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>Welcome to the deep Dive. We're here to help you

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<v Speaker 2>get a handle on complex science and understand those invisible

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<v Speaker 2>forces really shaping our world.

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<v Speaker 3>And today we're tackling something vital.

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<v Speaker 2>Absolutely, we're diving into Earth's magnetic field, you know, our

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<v Speaker 2>planet's primary shield. It's fundamental, really, it's.

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<v Speaker 3>What makes life possible, blogging, harmful cosmic rays, charge particles

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<v Speaker 3>from the Sun, all that stuff exactly.

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<v Speaker 2>Without it, our tech in orbit and eventually well us,

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<v Speaker 2>we'd be in serious trouble.

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<v Speaker 3>And we've got some incredible data to dig into. We're

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<v Speaker 3>looking at what a eleven years of continuous, really precise measurements.

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<v Speaker 2>Right mostly from the European Space Agency's Swarm mission, those

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<v Speaker 2>satellites up there.

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<v Speaker 3>And our goal today is to go beyond just the headlines.

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<v Speaker 3>Want to unpack what this decade of data tells us

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<v Speaker 3>about the field strength, it's weaknesses which seem to be growing.

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<v Speaker 3>And you know what's driving these changes deep inside the Earth.

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<v Speaker 2>And we have to start with the big story here,

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<v Speaker 2>the one the data really flags, this huge expansion of

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<v Speaker 2>the weak spot over the South.

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<v Speaker 3>Atlantic South Atlantic Anomaly or SAA.

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<v Speaker 2>Yeah, the SAA, it's grown a lot, and the data

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<v Speaker 2>suggests the weakening is actually speeding up in some places.

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<v Speaker 3>It's not theoretical anymore. This is a measurable shift in

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<v Speaker 3>our planet's defenses happening right now.

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<v Speaker 2>So let's get into it. The swarm data shows this

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<v Speaker 2>SAA expansion and acceleration is kind of the dominant thing happening.

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<v Speaker 3>Right It's certainly a major focus, yes, but the field

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<v Speaker 3>is dynamic everywhere. Still, the ESAA changes are dramatic. We

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<v Speaker 3>need to look at the effects, sure, but also the

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<v Speaker 3>cause a down in the Earth's core.

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<v Speaker 2>Okay, let's start deep down then, like three thousand kilometers

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<v Speaker 2>beneath our feet. What's actually generating this field? Most people

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<v Speaker 2>picture like a simple bar magnet right.

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<v Speaker 3>Right, the textbook picture, but the reality is much messier,

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<v Speaker 3>more chaotic. Think heat, pressure, fluid.

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<v Speaker 2>Motion down in the outer core exactly.

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<v Speaker 3>Whatever the geodynamo, it's mostly generated by this vast ocean

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<v Speaker 3>of molten liquid irons swirling.

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<v Speaker 2>Around an ocean of liquid metal, a huge one, and

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<v Speaker 2>it's moving.

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<v Speaker 3>It's a conducting fluid, so as it flows, it generates

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<v Speaker 3>electrical currents. These currents in turn create the magnetic field like.

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<v Speaker 2>A giant dynamo, a generator sort of.

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<v Speaker 3>Yeah, that's the basic idea, like a bicycle dynamo, but

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<v Speaker 3>you know, on a planetary scale and way more turbulent.

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<v Speaker 3>It's less a neat machine and more like a huge,

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<v Speaker 3>self sustaining, very messy power plant.

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<v Speaker 2>So the movement creates current current creates the field that

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<v Speaker 2>reaches into space. But you mentioned complexity.

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<v Speaker 3>Why isn't it simple, Well, it's a turbulence. This liquid

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<v Speaker 3>iron is flowing smoothly. Earth's rotation stirs it up the

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<v Speaker 3>Coriolis effect. Plus there's heat rising from the innercore, driving

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<v Speaker 3>convection and even chemical.

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<v Speaker 2>Changes, so it's churning basically immensely.

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<v Speaker 3>It creates these huge swirling eddies and streams, not a

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<v Speaker 3>uniform flow at all, and that means the magnet field

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<v Speaker 3>it produces isn't smooth or symmetric. Either it's lumpy, it

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<v Speaker 3>changes direction locally. It's incredibly difficult to model accurately over time.

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<v Speaker 2>Which is why you need constant, really precise measurements exactly.

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<v Speaker 2>Which brings us to SWARM right, the tool that's giving

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<v Speaker 2>us these insights tell us about this mission. It's not

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<v Speaker 2>just one satellite, is it.

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<v Speaker 3>No, And that's key. SWARM is an EESA Earth Explorer

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<v Speaker 3>mission part of their future EO program. It's actually a

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<v Speaker 3>constellation of three identical satellites launched back in November twenty thirteen.

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<v Speaker 3>So over eleven years of data.

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<v Speaker 2>Now three identical ones. Why three wouldn't one super precise

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<v Speaker 2>satellite do the job?

