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Those Beautiful Auroras Were From A Major Solar Flare
Live Science
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1/19/2025
After Northern Lights appeared as far south as Colorado, Live Science discusses how "cannibal" coronal mass ejections (CME) are formed and what impact they have on Earth.
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Transcript
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00:00
There are some beautiful auroras happening in the northwest of America right now.
00:04
Yeah, so like NOAA scientists have given this a really, really simple explanation,
00:09
and it's called a cannibal coronal mass ejection.
00:14
That's the thing that's causing all of these auroras going on right now.
00:19
Cannibal corona mass ejection.
00:22
Yeah.
00:22
That sounds a little terrifying.
00:24
I mean, it's kind of funny, right?
00:25
Because just as soon as we get over one kind of corona, we get hit by another.
00:28
But this one, a cannibal coronal mass ejection, if I break that down for you,
00:34
it's caused by sunspots.
00:36
So there's a sunspot on the sun called AR2975 right now.
00:41
And what it's been doing over the last, say, few days is producing up to 17 solar eruptions,
00:48
two of which have headed straight towards us.
00:52
Now, one of them was traveling faster than the other.
00:55
It was the one that came just after the first one that was emitted.
01:01
Now, when that second coronal mass ejection caught up with the first, it cannibalized it.
01:09
It swept it all up into this one big wave of these charged particles,
01:14
and then they all swept towards the Earth.
01:16
And then when they hit it, they caused a geomagnetic storm.
01:21
Where they come from in how sunspots are created is magnetic fields are created on the sun.
01:26
The sun is just a giant ball of plasma.
01:29
So there's loads of charged particles eddying and moving around inside the sun, across the
01:34
sun's surface.
01:35
Now, when you have charged particles moving, you're going to induce some magnetism there.
01:40
But because magnetic field lines can't cross, and you've got all these moving particles,
01:44
like this giant traffic jam of particles moving everywhere,
01:47
you'll inevitably get these field lines bunched up next to each other.
01:50
They'll form into these tight knots that can't escape anywhere else.
01:54
And eventually, they will have to snap and release energy.
01:58
Now, they release energy either in the form of a solar flare, like a bright flare of radiation,
02:03
or they'll release energy in the form of like chucking out some of that plasma from the sun.
02:07
What's the difference between solar flares and coronal mass ejections?
02:11
So solar flares is just the bright flash that you'll see of radiation
02:16
from that field line snapping that energy release.
02:19
A coronal mass ejection is some of the sun's plasma soup actually being burped out of the sun.
02:26
I love that phrase, plasma soup.
02:28
Yeah, tasty plasma soup.
02:31
I mean, pretty, but I mean, a little terrifying, right?
02:36
I mean, does it affect Earth?
02:40
So it does.
02:41
But not in like a...
02:44
So not in an always really terrible way.
02:47
Most of the time, the Earth has a pretty strong magnetic field,
02:51
which is really, really good news for us,
02:53
because it protects us from all of these like highly energized particles
02:57
that the sun has just spewed out at us.
02:59
In this case, at like speeds of like 2 million miles per hour,
03:02
which is just, I guess, 33 times less than the speed of light.
03:06
Pretty quick.
03:07
So what the Earth's magnetic field will do is it will absorb all of these particles.
03:14
The energy will go into stretching out the magnetic field in space.
03:18
So it's like it's kind of bunched out towards the...
03:21
It gives it a long tail.
03:24
And then most of those particles will gather kind of towards the poles
03:29
where they will like go downwards and then energize some of the molecules in the atmosphere.
03:36
And when these molecules in the atmosphere then give out light
03:41
in order to kind of go down to a lower energy level,
03:44
that's why we see the aurora.
03:46
Now, because there's so many of these like particles coming in,
03:50
you're getting auroras much lower down along the northern hemisphere
03:54
than you would normally expect to see.
03:57
That's a pretty...
03:59
That's a nice effect there.
04:01
And I know that people had already taken video from it.
04:06
This is from Manitoba in Canada.
04:11
Beautiful.
04:11
Just absolutely beautiful.
04:13
Yeah, yeah, yeah.
04:14
And like I think also you could see the aurora in the U.S.
04:17
certainly like as far south as Pennsylvania, Iowa and Oregon over the last few days as well.
04:23
Oh, right.
04:24
On spaceweather.com that you guys were sharing information from,
04:29
they showed some pictures.
04:30
Purple.
04:31
I mean, purple.
04:33
What an aura that Earth is giving off of this aurora.
