WEBVTT

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<v Speaker 1>Welcome to Bedtime Astronomy. Explore the wonders of the cosmos

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<v Speaker 1>with our soothing Bedtime Astronomie podcast. Each episode offers a

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<v Speaker 1>gentle journey through the stars, planets, and beyond, perfect for

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<v Speaker 1>unwinding after a long day. Let's travel through the mysteries

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<v Speaker 1>of the universe as you drift off into a peaceful

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<v Speaker 1>slumber under the night sky.

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<v Speaker 2>I want you to tray something for me real quick.

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<v Speaker 2>Just close your eyes for a second. Imagine you are

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<v Speaker 2>standing outside on a really perfect day. It's mid July.

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<v Speaker 2>Maybe you're at the beach or just hanging out in

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<v Speaker 2>your backyard, and you feel that warmth hitting your face.

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<v Speaker 2>It feels totally consistent, right. It feels a steady, like

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<v Speaker 2>a reliable old radiator that just you know, keeps the

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<v Speaker 2>whole planet alive.

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<v Speaker 3>It is a very comforting sensation. Yeah, honestly, it is

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<v Speaker 3>the definition of stability for most of us.

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<v Speaker 2>But here's the thing about that feeling. It is a

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<v Speaker 2>complete lie. Ah, It is a total illusion, because if

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<v Speaker 2>we could strip away the distance, if we could zoom in,

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<v Speaker 2>and I mean really really zoom in, that steady ball

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<v Speaker 2>of light is actually a screaming, chaotic nightmare of nuclear fire.

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<v Speaker 3>Well, nightmare might be a bit subjective, but chaotic is

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<v Speaker 3>definitely scientifically precise to us. It's a light bulb, but

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<v Speaker 3>up close it's a battlefield, right.

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<v Speaker 2>And usually when we talk about this, we talk about

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<v Speaker 2>the big explosions, the flares, the coronal mass ejections that

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<v Speaker 2>sound like doomsday.

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<v Speaker 3>Weapons, dramatic events.

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<v Speaker 2>Yeah, But today, for this exploration, we are looking at

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<v Speaker 2>something different, something strangely organized amidst all that chaos. I

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<v Speaker 2>want you to picture a giant blast of glowing gas,

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<v Speaker 2>but instead of just exploding everywhere randomly, it forms a shape,

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<v Speaker 2>a very specific shape.

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<v Speaker 3>We are talking about turbulence, but not just random turbulence.

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<v Speaker 3>We're talking about structure.

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<v Speaker 2>We are talking about smoke rings. We are giant planet

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<v Speaker 2>size smoke rings rolling off the surface of the Sun.

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<v Speaker 2>It sounds completely impossible, but we are going to unpack

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<v Speaker 2>a major new study that says this is exactly what

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<v Speaker 2>is happening right now.

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<v Speaker 3>And this is an old news by the way, this

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<v Speaker 3>is very fresh from the.

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<v Speaker 2>Lab, literally days old. This study comes from the University

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<v Speaker 2>of Hawaii at MANOAH, published just two days ago February eighteenth,

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<v Speaker 2>twenty twenty six. It's in the Astrophysical Journal, which I'm

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<v Speaker 2>told is a pretty huge deal.

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<v Speaker 3>Oh, it is the gold standard for this kind of research.

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<v Speaker 3>If it is in there, the data has been put

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<v Speaker 3>through the absolute ringer.

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<v Speaker 2>The research is led by A. Shadia Habal at the

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<v Speaker 2>Institute for Astronomy, and what her team found it basically

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<v Speaker 2>changes how we understand the Sun's atmosphere. They found that

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<v Speaker 2>the Sun is pumping out these aerodynamic shapes vortex rings

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<v Speaker 2>that actually travel through space. It's literally like the Sun

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<v Speaker 2>is blowing smoke rings at us.

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<v Speaker 3>It is a fantastic image, but the physics behind it

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<v Speaker 3>are even more interesting because this is about energy transfer,

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<v Speaker 3>It is about the invisible machinery that drives space weather,

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<v Speaker 3>and ultimately it is about understanding the environment we actually live.

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<v Speaker 2>In, because, as you always remind me, we don't just

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<v Speaker 2>live on Earth. We actually live inside the atmosphere of

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<v Speaker 2>the Sun.

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<v Speaker 3>We do, we absolutely do, and that atmosphere is a

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<v Speaker 3>lot more turbulent than we ever thought.