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<v Speaker 3>Ah, good question. It's about separating the signals. One satellite

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<v Speaker 3>tells you the field strength right here, right now. But

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<v Speaker 3>Earth's magnetic field comes from multiple sources. Well, the main

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<v Speaker 3>one is the core, the dynamo we just talked about,

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<v Speaker 3>but there are also magnetic signals from the Earth's crust,

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<v Speaker 3>from the mantle, even from electrical currents in the oceans,

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<v Speaker 3>the ionosphere, the magnetosphere way out in space.

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<v Speaker 2>Wow, Okay, lots of layers contributing precisely.

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<v Speaker 3>And if you want to understand the core behavior the

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<v Speaker 3>source of the SAA problem. You need to filter out

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<v Speaker 3>all that other magnetic noise.

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<v Speaker 2>So how did the three satellites help with that?

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<v Speaker 3>They fly in a specific formation. Two fly close together

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<v Speaker 3>side by side at a lower altitude around four hundred

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<v Speaker 3>fifty kilometers up. The third one flies higher, and.

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<v Speaker 2>The altitude difference is the trick.

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<v Speaker 3>Yes, the lower pair can measure the finer details the

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<v Speaker 3>smaller scale magnetic structure is coming from the core and crust.

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<v Speaker 3>By comparing the readings from the lower pair with the

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<v Speaker 3>higher satellite taken at the same time, scientists can effectively

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<v Speaker 3>distinguish between the signals originating deep inside the Earth and

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<v Speaker 3>those coming from external sources like the ionosphere or solar

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<v Speaker 3>wind effects.

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<v Speaker 2>Okay, so it's like using triangulation almost to pinpoint the

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<v Speaker 2>source in a way.

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<v Speaker 3>Yes, it gives you that separation. It's like having multiple

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<v Speaker 3>microphones in a noisy room to isolate one specific voice.

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<v Speaker 3>Swarm isolates the voice of the Earth's core.

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<v Speaker 2>That level of detail is crucial then to figure out

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<v Speaker 2>why the field is weakening in the SAA or strengthening elsewhere.

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<v Speaker 2>You're mapping the entire magnetic finger press exactly.

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<v Speaker 3>Without this long term, high precision multipoint data, we just

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<v Speaker 3>be making educated guesses about what's happening three thousand kilometers down. Yeah,

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<v Speaker 3>SWARM gives us the hard evidence.

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<v Speaker 2>Okay, so let's use that evidence. Let's look at the

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<v Speaker 2>primary symptom everyone's talking about, the South Atlantic Anomaly. How

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<v Speaker 2>much has it actually changed since SWARM started watching.

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<v Speaker 3>Well, THEESSAA itself isn't new. Scientists first noticed this dip

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<v Speaker 3>and field strength southeast of South America way back in

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<v Speaker 3>the nineteenth century.

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<v Speaker 2>But it's become a much bigger issue now, right, especially

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<v Speaker 2>for satellites.

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<v Speaker 3>Definitely, and the SWARM data, particularly the analysis covering twenty

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<v Speaker 3>fourteen to twenty twenty five quantifies this change pretty starkly.

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<v Speaker 2>How big are we talking? Give us a sense of

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<v Speaker 2>the scale.

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<v Speaker 3>Since twenty fourteen, the total area defined as the SAA

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<v Speaker 3>the region of significant weakness, has expanded by an area

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<v Speaker 3>roughly half the size of continental Europe.

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<v Speaker 2>Half of Europe. That's huge, it is.

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<v Speaker 3>Imagine the magnetic shield over an area likes a Portugal, Spain,

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<v Speaker 3>France and Germany combined getting significantly weaker, all in just

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<v Speaker 3>over ten years. It's a major structural change.

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<v Speaker 2>That's a massive chunk of our planetary shield becoming less effective.

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<v Speaker 2>Is the weakening uniform across this new larger area, No,

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<v Speaker 2>it's not, And.

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<v Speaker 3>This is where swarm's precision really comes into play. While

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<v Speaker 3>the overall area grew steadily, the data pinpoint at a

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<v Speaker 3>specific zone southwest of Africa, in the Atlantic Ocean, where

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<v Speaker 3>the weakening has accelerated, especially since twenty twenty. The magnetic

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<v Speaker 3>field strength there is dropping even faster than in the

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<v Speaker 3>rest of the essay.

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<v Speaker 2>So it's not just strutting out. It's getting deeper, more

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<v Speaker 2>intense in certain.

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<v Speaker 3>Spots exactly, it's becoming more lopsided. Professor Chris Finlay, one

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<v Speaker 3>of the researchers, noted, the SAA is not just a

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<v Speaker 3>single block. The way it's behaving near Africa is different,

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<v Speaker 3>more intense than how it's behaving near South America.

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<v Speaker 2>That asymmetry must be a clue about the cause, right,

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<v Speaker 2>which we'll get to. But first the so what why

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<v Speaker 2>should someone listening care about a weak magnetic spot over

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<v Speaker 2>the ocean? How does it affect us?

