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How Antennas on Earth Hear Solar Flares ⚡ экспресс

Original: "Real-time detection of solar flares from ground-based VLF data"
arXiv:2605.11822 · 2026-05-12 · CC BY 4.0 · ⏱ 1 min · Instrumentation Stellar
Ordinary antennas capture the echo of solar flares in the ionosphere's radio mirror and warn of danger faster than satellites.
Abstract

Scientists have found a way to spot solar flares using radio waves that reflect off the ionosphere like an echo. It’s similar to how ripples on water reveal a thrown stone. The new method works faster than satellites and isn’t fazed by their breakdowns. The real question is: might we soon predict flares as effortlessly as checking the weather forecast?

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The ionosphere at an altitude of 70 kilometers acts like a giant mirror for radio waves. Ground antennas constantly beam signals into it and listen for the reflection. When a solar flare occurs on the Sun, a stream of X-rays reaches Earth in 8 minutes and compresses the lower layer of the ionosphere. It's like tilting a mirror slightly—the reflected beam shifts in phase (the arrival time of the wave). Sensitive receivers notice this shift and instantly alert to powerful M-class and X-class flares, which are dangerous for satellites and power grids.

At night, the D-region of the ionosphere disappears, and the mirror vanishes. But during the day, the system works perfectly.

The system combines data from multiple transmitters, as if we were looking at the mirror from different angles, and using spectrometric assessment determines the strength of the burst. Ground antennas are cheap and independent of satellites, which can delay data. In the future, this will become part of a global defense against space weather.

The X-rays from a flare travel 8 minutes, just like light from the Sun. It might seem that satellites in orbit should see it instantly, but they need time to process. The ground method reacts to the reflection distortion even before the satellite sends data—and often warns faster.

🎯 The very low frequency waves used in this method can travel through water—which is why they are used to communicate with submarines at depth.

🎬 Now we're not just reading about space weather in sci-fi—we're listening to solar storms through the ionosphere's radio mirror.

Scientists
Christian DopplerD. B. McLaughlinDidier QuelozMichel MayorR. A. RossiterAlbert Einstein
Tags
Sun spectroscopy speed of light
Laws
Doppler effectprinciple of constancy of the speed of lightmass–energy equivalenceMaxwell's equationsPlanck's lawLorentz transformations
Original: arXiv:2605.11822 · CC BY 4.0 · bridge42worlds