Solar maximum: What is it and when will it occur?

Solar maximum refers to the highest rate of solar activity during the sun’s approximately 11-year solar cycle. It is indicated by the intensity and frequency of sunspots visible on the surface.

Solar minimum is the opposite of solar maximum and marks the lowest rate of solar activity during a given solar cycle.

Solar activity has been gradually gaining strength during its current Solar Cycle 25, and the National Oceanic and Atmospheric Administration’s (NOAA) Space Weather Prediction Center (SWPC) estimates that solar maximum will occur between late 2024 and early 2026.

However, scientists cannot know whether the solar maximum has been reached until at least seven months after the fact due to how the solar maximum is computed.

Solar maximum FAQs

What is solar maximum?

Solar maximum refers to the highest rate of solar activity during its approximately 11-year solar cycle.

When was the last solar maximum?

The last solar maximum was reached in April 2014 according to the World Data Center for the Sunspot Index and Long-term Solar Observations (SILSO), it was part of Solar Cycle 24.

Is solar maximum happening now?

Solar activity is gaining strength but scientists cannot determine whether solar maximum has occurred until at least seven months after the fact. According to the National Oceanic and Atmospheric Administration’s (NOAA) Space Weather Prediction Center (SWPC), solar maximum is predicted to occur between late 2024 and early 2026.

Solar maximum 2024

Solar maximum corresponds to heightened solar activity. (Image credit: Science Photo Library via Getty Images)

We are currently experiencing Solar Cycle 25 and as it stands, predictions from the World Data Center for the Sunspot Index and Long-term Solar Observations (SILSO) at the Royal Observatory of Belgium indicate a maximum between mid-2024 and the end of 2025. Meanwhile, NOAA’s Space Weather Prediction Center (SWPC) estimates that solar maximum could occur between late 2024 and early 2026.

Predicting when solar maximum will occur is no mean feat. Scientists compute solar maximum through careful analysis of the frequency of sunspots visible on the sun‘s surface.

Graph showing solar cycle progression with measured and predicted values. There is a distinct peak between 2024 and 2026 when solar maximum is expected to occur.

Solar cycle progression graph showing a peak between late 2024 and early 2026. (Image credit: NOAA Space Weather Prediction Center)

“The maximum is computed (as a convention) with the 13-month smoothed sunspot number (which means that for each month you use the value of six months before and six months after),” ESA’s SSA Space Weather Coordination Centre (SSCC) solar expert service center told Space.com in an email. “The exact value of this quantity for time T is known only 6 months later” the SSCC solar scientists continued.

For example, let’s say solar maximum did occur in April 2024. Scientists would need sunspot number data from the previous six months, the month of April 2024 and the next six months which would take us to October 2024. So we would have to wait until November 2024 to be able to declare that solar maximum had occurred in April 2024.

And sometimes just when we think we’ve got it all figured out, the sun can fool us! Increased solar activity can sometimes turn out to be what is known as a ‘local maxima’ and not representative of the entire solar cycle. Sunspot cycles can also experience ‘double maxima’, called a Gnevishev’s gap, which means that the first peak might not be the highest and another large peak can follow.

All of this means we could have some time to wait before we know exactly when Solar Cycle 25’s solar maximum has occurred.

Does solar maximum affect the northern lights?

the sky is illuminated by ribbons of green and blue light which is reflected in the water below, that contains several large rocks.

The northern aurora lights up the sky over the Gulf of Finland. (Image credit: Shutterstock)

The northern lights (aurora borealis) and the southern lights (aurora australis) are created when energized particles from the sun hit Earth’s atmosphere and are funneled toward the poles by our planet’s magnetic field. As the particles are redirected toward the poles, they interact with our atmosphere, by depositing energy and causing the atmosphere to fluoresce. During times of heightened solar activity around solar maximum, a greater amount of energized particles can be emitted from the sun, through large expulsions of plasma and magnetic fields known as coronal mass ejections (CMEs), solar flares and increased solar wind. These energized particles can trigger geomagnetic storms, also known as solar storms — large disturbances in Earth’s magnetosphere which, in turn, can lead to stronger aurora displays.

