How Do Auroras Form? A Dance of Solar Fire and Magnetic Veils

Some call them northern lights, but I call them the thing I’ve wanted to see my whole life. My husband is from Minnesota and rolls his eyes whenever I talk about them longingly. Apparently they’re very overrated when you’ve grown up with them in the sky.

But auroras are more than a visual feast to long after (or think indifferently about apparently), they’re a conversation between stars and planets, radiation and resistance, and between fire and shield.

They don’t begin their lives on Earth, but in the sun’s volatile lungs, and what we see (those green ribbons, purple flames, ghostly pulses across the poles) isn’t light, really.

It’s actually a reaction, a celestial side effect of something far older and wilder than I could’ve ever imagined.

Where Auroras Really Begin

Every so often, the sun loses its temper and throws a little fit.

It hurls plasma, charged particles, accelerated to incredible speeds into space. These are what we call solar flares and coronal mass ejections (CMEs), they’re storms born of magnetism and heat.

When these high-energy particles reach Earth, they don’t hit us directly. Instead, they meet something invisible and crucial to our protection, our magnetosphere. If you’ve never given this a thought a day in your life, don’t feel bad, I hadn’t either.

This magnetic shield, generated by the molten core of our planet, deflects most solar radiation and keeps us safe from angry plasma-throwing suns.

But near the poles, it bends a little and lets just enough in. When those solar particles collide with the gases in our atmosphere (oxygen & nitrogen the good ole Google tells me) they get all excited and glow. And that glow is the aurora we ooo and ahh at. Well…some of us anyway.

You might be wondering why some auroras are different colors (if you weren’t, I was doing it for you). It’s chemistry, cloaked in poetry of light waves and physics.

Green: the most common color, caused by oxygen about 60–150 miles above Earth.
Purple or Violet: nitrogen molecules excited at lower altitudes.
Red: rare and dramatic, caused by high-altitude oxygen (300+ miles above us).
Blue: nitrogen, but only under intense solar activity.

Each hue is carrying around some evidence of a particular gas meeting a particular energy at a particular height. Particular, no?

They’re not just pretty too, they’re coded messages from space playing telephone with our atmosphere.

Auroras Are Not Just Earth’s Phenomenon

Auroras shimmer on Jupiter, Saturn, and Uranus too. They shimmered last month on Mars for the first time we’ve seen, when a surge of solar particles lit up its thin sky in green light, captured for the first time by NASA’s Perseverance rover.

(Read about the sun’s awakening and Mars’s aurora here.)

Each planet has a different magnetic field and atmosphere, so each aurora is unique.

But the dance is the same curtsy and waltz. The sun throws sparks and the planets answer with color.

In 1859, a solar storm so intense hit Earth that the auroras were seen all the way in Cuba. Telegraphs caught fire, compasses spun wildly, and messages were transmitted without being connected to a power source. Spooky, eh?

It was called The Carrington Event, and if it happened today, it would disrupt satellites, power grids, and entire economies.

The aurora then wasn’t just a light show, it was a warning flare. Our relationship with the sun is beautiful, but also more fragile than we might realize.

What It Takes to See One

To witness an aurora, you need a geomagnetic storm (shouldn’t be too hard to come by these days, the sun is angry lately), clear, dark skies, and a location near the poles, or a rare event that pushes the aurora farther south than normal.

People chase them in Iceland, Norway, Alaska, and Canada. Sometimes, on lucky nights, they slip south, seen from Montana, or Michigan, Minnesota, or even as far as Oklahoma during extreme solar storms.

They don’t always shimmer, sometimes they pulse and flicker oddly while they stretch across the sky in silence.

It’s not just light, it’s the cosmic language of the sun, space, and chemicals chilling in our air.

If you’re wondering if we’re seeing more auroras lately, the answer is yes. Because the sun is waking up like a toddler after a nap that only lasted about ten minutes.

We’re entering a period of heightened solar activity, with more flares, more CMEs, and more chances for auroras to appear farther and more frequently. This doesn’t just mean more beauty…it means more vulnerability to tech disruption, radiation surges, and satellite drift. So the next time you curse at your phone for failing you, just know it might not be its fault entirely.

But for sky-watchers, it means more opportunities to see the cosmos perform.

Why the Sun’s Color Isn’t What You Think

While we’re here, let’s clear something up: The sun isn’t yellow.

It’s white, like perfect white…light spread evenly across all visible wavelengths.
It only appears yellow because of how our atmosphere scatters light. Our atmosphere just seems to enjoy dancing with light waves and plasma of all shapes and sizes.

So what you see gold at noon and crimson at dusk is an illusion. A beautiful lie if you will. Not true in any sense of the word.

Auroras are sort of the opposite. They look like fantasy brought to life, but they’re realer than we realize.

The sun doesn’t try to be poetic and artistic, it simply exists…violent, vast, and pulsing with power.

And Earth…well, I’d like to think we’re its favorite satellite. Close enough to be warmed, but far away enough to not be destroyed. And in the zones where our magnetic guard weakens…they meet. It’s your planet, protecting you in color.

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Michele Edington (formerly Michele Gargiulo)

Writer, sommelier & storyteller. I blend wine, science & curiosity to help you see the world as strange and beautiful as it truly is.

http://www.michelegargiulo.com
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The Sun Is Waking Up, and the Earth May Feel It