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<v Speaker 2>So let's start this investigation. We have the what is

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<v Speaker 2>the smoke rings on the Sun, But I really want

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<v Speaker 2>to start with the how, because when I was reading

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<v Speaker 2>through the study, one thing stood out immediately. They didn't

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<v Speaker 2>find this using the ten billion dollar James Webb telescope.

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<v Speaker 2>They didn't find it using the Solar Dynamics Observatory or

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<v Speaker 2>some giant satellite can use the moon, right, They used

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<v Speaker 2>a solar eclipse. And I have to ask the really

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<v Speaker 2>obvious question. Here we are in twenty twenty six. We

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<v Speaker 2>have probes that can literally touch the Sun as atmosphere.

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<v Speaker 2>Why are we still relying on a rock floating in

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<v Speaker 2>front of the Sun to do cutting edge science? Why

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<v Speaker 2>is the moon a better tool than our best technology?

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<v Speaker 3>It is a fair question. It feels a bit analog,

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<v Speaker 3>doesn't it Like using a sun dial in the age

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<v Speaker 3>of the Apple Watch?

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<v Speaker 2>Exactly? It feels complete nage.

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<v Speaker 3>But it all comes down to a very specific problem

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<v Speaker 3>in optics called dynamic range. Think about it this way.

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<v Speaker 3>Imagine you were driving at night and a car is

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<v Speaker 3>coming towards you with its high beams blaring. You are

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<v Speaker 3>completely blinded. Yeah, Now imagine a moth flies right in

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<v Speaker 3>front of those headlights. Can you see the moth?

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<v Speaker 2>No? Way, The glare is way too strong.

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<v Speaker 3>Right, The signal to noise ratio is impossible. The Sun

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<v Speaker 3>is millions of times brighter than its outer atmosphere, which

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<v Speaker 3>we call the corona. To see the corona, that faint,

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<v Speaker 3>wispy moth, you have to block.

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<v Speaker 2>The headlight, which is what we do with satellites, isn't it.

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<v Speaker 2>They have those little metal disks inside them, corona graphs

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<v Speaker 2>they do.

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<v Speaker 3>We build artificial eclipses inside our telescopes. We put a

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<v Speaker 3>little disk right in front of the sensor to block

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<v Speaker 3>the sun. But here's the problem with that diffraction.

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<v Speaker 2>Okay, walk us through diffraction.

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<v Speaker 3>When light hits the edge of that metal disk inside

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<v Speaker 3>the telescope, it bends, it scatters, It creates this fuzzy

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<v Speaker 3>bright edge. To keep that stray light from completely ruining

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<v Speaker 3>the image, we have to make the blocking disc slightly

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<v Speaker 3>larger than the sun itself. We have to overblock.

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<v Speaker 2>Oh so you're covering the Sun, but you're also covering

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<v Speaker 2>the most interesting part, the edge where the surface actually

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<v Speaker 2>meets the atmosphere exactly.

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<v Speaker 3>We lose the inner corona, We lose the shore line

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<v Speaker 3>basically because we are blocking the view of the ocean

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<v Speaker 3>just to save our eyes. But the moon, the moon

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<v Speaker 3>is perfect nature's lens cap. It really is. It is

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<v Speaker 3>effectively infinitely far away from the observer on Earth, so

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<v Speaker 3>there's no scattering inside your eye or inside the telescope.

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<v Speaker 3>It fits over the Sun with incredible precision. When the

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<v Speaker 3>Moon blocks that bright disc, we can see right down

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<v Speaker 3>to the surface. We get this eclipse view that reveals

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<v Speaker 3>details no satellite can match.

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<v Speaker 2>And the study mentions this specifically. It says that standard

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<v Speaker 2>satellite observations show a smoothed out view of the corona.

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<v Speaker 3>Right, if you look at a satellite image, the corona

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<v Speaker 3>looks like this soft, growing halo. It looks almost static,

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<v Speaker 3>like a painting.

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<v Speaker 2>But the eclipse view, the eclipse.

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<v Speaker 3>View reveals the truth. It isn't a soft halo at all.

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<v Speaker 3>It is made of thousands of sharp, distinct threads. It

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<v Speaker 3>is far more dynamic.

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<v Speaker 2>Dynamic is just the polite scientist word for chaos.

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<v Speaker 3>Right in this context, yes, it means everything is moving,

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<v Speaker 3>twisting and changing constantly. These threads are magnetic field lines,

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<v Speaker 3>and they are guiding the plasma in very complex ways.