You might have seen various media outlets claiming “THIS is the year for the northern lights, book now for the BEST displays!” or something to that effect. While it is true that heightened solar activity can lead to more dynamic aurora displays, it is somewhat misleading to claim that this year is THE time to see them because of ‘solar maximum’.

Firstly, we still don’t know when solar maximum will occur, so for all we know, solar activity could still ramp up until early 2026 according to NOAA’s SWPC estimates. Solar maximum is also not a single moment in time and can last for years. When scientists calculate the ‘absolute maximum’ it refers to the moment the sun’s magnetic field flips and indicates the halfway point, with half of the solar maximum over and half still to come.

Secondly, auroras are visible at any time in the solar cycle, even during solar minimum. The sun doesn’t stop bombarding us with energetic particles just because its activity has reduced. For example, the last solar minimum — when the sun is least active — occurred in December 2019. In the same year, several months earlier on March 26, photographer Miguel Claro captured this stunning display of springtime auroras. This is evidence that even during periods of weakened solar activity, it’s still possible to see a truly remarkable sight.

And last but not least, auroras are fickle creatures, you can have the perfect geomagnetic conditions and fail to see a show, or it can be in the middle of solar minimum and suddenly the skies light up with an exquisite display. So while heightened solar activity over the next few years increases your chances of seeing the northern lights, you need to be aware that this is not a guarantee nor does it mean you can’t see them at any other time during the solar cycle.

Solar maximum expert Q&A

We spoke with Mark Miesch, space weather research scientist at NOAA’s Space Weather Prediction Center (SWPC) about solar maximum.

Mark Miesch

Mark Miesch is a research scientist and member of the solar and solar wind modeling team at NOAA’s Space Weather Prediction Center (SWPC)

How was the solar cycle discovered?

Humanity has known for over 2,000 years that the sun sometimes has dark spots on it that we call sunspots (best viewed now with a solar telescope — don’t look directly at the sun!). More than 150 years ago, scientists noticed that the average number of sunspots rises and falls approximately every 11 years. We call this the solar cycle.

What happens during solar maximum?

Solar maximum is the peak of the solar cycle — when the average number of sunspots is larger than at any other time during the cycle. So, it happens roughly every 11 years but the time between solar maxima can be as short as 9 years or as long as 13 years. The last solar maximum was in 2014 and we expect the next solar maximum to occur a little earlier than average, in 2024.

How long does solar maximum last?

Though solar maximum is often referred to in terms of the month where the sunspot number peaks, the associated period of high activity lasts longer than that — from one year to over two years. So, in the current solar maximum, we expect high levels of solar activity throughout 2024 and likely into 2025.

What does solar maximum mean for us on Earth? Is it dangerous?

We now know that sunspots are a magnetic phenomenon and that magnetic fields have energy.

When that magnetic energy is released explosively, it can power colossal solar storms known as solar flares and coronal mass ejections (CMEs). When the effects of those storms reach Earth, they can damage electrical power grids, disable satellites, disrupt radio communications and GPS navigation, and endanger astronauts brave enough to venture outside the protective confines of Earth’s atmosphere and magnetosphere.

Though a large solar storm has the potential to be a natural disaster on the scale of a hurricane, most average citizens don’t have to worry much about space weather. If we do our jobs right in forecasting solar storms and if the power companies, satellite companies, airlines and other industries do their jobs in responding to them, then most people will not notice much of a difference between solar minimum and solar maximum. That is, unless you live at high latitudes, where the enhanced activity around solar maximum will produce celestial light shows that we call the aurora.

Additional resources

Check out NOAA’s Space Weather Prediction Center (SWPC) for official space weather forecasts for the U.S. Explore more about space weather impacts with NOAA’s SWPC. See the solar cycle like never before with this impressive composite image from the Solar and Heliospheric Observatory (SOHO), which shows changes in the sun’s appearance over the solar cycle. If you’re an avid aurora chaser or want to learn more about sightings all over the world, Aurorasaurus is a citizen science site where you can report your aurora sightings and also learn more about auroras with their informative blog.