lights in parts of the country where auroras are not often visible.
In this case, a rapid, intense flash of electromagnetic energy ranked as an R3 on NOAA's scale, making it strong enough to disrupt radio signals on the sunlit side of the planet. Ham radio operators around Hawaii may have noticed a loss of signal at frequencies below 25 MHz, according to spaceweather.com.
Eric Lagatta is the Space Connect reporter for the USA TODAY Network. Reach him at elagatta@gannett.com
This article originally appeared on USA TODAY: NASA captures image of powerful solar flare: See photo
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CNN
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A hunt for ghostly particles found strange signals coming from Antarctic ice. Scientists are still trying to explain them
Scientists are trying to solve a decade-long mystery by determining the identity of anomalous signals detected from below ice in Antarctica. The strange radio waves emerged during a search for another unusual phenomenon: high-energy cosmic particles known as neutrinos. Arriving at Earth from the far reaches of the cosmos, neutrinos are often called 'ghostly' because they are extremely volatile, or vaporous, and can go through any kind of matter without changing. Over the past decade, researchers have conducted multiple experiments using vast expanses of water and ice that are designed to search for neutrinos, which could shed light on mysterious cosmic rays, the most highly energetic particles in the universe. One of these projects was NASA's Antarctic Impulsive Transient Antenna, or ANITA, experiment, which flew balloons carrying instruments above Antarctica between 2006 and 2016. It was during this hunt that ANITA picked up anomalous radio waves that didn't seem to be neutrinos. The signals came from below the horizon, suggesting they had passed through thousands of miles of rock before reaching the detector. But the radio waves should have been absorbed by the rock. The ANITA team believed these anomalous signals could not be explained by the current understanding of particle physics. Follow-up observations and analyses with other instruments, including one recently conducted by the Pierre Auger Observatory in Argentina, have not been able to find the same signals. The results of the Pierre Auger Collaboration were published in the journal Physical Review Letters in March. The origin of the anomalous signals remains unclear, said study coauthor Stephanie Wissel, associate professor of physics, astronomy and astrophysics at the Pennsylvania State University. 'Our new study indicates that such (signals) have not been seen by an experiment … like the Pierre Auger Observatory,' Wissel said. 'So, it does not indicate that there is new physics, but rather more information to add to the story.' Larger, more sensitive detectors may be able to solve the mystery, or ultimately prove whether the anomalous signals were a fluke, while continuing the search for enigmatic neutrinos and their sources, scientists say. Detecting neutrinos on Earth allows researchers to trace them back to their sources, which scientists believe are primarily cosmic rays that strike our planet's atmosphere. The most highly energetic particles in the universe, cosmic rays are made up mostly of protons or atomic nuclei, and they are unleashed across the universe because whatever produces them is such a powerful particle accelerator that it dwarfs the capabilities of the Large Hadron Collider. Neutrinos could help astronomers better understand cosmic rays and what launches them across the cosmos. 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When ANITA watches a cosmic ray, the flashlight beam is really a burst of radio waves one-billionth of a second long that can be mapped like a wave to show how it reflects off the ice. Twice in their data from ANITA flights, the experiment's original team spotted signals coming up through the ice at a much sharper angle than ever predicted by any models, making it impossible to trace the signals to their original sources. 'The radio waves that we detected nearly a decade ago were at really steep angles, like 30 degrees below the surface of the ice,' Wissel said. Neutrinos can travel through a lot of matter, but not all the way through the Earth, Vandenbroucke said. 'They are expected to arrive from slightly below the horizon, where there is not much Earth for them to be absorbed,' he wrote in an email. 'The ANITA anomalous events are intriguing because they appear to come from well below the horizon, so the neutrinos would have to travel through much of the Earth. 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'By using computer simulations of what such a shower of particles would look like if it had behaved like the ANITA anomalous events, they are able to generate a kind of template for similar events and then search their data to see if anything like that appears.' Gorham, who was not involved with the new research, designed the ANITA experiment and has conducted other research to understand more about the anomalous signals. While the Auger Observatory was designed to measure downward-going particle showers produced in the atmosphere by ultrahigh-energy cosmic rays, the team redesigned their data analysis to search for upward-going air showers, Vandenbroucke said. Vandenbroucke did not work on the new study, but he peer-reviewed it prior to publication. 'Auger has an enormous collecting area for such events, larger than ANITA,' he said. 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When they decay at high energies, they produce another tau neutrino, as well as a particle called a tau lepton — similar to an electron, but much heavier. But what makes the tau neutrino scenario very unlikely is the steepness of the angle connected to the signal, Wissel said. 'You expect all these tau neutrinos to be very, very close to the horizon, like maybe one to five degrees below the horizon,' Wissel said. 'These are 30 degrees below the horizon. There's just too much material. They really would actually lose quite a bit of energy and not be detectable.' At the end of the day, Gorham and the other scientists have no idea what the origin of the anomalous ANITA events are. So far, no interpretations match up with the signals, which is what keeps drawing scientists back to try to solve the mystery. The answer may be in sight, however. 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'The most likely scenario is that it's some mundane physics that can be explained, but we're sort of knocking on all the doors to try to figure out what those are.'


