3 powerful solar flares erupt in less than 24 hours, ending weeks of calm on the sun (video)

After more than three weeks without a powerful solar flare, the sun has suddenly ramped up its activity, firing off three M-class solar flares in less than 24 hours.

While the sun has been popping off plenty of smaller C-class flares lately, Sunday’s M2.9 eruption at 10:01 a.m. EDT (1401 GMT) on Aug. 3 was the first M-class flare since July 12, according to space weather website SolarHam.com’s post on X. The flare marked the end of a 22-day lull in moderate solar flare activity.

Two more followed in rapid succession: an M2 flare at 1:05 a.m. EDT (0505) on Aug. 4 and an M1.4 peaked just 16 minutes later at 1:21 a.m. EDT (0521 GMT). All three eruptions came from sunspot region AR 4168, which rapidly developed a more complex magnetic structure over the weekend.

Space weather forecasters are watching for faint CMEs that could reach Earth later this week. (Image credit: Sun image captured by Daisy Dobrijevic using the Vaonis Vespera Pro. Inset image credit: NASA / SDO and the AIA, EVE, and HMI science teams, helioviewer.org)

Solar flares are powerful bursts of radiation from the sun’s atmosphere, caused by sudden releases of magnetic energy near sunspots. They’re classified by strength into five categories: A, B, C, M, and X. Each level represents a tenfold increase in energy output. While C-class flares are generally minor, M-class flares are moderate and can sometimes disrupt radio communications. The most intense, X-class flares, have the potential to trigger widespread radio blackouts and even impact satellites and power grids on Earth.

A view of the sun captured on Aug. 3, from the U.K using Vaonis Vespera Pro. (Image credit: Daisy Dobrijevic)

According to Spaceweather.com, both active regions 4168 and 4167 now harbor unstable “delta-class” magnetic fields, an arrangement known to power strong solar eruptions, including potential X-class flares and Earth-directed coronal mass ejections (CMEs).




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