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<v Speaker 3>But here is the real kicker with this specific study

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<v Speaker 3>from the University of Hawaii. They didn't just take one

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<v Speaker 3>picture of one eclipse and call it a day.

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<v Speaker 2>That's the other part that blew my mind and eclipse

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<v Speaker 2>last what four minutes?

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<v Speaker 3>If you are lucky, sometimes it's two minutes.

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<v Speaker 2>So you have two minutes of data. How do you

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<v Speaker 2>build a massive scientific paper on two minutes of data?

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<v Speaker 3>You don't, You wait, you travel, and you do it again.

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<v Speaker 3>Shadiyahabal and her team didn't just chase one shadow. This

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<v Speaker 3>study utilizes data collected over nearly twelve years.

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<v Speaker 2>Twelve years. That is incredible dedication just chasing two minute

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<v Speaker 2>windows around the world.

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<v Speaker 3>It is fundamental though. Think about the Sun's heartbeat. The

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<v Speaker 3>Sun isn't the same every single day. It goes through

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<v Speaker 3>a cycle, the solar cycle, which is roughly eleven years long.

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<v Speaker 2>Right, solar minimum and solar maximum.

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<v Speaker 3>Exactly. At solar minimum, the sun is relatively quiet, the

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<v Speaker 3>magnetic field is organized. At solar maximum, the magnetic field

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<v Speaker 3>is a tangled mess, and the Sun is firing off

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<v Speaker 3>flares left and right. If you only looked at one

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<v Speaker 3>eclipse in say twenty fifteen, you wouldn't know if what

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<v Speaker 3>you saw was normal or just a weird Tuesday.

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<v Speaker 2>You need the whole movie, not just a screenshot.

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<v Speaker 3>Precisely, by tracking this over a full twelve year cycle,

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<v Speaker 3>have All's team can see the evolution they could prove

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<v Speaker 3>that these structures they found weren't just accidents. They are

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<v Speaker 3>a fundamental part of how the sun works.

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<v Speaker 2>Okay, so we have the perfect tool, the eclipse. We

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<v Speaker 2>have the long term data, twelve years of chasing shadows

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<v Speaker 2>across the globe. Now let's get to the thing they

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<v Speaker 2>actually found, the smoke rings.

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<v Speaker 3>The vortex rings.

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<v Speaker 2>Use the fancy term if you want, but they look

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<v Speaker 2>like smoke rings to me. The study describes turbulent structures

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<v Speaker 2>forming in the corona.

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<v Speaker 3>Yes, and this is a big deal because for a

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<v Speaker 3>long time the corona was thought to be fairly laminar, smooth,

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<v Speaker 3>flowing in straight lines like water in a calm river. Ay,

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<v Speaker 3>But what they found was turbulence, eddies, swirls, and specifically,

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<v Speaker 3>these vortex rings explain.

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<v Speaker 2>The physics of a vortex ring. To us, how do

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<v Speaker 2>you get a donut shape made of gas?

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<v Speaker 3>It is a fluid dynamics classic. A vortex ring forms

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<v Speaker 3>when a fast moving slug of fluid pushes through a

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<v Speaker 3>stationary or slower moving fluid. The friction at the edges

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<v Speaker 3>basically rolls the fluid back on itself.

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<v Speaker 2>Like blowing a smoke ring, you push the smoke out

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<v Speaker 2>quickly through your lips, and the air in the room

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<v Speaker 2>drags on the edges and it spins into a doughnut exactly.

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<v Speaker 3>Seeing this on the Sun tells us something very specific.

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<v Speaker 3>There is a massive speed difference involved. There is a

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<v Speaker 3>pulse of energy pushing plasma through the atmosphere at incredible speeds.

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<v Speaker 2>And the study also mentions rolling waves. They compared them

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<v Speaker 2>to clouds on Earth.

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<v Speaker 3>Yes, likely Kelvin Helmoltz instabilities. You have seen these before.

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<v Speaker 3>Have you ever looked up at the sky and seen

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<v Speaker 3>a cloud layer that looks like ocean waves breaking like

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<v Speaker 3>a perfect row of surfer curls.

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<v Speaker 2>Yeah, they look like a van go painting. It's super trippy.

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<v Speaker 3>Yeah, that happens when two layers of air moving past

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<v Speaker 3>each other in different speeds, the sheer force rolls the

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<v Speaker 3>boundary up into a wave. Finding that on the Sun

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<v Speaker 3>is remarkable, means the solar atmosphere isn't just hot gas

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<v Speaker 3>hanging there. It has weather, It has wind shear, it

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<v Speaker 3>has storms.

