The Sun follows an approximately 11-year cycle, during which its magnetic field completely reverses polarity. Sunspots — dark, magnetically active regions on the solar surface — rise and fall in number, producing solar flares and coronal mass ejections that can disrupt satellites, communications, and power grids on Earth. But predicting the strength of the next cycle has always been difficult because no two cycles are exactly alike.

The Switch-Off Discovery

Professor Sandra Chapman of the University of Warwick and her team have developed a new method that changes the forecasting game. Using a tool called a "sunclock," which maps the Sun's irregular activity cycles onto a standard clock face, the researchers noticed something unexpected: the most extreme space weather events do not taper off gradually as the solar cycle declines. Instead, they stop almost entirely at a sharply defined point.

"The Sun doesn't gently go to sleep and then gently wake up again," said Professor Chapman. "Instead, we've discovered that the most extreme space weather switches off quite suddenly at a specific point in every solar cycle. By identifying that point, we've found a new way to predict how active the next solar cycle is likely to be."

How the Prediction Works

The number of sunspots present at this switch-off point is closely linked to the peak sunspot number of the following solar cycle. This means that by simply counting sunspots at the moment extreme weather ends, astronomers can forecast the next cycle's intensity — roughly six to seven years before it reaches its maximum. Current methods must wait until the solar minimum, giving far less lead time.

Using this approach, the team has made an early prediction for Solar Cycle 26: a moderate cycle with a peak sunspot number of around 100 to 120, similar to or weaker than the current Cycle 25. However, the prediction will not be finalized for another two years, when the current cycle reaches its actual switch-off point and observations replace projections.

Why This Matters

Solar storms can cause billions of dollars in damage to infrastructure. A strong geomagnetic storm in 1859 — the Carrington Event — set telegraph wires on fire. A similar event today could knock out power grids, disable GPS satellites, and disrupt global communications for weeks. Having a reliable long-range forecast of solar activity gives governments and grid operators years of preparation time rather than days.

The research was presented at the Royal Astronomical Society's National Astronomy Meeting in Birmingham, 2026. The team also hopes that the switch-off point will help scientists understand the solar dynamo — the still-mysterious process that generates the Sun's magnetic field — and unravel why solar cycles vary so much in strength and length.