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A hunt for ghostly particles found strange signals coming from Antarctic ice. Scientists are still trying to explain them
Scientists are trying to solve a decade-long mystery by determining the identity of anomalous signals detected from below ice in Antarctica. The strange radio waves emerged during a search for another unusual phenomenon: high-energy cosmic particles known as neutrinos. Arriving at Earth from the far reaches of the cosmos, neutrinos are often called 'ghostly' because they are extremely volatile, or vaporous, and can go through any kind of matter without changing. Over the past decade, researchers have conducted multiple experiments using vast expanses of water and ice that are designed to search for neutrinos, which could shed light on mysterious cosmic rays, the most highly energetic particles in the universe. One of these projects was NASA's Antarctic Impulsive Transient Antenna, or ANITA, experiment, which flew balloons carrying instruments above Antarctica between 2006 and 2016. It was during this hunt that ANITA picked up anomalous radio waves that didn't seem to be neutrinos. 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'So, it does not indicate that there is new physics, but rather more information to add to the story.' Larger, more sensitive detectors may be able to solve the mystery, or ultimately prove whether the anomalous signals were a fluke, while continuing the search for enigmatic neutrinos and their sources, scientists say. Detecting neutrinos on Earth allows researchers to trace them back to their sources, which scientists believe are primarily cosmic rays that strike our planet's atmosphere. The most highly energetic particles in the universe, cosmic rays are made up mostly of protons or atomic nuclei, and they are unleashed across the universe because whatever produces them is such a powerful particle accelerator that it dwarfs the capabilities of the Large Hadron Collider. Neutrinos could help astronomers better understand cosmic rays and what launches them across the cosmos. 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When ANITA watches a cosmic ray, the flashlight beam is really a burst of radio waves one-billionth of a second long that can be mapped like a wave to show how it reflects off the ice. Twice in their data from ANITA flights, the experiment's original team spotted signals coming up through the ice at a much sharper angle than ever predicted by any models, making it impossible to trace the signals to their original sources. 'The radio waves that we detected nearly a decade ago were at really steep angles, like 30 degrees below the surface of the ice,' Wissel said. Neutrinos can travel through a lot of matter, but not all the way through the Earth, Vandenbroucke said. 'They are expected to arrive from slightly below the horizon, where there is not much Earth for them to be absorbed,' he wrote in an email. 'The ANITA anomalous events are intriguing because they appear to come from well below the horizon, so the neutrinos would have to travel through much of the Earth. 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'By using computer simulations of what such a shower of particles would look like if it had behaved like the ANITA anomalous events, they are able to generate a kind of template for similar events and then search their data to see if anything like that appears.' Gorham, who was not involved with the new research, designed the ANITA experiment and has conducted other research to understand more about the anomalous signals. While the Auger Observatory was designed to measure downward-going particle showers produced in the atmosphere by ultrahigh-energy cosmic rays, the team redesigned their data analysis to search for upward-going air showers, Vandenbroucke said. Vandenbroucke did not work on the new study, but he peer-reviewed it prior to publication. 'Auger has an enormous collecting area for such events, larger than ANITA,' he said. 'If the ANITA anomalous events are produced by any particle traveling through the Earth and then producing upward-going showers, then Auger should have detected many of them, and it did not.' A separate follow-up study using the IceCube Experiment, which has sensors embedded deep in the Antarctic ice, also searched for the anomalous signals. 'Because IceCube is very sensitive, if the ANITA anomalous events were neutrinos then we would have detected them,' wrote Vandenbroucke, who served as colead of the IceCube Neutrino Sources working group between 2019 and 2022. 'It's an interesting problem because we still don't actually have an explanation for what those anomalies are, but what we do know is that they're most likely not representing neutrinos,' Wissel said. Oddly enough, a different kind of neutrino, called a tau neutrino, is one hypothesis that some scientists have put forth as the cause of the anomalous signals. Tau neutrinos can regenerate. When they decay at high energies, they produce another tau neutrino, as well as a particle called a tau lepton — similar to an electron, but much heavier. But what makes the tau neutrino scenario very unlikely is the steepness of the angle connected to the signal, Wissel said. 'You expect all these tau neutrinos to be very, very close to the horizon, like maybe one to five degrees below the horizon,' Wissel said. 'These are 30 degrees below the horizon. There's just too much material. They really would actually lose quite a bit of energy and not be detectable.' At the end of the day, Gorham and the other scientists have no idea what the origin of the anomalous ANITA events are. So far, no interpretations match up with the signals, which is what keeps drawing scientists back to try to solve the mystery. The answer may be in sight, however. Wissel is also working on a new detector, the Payload for Ultra-High Energy Observations or PUEO, that will fly over Antarctica for a month beginning in December. Larger and 10 times more sensitive than ANITA, PUEO could reveal more information on what is causing the anomalous signals detected by ANITA, Wissel said. 'Right now, it's one of these long-standing mysteries,' Wissel said. 'I'm excited that when we fly PUEO, we'll have better sensitivity. In principle, we should be able to better understand these anomalies which will go a long way to understanding our backgrounds and ultimately detecting neutrinos in the future.' Gorham said that PUEO, an acronym that references the Hawaiian owl, should have the sensitivity to capture many anomalous signals and help scientists find an answer. 'Sometimes you just have to go back to the drawing board and really figure out what these things are,' Wissel said. 'The most likely scenario is that it's some mundane physics that can be explained, but we're sort of knocking on all the doors to try to figure out what those are.'
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