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<v Speaker 2>Makes the Sun feel so much more tangible. It's not

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<v Speaker 2>just a light source. It's a place, a place with

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<v Speaker 2>really really violent weather.

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<v Speaker 3>Violent is the right word, because remember on Earth, those

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<v Speaker 3>clouds are water vapor On the Sun, there are a

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<v Speaker 3>million degree plasma.

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<v Speaker 2>Which leads me to the next big question. On Earth

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<v Speaker 2>storms are caused by hot air meeting cold air, or

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<v Speaker 2>high pressure meeting low pressure. What causes a storm on

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<v Speaker 2>a star? What is the engine creating these smoke rings?

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<v Speaker 3>That is the core discovery of this paper. They trace

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<v Speaker 3>these smoke rings back to their source, and the culprit

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<v Speaker 3>is a structure called a prominence.

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<v Speaker 2>A prominence, I've seen pictures of these. They look like

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<v Speaker 2>big l loop sticking out of the sun like handlebars.

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<v Speaker 3>A good visual. A prominence is a large, bright feature

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<v Speaker 3>extending outward from the Sun's surface. It is anchored to

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<v Speaker 3>the Sun, usually in a loop shape. But here's the

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<v Speaker 3>thing that makes them chaotic. They are cold.

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<v Speaker 2>Okay, you keep doing this, you say cold when we

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<v Speaker 2>are talking about the Sun explained.

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<v Speaker 3>It is all relative. The corona, the outer atmosphere where

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<v Speaker 3>these things live, is bafflingly hot. It is over a

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<v Speaker 3>million degrees celsius. Okay, But the prominence, the material inside

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<v Speaker 3>that loop, it is much much cooler, maybe tens of

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<v Speaker 3>thousands of degrees.

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<v Speaker 2>So it's basically an ice cube in.

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<v Speaker 3>That specific environment. Yes, it is a dense, heavy, cool

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<v Speaker 3>iceberg of plasma sitting right in the middle of a

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<v Speaker 3>sparse million degree furnace.

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<v Speaker 2>And I'm guessing those two things don't get along.

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<v Speaker 3>Nature hates a sharp gradient. Nature wants equilibrium. When you

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<v Speaker 3>have cool, dense matter right next to hot, thin matter,

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<v Speaker 3>you create an incredibly unstable boundary. It's a plash. It

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<v Speaker 3>is a war zone of physics. The study explained that

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<v Speaker 3>where these two extremes meet, you get sharp changes in

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<v Speaker 3>temperature and density. This creates massive instability. The hot plasma

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<v Speaker 3>tries to rush in the cold plasma is heavy and

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<v Speaker 3>tries to fall. The magnetic fields are twisting to hold

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<v Speaker 3>it all together.

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<v Speaker 2>It sounds like a pressure cooker lid rattling before it blows.

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<v Speaker 3>That is a great analogy. And when it rattles, it

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<v Speaker 3>creates turbulence. It sheds these layers. The instability triggers the

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<v Speaker 3>formation of these vortex rings. It basically peels them off

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<v Speaker 3>the main structure.

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<v Speaker 2>So the smoke rings are essentially the exhaust from this

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<v Speaker 2>clash between the hot atmosphere and the cool loop.

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<v Speaker 3>Exactly. They're the visible sign of the Sun trying to

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<v Speaker 3>balance out this massive temperature difference.

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<v Speaker 2>Okay, so we have the storm, we have the smoke

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<v Speaker 2>rings forming, but usually turbulence just stops. If I stir

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<v Speaker 2>my coffee, the swirl lasts for a few seconds and

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<v Speaker 2>then friction kills it right.

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<v Speaker 3>In normal fluid dynamics, viscosity eats up the energy, the

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<v Speaker 3>turbulence dissipates into heat.

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<v Speaker 2>But Hubball's team says, these things don't just sit there

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<v Speaker 2>and fade out. They travel.

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<v Speaker 3>They do, and this is the part that connects the

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<v Speaker 3>Sun to us.

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<v Speaker 2>There's a quote from Haball in the notes. For the

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<v Speaker 2>first time, we were able to watch these turbulent structures

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<v Speaker 2>form near the Sun and then follow them as they

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<v Speaker 2>float outward.