04:37
And when you mentioned poles,
04:41
I'm like, that's why they're always up there towards the poles.
04:44
We got to get closer to some poles, Ben.
04:46
Yeah, yeah.
04:47
But so, okay.
04:48
So that's the good.
04:51
How about damage?
04:53
Okay, yes.
04:54
So damage.
04:57
So they can cause damage.
04:59
So one of the most recent kind of power outages that was caused by a storm of this type
05:06
was the 1989 Quebec power cut, which was caused by a geomagnetic storm.
05:11
Now, most of the time,
05:13
especially when it comes to people who provide like power lines and stuff,
05:16
a lot of them have shielded like their power cables and things like that
05:20
with a kind of Faraday cage, basically, which diverts the energy.
05:25
Or they also have like other techniques that allow them to kind of siphon off excess energy
05:30
that might be given to power lines by storms like this.
05:33
But like that hasn't always been the case.
05:35
Like, especially back in 1859,
05:38
there was a really big event called the Great Carrington event,
05:41
which was the largest sort of solar storm in modern human history.
05:45
I'm sure there have been solar storms just as large throughout our past.
05:50
But like before that point, we weren't really documenting it.
05:53
We didn't have many electronics around, so we didn't really care.
05:57
But in this case, the Great Carrington event fried
06:01
most of the telegram systems in the US and in Europe that had been developed at the time.
06:06
And it also led to auroras that could be seen around like as far south as the Caribbean.
06:13
And like there were people waking up at night,
06:16
thinking that it was daytime in the Caribbean
06:20
because of these enormous auroras from this event.
06:23
I mean, we're freaked out about it now when we see things like that.
06:26
We know more, but I can't even imagine, you know, over 100 years ago.
06:30
Yeah, exactly.
06:32
In terms of more modern sort of phenomena that have caused more modern damage,
06:37
other than the Quebec event,
06:39
recently, actually, there was another geomagnetic storm
06:42
that caused the downing of 40 of SpaceX's Starlink satellites.
06:48
That was one thing that happened.
06:50
And on top of that as well,
06:52
there's a potential risk that the internet in general,
06:57
especially in the United States, could be cut out by a geomagnetic storm
07:02
because a lot of these cables run underwater
07:05
through latitudes that would be affected by it.
07:09
And you would have a geomagnetic storm.
07:12
They're not shielded.
07:13
So they would basically be probably quite severely affected by this.
07:16
But as is the case with a lot of things and how they're done with legislation,
07:22
it's like earthquakes.
07:22
It doesn't often get legislated for until the worst has already happened.
07:26
Yeah, that's a shame.
07:27
I mean, I really like the internet.
07:29
I really, I like to keep it around.
07:31
This is how we get to communicate, right?
07:36
But you're saying that we have protections now.
07:39
So I think most power companies have already built in protections
07:44
into their grids for these kind of things.
07:46
It's just, yeah, you're not going to be getting any,
07:49
I guess, coronal mass ejection memes in the middle of a coronal mass ejection.
07:53
You have to wait a few weeks for them to fix the underwater cables.
07:57
Yeah.
07:57
And luckily, Earth, we have this nice electromagnetic shield, right?
08:02
Already built in, otherwise we'd be goners.
08:05
Yeah, it would fry us and it would also fry our atmosphere.
08:08
Like a big reason why Mars doesn't have much of an atmosphere, for instance,
08:11
is it doesn't really have a very active magnetic field.
08:14
So all of the atmosphere, when it gets hit by this wave of hydrogen particles,
08:21
like these protons, the atmosphere gets stripped away quite quickly.
08:25
Poor Mars, poor Mars.
08:27
Yeah.
08:28
But that's why we're here, right?
08:30
I mean, we are on Mars, but not yet.
08:33
Not yet, not yet.
08:34
Well, so is there a way to know when things like this will happen?
08:39
I know we watch the sun, we have video of the sun.
08:42
It seems more like after the fact.
08:46
Yeah.
08:46
So you get a bit of advanced warning.
08:49
For instance, the Great Carrington Event is named after Richard Carrington,
08:52
who spotted intense solar flares in the sky a few hours,
08:58
maybe about 15 hours before the actual event hit.
09:02
But the sun is quite a complex object.
09:05
There's loads going on in those magnetic fields.
09:08
It's still really, really hard for scientists to predict what's going on there.
09:11
Yeah, if only, if only.
09:14
Well, until the next major astronomical event.
09:18
Thanks so much, Ben.
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