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The sun is at its solar maximum — which means more auroras are likely in store


The Summary

  • The recent flurry of solar storms suggests the sun is in a period of maximal activity as part of its 11-year cycle.
  • The active period is likely to continue over the next year, so more auroras could be in store.
  • Next month, NASA will get an up-close view of the solar activity as the Parker Solar Probe makes its closest-ever approach to the sun.

The sun is awake.

In recent months, Earth’s star has ramped up activity, with giant flares erupting off the surface and belching streams of plasma and charged particles into space. Several of the solar storms have been aimed at our planet, and they triggered severe geomagnetic storms and supercharged dazzling displays of the northern lights.

The sun’s flurry of outbursts, coming after years of relative quiet and calm, is a sure sign that the star has entered a busy phase of its natural cycle, according to experts: solar maximum.

The active period is likely to continue over the next year, which means more solar storms and spectacular auroras could be in store.

“This is definitely the season for big solar storms,” said Kelly Korreck, a program scientist in the heliophysics division at NASA. “I expect we will see the skies lit up with auroras again.”

Aurora Borealis.
The aurora borealis above Kiruna, Sweden, on March 7.Leon Neal / Getty Images file

Later this month, NASA will get an up-close view of the high solar activity as the agency’s Parker Solar Probe makes its closest-ever approach to the sun on Dec. 24.

The spacecraft is on a path to swoop within 3.86 million miles of the solar surface — closer than any other human-made object in history. It is expected to fly through plumes of the sun’s plasma and potentially dive into active regions of the star.

“If you think of an American football field, and Earth is on one side and the sun is on the other, this is like going to the sun’s 4-yard line,” Korreck said.

Parker Solar Probe
The Parker Solar Probe in a clean room in Titusville, Fla., in 2018, after the installation of its heat shield.Johns Hopkins APL / Ed Whitman / NASA

The Parker Solar Probe launched in 2018 on a mission to study the sun’s atmosphere, an ultrahot region known as the corona. Last month, the car-size spacecraft flew by Venus in a maneuver that will help slingshot it near the sun.

Korreck said the probe’s close encounter could yield especially valuable insights if there are active sunspot regions — temporary features that appear as dark blemishes on the sun’s surface — along its path. Such observations could help researchers better understand how the sun’s activity waxes and wanes.

The solar cycle generally lasts around 11 years, as the sun transitions from periods of low to high magnetic activity. As the star moves out of its calm phase — solar minimum — and reaches the height of the solar cycle, its magnetic poles flip, ushering in solar maximum, when activity is heightened and eruptions become more frequent and intense.

The main way scientists can tell that the sun has reached its maximum is by monitoring sunspot formation. As the sun spins, its magnetic field becomes roiled, warping and tightening in some areas, Korreck said. That’s what creates the sunspots that appear in telescope images as dark patches.

Giant, bright coronal loops trace out the magnetic field lines above an active region.
Giant, bright coronal loops trace out the magnetic field lines above an active region of the sun in 2018.Solar Dynamics Observatory / NASA

“The sun is a magnetic ball, but because it doesn’t move as a solid object, its magnetic field gets all twisted up as it turns,” Korreck said.

The number of those sunspots steadily increases as the star moves toward solar maximum. Once there is a notable decline, researchers can define the start and end of the active period.

In some sunspot areas, the magnetic field can be about 2,500 times stronger than Earth’s magnetic field, according to NASA. Over time, sunspots can release enormous amounts of pent-up magnetic energy in the form of solar storms.

Two major solar storms this year — one in May and another in early October — stunned skywatchers as far south as Texas and Alabama with night skies painted in bright pink, green and purple hues. The event in May was the strongest geomagnetic storm to hit Earth in two decades, according to NASA.

Aurora borealis.
A solar storm over the National Monument of Scotland in Edinburgh on May 10.Jacob Anderson / AFP – Getty Images file
A cactus in an Aurora borealis.
The aurora borealis illuminates the sky over the desert in Tonto National Forest, northeast of Phoenix, on Oct. 10.Michael Chow / USA Today Network

Auroras occur when clouds of charged particles that spew from the sun during solar storms slam into Earth’s magnetic field and interact with atoms and molecules in the planet’s upper atmosphere. The colorful displays are a beautiful byproduct of that process, typically visible only at high latitudes. But during periods of intense solar activity, the lights can wander much farther south than usual.

But there can be negative consequences, as well. Strong geomagnetic storms can cause problems for astronauts in space, along with GPS systems and satellites in orbit.



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