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<v Speaker 3>Flowed outward. That implies survival.

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<v Speaker 2>But how did they track them? You just said the

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<v Speaker 2>eclipse only last a few minutes. You can't watch a

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<v Speaker 2>smoke ring travel a million miles and four minutes.

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<v Speaker 3>No, you can't. This is where they had to get

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<v Speaker 3>really clever and combine their ancient eclipse method with the

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<v Speaker 3>absolute cutting edge. They took the high resolution images from

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<v Speaker 3>the ground, the eclipse data, and they overlaid them with

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<v Speaker 3>data from space, which satellite the Parker Solar Probe, specifically,

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<v Speaker 3>the whisper instrument, the wide fueled imager for solar probe.

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<v Speaker 2>The Parker Solar Probe. That's the one that's basically hugging

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<v Speaker 2>the Sun right. Yeah.

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<v Speaker 3>It is the fastest man made object in history, and

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<v Speaker 3>it is actively diving into the solar corona. It is

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<v Speaker 3>flying through the very atmosphere we are discussing right now.

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<v Speaker 2>That is bonkers. So they take the picture from Earth

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<v Speaker 2>and they take the picture from the probe inside the corona.

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<v Speaker 3>And they match the structure. They saw the exact same

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<v Speaker 3>vortex rings in the eclipse data and in the space

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<v Speaker 3>based images.

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<v Speaker 2>That is the smoking gun.

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<v Speaker 3>It is, and it proves that these features remain intact

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<v Speaker 3>over enormous distances. They survive the journey away from the

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<v Speaker 3>Sun moving out into the Solar system.

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<v Speaker 2>How how does a swirl of gas hold its shape

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<v Speaker 2>for millions of miles magnetism.

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<v Speaker 3>If this were just normal gas, it would dissipate, Okay,

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00:13:25.080 --> 00:13:28.000
<v Speaker 3>but this is plasma. It is highly charged. It carries

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<v Speaker 3>a magnetic field. These vortex rings are essentially magnetic capsules.

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<v Speaker 3>The magnetic field locks the plasm in place, holding the

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<v Speaker 3>shape together as it travels through the vacuum.

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<v Speaker 2>So it's not just a puff of smoke. It's a

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<v Speaker 2>magnetic bullet.

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<v Speaker 3>That is a very evocative and somewhat concerning way to

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00:13:43.600 --> 00:13:43.879
<v Speaker 3>put it.

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<v Speaker 2>But yes, which brings us to the part of the

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<v Speaker 2>show where we ask, so what why should you or

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<v Speaker 2>I care? I'm sitting here on Earth drinking my coffee.

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<v Speaker 2>Why do I care if the Sun is firing magnetic

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<v Speaker 2>bullets into space?

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<v Speaker 3>Because you are in the line of fire? Comforting, We

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<v Speaker 3>need to talk about the solar wind.

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<v Speaker 2>Okay, the solar wind, I know it exists. It's the

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<v Speaker 2>stuff that makes the northern lights right, that is.

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<v Speaker 3>The beautiful side of it. Yes, the solar wind is

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<v Speaker 3>a constant stream of charged particles flowing out from the

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00:14:10.919 --> 00:14:14.080
<v Speaker 3>Sun in all directions. It fills the entire solar system.

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<v Speaker 3>But we have always had a really hard time explaining

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<v Speaker 3>exactly how it gets so fast. It actually accelerates as

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<v Speaker 3>it moves away from the Sun.

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<v Speaker 2>Which makes no sense at all. Gravity should be pulling

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<v Speaker 2>it back and slowing it down.

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00:14:26.440 --> 00:14:29.120
<v Speaker 3>Exactly. Something is pushing it, something is adding energy to

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<v Speaker 3>the flow.

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00:14:29.799 --> 00:14:32.039
<v Speaker 2>And let me guess the smoke rings.

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<v Speaker 3>The smoke rings. The study suggests that this turbulence, these

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<v Speaker 3>vortex rings and rolling waves plays a key role in

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00:14:40.639 --> 00:14:41.960
<v Speaker 3>accelerating the solar.

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<v Speaker 2>Winds, so they are like little booster rockets.

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00:14:43.919 --> 00:14:48.159
<v Speaker 3>They are packets of energy and momentum. As they travel outward,

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00:14:48.480 --> 00:14:51.840
<v Speaker 3>they transfer that energy to the surrounding particles, kicking the

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00:14:51.840 --> 00:14:53.600
<v Speaker 3>wind up to higher and higher speeds.

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00:14:53.720 --> 00:14:56.080
<v Speaker 2>So the storms on the Sun are basically the engine

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<v Speaker 2>that drives the wind that hits Earth.

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<v Speaker 3>Correct And that wind isn't just a gentle breeze when

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00:15:00.919 --> 00:15:02.440
<v Speaker 3>it hits Earth. We call it space weather.

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<v Speaker 2>Space weather. It always sounds like a bad sci fi

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00:15:04.840 --> 00:15:06.720
<v Speaker 2>movie title to me, But it's a real problem for

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00:15:06.759 --> 00:15:07.519
<v Speaker 2>our tech, isn't it.

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<v Speaker 3>It is a critical vulnerability for modern society. When the

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<v Speaker 3>solar wind is turbulent, when it is full of these

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<v Speaker 3>dense magnetic structures, it impacts Earth's magnetic field. It compresses it,

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<v Speaker 3>it shakes.

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00:15:20.120 --> 00:15:22.000
<v Speaker 2>It, and that shaking breaks things.

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00:15:22.039 --> 00:15:26.360
<v Speaker 3>It disrupts things heavily. The study explicitly lists the consequences. First,

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00:15:26.440 --> 00:15:30.519
<v Speaker 3>up satellites GPS. GPS, your phone knows exactly where you

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00:15:30.559 --> 00:15:32.879
<v Speaker 3>are because it receives a signal from a satellite with

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00:15:33.000 --> 00:15:36.799
<v Speaker 3>nanosecond precision. That signal has to pass through the ionosphere,

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00:15:36.840 --> 00:15:37.679
<v Speaker 3>the upper part of our.

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00:15:37.559 --> 00:15:39.679
<v Speaker 2>Atmosphere, and when a solar storm hits.

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<v Speaker 3>The honosphere gets churned up. It gets thicker in places,

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00:15:42.080 --> 00:15:44.080
<v Speaker 3>thinner in others. It delays the signal, and.

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<v Speaker 2>A delay means an error.

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<v Speaker 3>A delay means your phone thinks the satellite is further

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<v Speaker 3>away than it actually is. Suddenly your GPS says you're

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<v Speaker 3>driving in the middle of a lake.

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00:15:53.639 --> 00:15:55.519
<v Speaker 2>Which is annoying for me trying to mind a coffee shop,

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00:15:55.559 --> 00:15:57.960
<v Speaker 2>but probably a catastrophic for a self driving car or

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00:15:58.000 --> 00:16:00.240
<v Speaker 2>an airplane landing in fog exactly.

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00:16:01.000 --> 00:16:05.600
<v Speaker 3>Then there is radio communication, high frequency radios used by airlines,

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00:16:05.960 --> 00:16:08.159
<v Speaker 3>and the military can be completely blacked out.

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00:16:08.519 --> 00:16:11.440
<v Speaker 2>And the big one the power grid a grid.

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00:16:12.039 --> 00:16:15.480
<v Speaker 3>This is the black Swan event everyone fears in this field.

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<v Speaker 2>Explain how a storm on the Sun turns off the

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00:16:18.320 --> 00:16:19.240
<v Speaker 2>lights in Chicago.

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00:16:19.480 --> 00:16:23.279
<v Speaker 3>It is basic physics. A changing magnetic field creates an

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00:16:23.279 --> 00:16:26.480
<v Speaker 3>electric current. That's literal how a generator works. When a

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00:16:26.519 --> 00:16:30.039
<v Speaker 3>solar storm hits Earth, it causes our planet's magnetic field

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<v Speaker 3>to fluctuate wildly. It wiggles, it wiggles, and that wiggling

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00:16:32.759 --> 00:16:36.200
<v Speaker 3>field induces electrical currents in any long conductor on the ground,

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00:16:36.360 --> 00:16:41.120
<v Speaker 3>like power lines, like power lines, oil pipelines, undersea internet cables.

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00:16:41.440 --> 00:16:45.360
<v Speaker 3>Suddenly you have massive amounts of uncontrolled electricity flowing through

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00:16:45.399 --> 00:16:47.600
<v Speaker 3>wires that were definitely not designed.

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00:16:47.240 --> 00:16:50.080
<v Speaker 2>For it, and the transformers explode, they melt.

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00:16:50.559 --> 00:16:54.039
<v Speaker 3>It has happened before. The nineteen eighty nine Quebec blackout

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00:16:54.080 --> 00:16:58.000
<v Speaker 3>is the classic example. Six million people lost power in

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<v Speaker 3>ninety seconds because of the solar storm.

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00:17:00.200 --> 00:17:02.240
<v Speaker 2>And that was nineteen eighty nine. We didn't have nearly

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00:17:02.279 --> 00:17:03.519
<v Speaker 2>as much tech dependency then.

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00:17:03.639 --> 00:17:07.079
<v Speaker 3>Exactly, we are far more vulnerable now. So bringing it

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00:17:07.119 --> 00:17:10.240
<v Speaker 3>back to Shorty A. Hubball's research, this isn't just about

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<v Speaker 3>finding cool shapes in the corona.

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<v Speaker 2>It is about prediction, right, because if we know how

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<v Speaker 2>these things form in the first.

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00:17:15.960 --> 00:17:20.519
<v Speaker 3>Place, exactly, Hubball says, understanding where this turbulence comes from

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00:17:20.680 --> 00:17:24.160
<v Speaker 3>is key to predicting those impacts. If we know that

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<v Speaker 3>a specific type of prominence interacting with the corona in

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00:17:27.359 --> 00:17:30.599
<v Speaker 3>a specific way generates these vortex.

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00:17:30.240 --> 00:17:32.200
<v Speaker 2>Ranks, we can spot it before it hits us.

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00:17:32.240 --> 00:17:33.839
<v Speaker 3>We can look at the sun and say, okay, see

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00:17:33.839 --> 00:17:36.799
<v Speaker 3>that loop on the eastern edge. It's unstable, it's pumping

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00:17:36.799 --> 00:17:39.240
<v Speaker 3>out turbulence. We're going to see a spike in solar

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00:17:39.279 --> 00:17:41.119
<v Speaker 3>wind velocity in three days.

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00:17:40.960 --> 00:17:43.000
<v Speaker 2>And that actually gives us time to prepare.

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00:17:43.240 --> 00:17:45.799
<v Speaker 3>We can put satellites in safe mode. We can d

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00:17:45.960 --> 00:17:49.559
<v Speaker 3>couple parts of the power grid to prevent a cascading failure.

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00:17:49.839 --> 00:17:52.000
<v Speaker 3>We can reroute flights away from the poles.

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00:17:52.119 --> 00:17:54.640
<v Speaker 2>It moves us from just reacting to disaster to actually

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00:17:54.720 --> 00:17:55.759
<v Speaker 2>forecasting it.

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00:17:55.759 --> 00:18:00.000
<v Speaker 3>It turns a potential disaster into a manageable event. Is

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00:18:00.119 --> 00:18:02.359
<v Speaker 3>the ultimate goal of all this space weather research.

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00:18:02.519 --> 00:18:04.960
<v Speaker 2>It is wild to think about the chain of events here.

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00:18:05.319 --> 00:18:08.559
<v Speaker 2>We started with a shadow a moon blocking the sun

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00:18:08.799 --> 00:18:12.920
<v Speaker 2>Step one. Then we saw the threads, then the prominence,

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00:18:12.960 --> 00:18:16.799
<v Speaker 2>the cold loop step two, then the clash, the temperature

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00:18:16.839 --> 00:18:17.920
<v Speaker 2>fight that creates.

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00:18:17.559 --> 00:18:19.839
<v Speaker 3>The smoke rings step three.

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00:18:20.000 --> 00:18:23.119
<v Speaker 2>Then the rings travel boosts the solar wind fly across

398
00:18:23.240 --> 00:18:25.759
<v Speaker 2>ninety three million miles of empty.

399
00:18:25.440 --> 00:18:27.480
<v Speaker 3>Space and potentially knock out your Wi Fi.

400
00:18:27.640 --> 00:18:30.599
<v Speaker 2>The butterfly effect, but with million degree.

401
00:18:30.359 --> 00:18:32.000
<v Speaker 3>Plasma, the plasma effect.

402
00:18:32.160 --> 00:18:35.119
<v Speaker 2>I like that. You know, this whole investigation has really

403
00:18:35.240 --> 00:18:37.240
<v Speaker 2>changed how I look at the Sun. I mean, usually

404
00:18:37.319 --> 00:18:38.960
<v Speaker 2>I just try not to get a sunburn. I don't

405
00:18:38.960 --> 00:18:40.480
<v Speaker 2>think about the machinery of it all.

406
00:18:40.640 --> 00:18:42.920
<v Speaker 3>It is humbling. I often think about the dual nature

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00:18:42.960 --> 00:18:46.200
<v Speaker 3>of the sun it is the giver of life. Without it,

408
00:18:46.319 --> 00:18:50.160
<v Speaker 3>we are just a frozen rock in the dark. Photosynthesis, warmth, rain,

409
00:18:50.559 --> 00:18:52.799
<v Speaker 3>it all comes from that energy. But at the same time,

410
00:18:52.960 --> 00:18:55.480
<v Speaker 3>it is a monster. It is a source of constant,

411
00:18:55.559 --> 00:18:58.720
<v Speaker 3>violent change. It is a nuclear bomb that literally never

412
00:18:58.759 --> 00:18:59.680
<v Speaker 3>stops exploding.

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00:19:00.039 --> 00:19:02.240
<v Speaker 2>And the eclipse is the only time we really get

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00:19:02.240 --> 00:19:03.119
<v Speaker 2>to peek under the hood.

415
00:19:03.200 --> 00:19:05.759
<v Speaker 3>It's the only time the glare stops long enough for

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00:19:05.839 --> 00:19:08.519
<v Speaker 3>us to see the gears turning, to see the vortex

417
00:19:08.599 --> 00:19:09.519
<v Speaker 3>ring spinning out.

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00:19:09.680 --> 00:19:11.519
<v Speaker 2>It reminds us that we are living next to a

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00:19:11.640 --> 00:19:14.240
<v Speaker 2>very active, very powerful neighbor.

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00:19:13.960 --> 00:19:17.160
<v Speaker 3>A neighbor that throws wild parties and occasionally tosses a

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00:19:17.200 --> 00:19:18.200
<v Speaker 3>smoke ring over the.

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00:19:18.160 --> 00:19:20.599
<v Speaker 2>Fence, and we just have to hope our windows don't break.

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00:19:20.680 --> 00:19:21.480
<v Speaker 3>Yeah, precisely.

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00:19:21.799 --> 00:19:24.640
<v Speaker 2>So here's the thought I want to leave you with, Listener,

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00:19:25.319 --> 00:19:28.599
<v Speaker 2>We are moving toward a time where solar eclipses are

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00:19:28.599 --> 00:19:31.240
<v Speaker 2>going to happen again. The next time you see a

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00:19:31.319 --> 00:19:34.519
<v Speaker 2>picture of one, maybe on your feed, or maybe you

428
00:19:34.559 --> 00:19:36.920
<v Speaker 2>are lucky enough to be in the path of totality.

429
00:19:37.799 --> 00:19:39.039
<v Speaker 2>Don't just look at the beauty.

430
00:19:39.279 --> 00:19:40.319
<v Speaker 3>Don't just look at the halo.

431
00:19:40.599 --> 00:19:43.759
<v Speaker 2>Yeah, don't just admire the diamond ring effect. Look closer,

432
00:19:43.880 --> 00:19:48.279
<v Speaker 2>look at the texture. Ask yourself, what invisible storms are

433
00:19:48.359 --> 00:19:51.799
<v Speaker 2>rolling off that edge right now? What magnetic vortexes are

434
00:19:51.880 --> 00:19:54.279
<v Speaker 2>spinning out into the dark, headed right toward us.

435
00:19:54.480 --> 00:19:56.960
<v Speaker 3>It is a beautiful view, but there is a massive

436
00:19:56.960 --> 00:19:58.920
<v Speaker 3>amount of physics happening in the dark.

437
00:19:59.079 --> 00:20:02.640
<v Speaker 2>It's not just a shadow, it's a laboratory, and thanks

438
00:20:02.640 --> 00:20:06.079
<v Speaker 2>to researchers like Shadia Habal, we are finally learning how

439
00:20:06.079 --> 00:20:06.799
<v Speaker 2>to read the data.

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00:20:06.960 --> 00:20:08.759
<v Speaker 3>Always more to learn out there, always.

441
00:20:08.839 --> 00:20:10.799
<v Speaker 2>Thanks for joining us on this trip to the edge

442
00:20:10.839 --> 00:20:11.240
<v Speaker 2>of the sun.

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00:20:11.519 --> 00:20:12.200
<v Speaker 3>It was a pleasure.

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00:20:12.359 --> 00:21:26.480
<v Speaker 2>We'll see you on the next investigation. Stay curious, characters,

445
00:21:30.519 --> 00:21:30.559
<v Speaker 2>U