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<v Speaker 3>The immediate impact is on technology in lower th orbit EOO.

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<v Speaker 3>That's where thousands of satellites operate for communications, whether GPS, Earth.

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<v Speaker 2>Observation, the workhourses of our space infrastructure.

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<v Speaker 3>Right, and the SAA is the place where the magnetic

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<v Speaker 3>field provides the least protection from incoming high energy particles

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<v Speaker 3>think protons, heavy ions blasted out by the Sun or

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<v Speaker 3>arriving as cosmic rays.

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<v Speaker 2>Because the shield is weakest there, these particles can get

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<v Speaker 2>closer to Earth, much.

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<v Speaker 3>Closer than anywhere else. It acts like a phenel. And

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<v Speaker 3>when the these high JV particles hit sensitive satellite electronics, well,

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<v Speaker 3>bad things can happen.

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<v Speaker 2>What kind of bad thing?

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<v Speaker 3>Two main types. First, there are single event upsets or SEUs,

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<v Speaker 3>A particle z app's a memory bit or a logic

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<v Speaker 3>gait causing a temporary.

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<v Speaker 2>Glitch like a computer crashing sort of.

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<v Speaker 3>You could be corrupt a data, a system reboot, a

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<v Speaker 3>temporary malfunction. Satellite operators actually planned for these scheduling reboots

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<v Speaker 3>sometimes when passing through the SAA.

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<v Speaker 2>Okay, annoying, but maybe manageable. What's the second type?

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<v Speaker 3>That's total dose effects. This is more serious. It's the

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<v Speaker 3>cumulative damage from radiation exposure. Over time, the particles physically

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<v Speaker 3>degrade the semiconductor materials.

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<v Speaker 2>Like sunburn for electronics, it.

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<v Speaker 3>Pretty good analogy. Yeah, it leads to permanent damage, components failing,

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<v Speaker 3>reduced performance, and eventually maybe the whole satellite just dies

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<v Speaker 3>a total blackout.

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<v Speaker 2>So every time a satellite flies through this expanding SAA,

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<v Speaker 2>it takes a radiation hit that shortens its life span.

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<v Speaker 3>Essentially, Yes, and they cross it hundreds even thousands of

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<v Speaker 3>times over their mission life. So operators have to take precautions.

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<v Speaker 2>Like putting the satellite into a safe mode.

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<v Speaker 3>Often, yes, they might shut down sensitive instruments, power down

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<v Speaker 3>non essential systems, or enter a protective standby mode just

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<v Speaker 3>for the SAA transit.

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<v Speaker 2>And if the SAA is now half the size of

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<v Speaker 2>Europe bigger, that means more downtime, less operational time for

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<v Speaker 2>these datag exactly.

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<v Speaker 3>It impacts efficiency, mission duration, and costs. The swarm data

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<v Speaker 3>is absolutely critical for updating the models used for mission planning,

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<v Speaker 3>for designing shielding, and for predicting when these protective measures

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<v Speaker 3>are needed.

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<v Speaker 2>Okay, that makes the risk very clear. So let's go

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<v Speaker 2>back underground. We see the symptom, the expanding, intensifying SAA.

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<v Speaker 2>What's the root cause? You mentioned the core mantle boundary.

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<v Speaker 3>Right, the boundary between the liquid outer core where the

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<v Speaker 3>field is generated and the rocky mantle above it. This interface,

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<v Speaker 3>the CMB is key. The specific mechanism driving the SAA

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<v Speaker 3>seems to be these things called reverse flux patches.

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<v Speaker 2>Reverse flux patches sounds intuitive, what are they okay?

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<v Speaker 3>Think about the normal field in the southern hemisphere, we

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<v Speaker 3>expect the magnetic field lines generated in the core to

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<v Speaker 3>point outwards.

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<v Speaker 2>From the Earth like arrows coming out of the South

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<v Speaker 2>Pole region.

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<v Speaker 3>Generally, yes, that's the configuration that gives us our shield.

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<v Speaker 3>But under the SAA, something different is happening in the

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<v Speaker 3>core fluid dynamics.

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<v Speaker 2>The turbulence again, yes, the.

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<v Speaker 3>Flow in certain localized spots is creating magnetic field lines

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<v Speaker 3>that point in the opposite direction. Instead of pointing out,

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<v Speaker 3>they point back into the core.

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<v Speaker 2>Whoa, so patches of reverse polarity deep inside the Earth.

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<v Speaker 3>That's essentially it. These reverse pointing field lines rise up

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<v Speaker 3>to the core mantle boundary. When they get there, they

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<v Speaker 3>meet the normal outward pointing field lines originating nearby, and

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<v Speaker 3>they cancel each other out effectively. Yes, they interact and

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<v Speaker 3>partially neutralize each other. This cancelation drastically weakens the total

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<v Speaker 3>magnetic field strength. Directly above that patch, and that weakened spot,

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<v Speaker 3>that leak in the shield is what we have at

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<v Speaker 3>the surface and in orbit as the South Atlantic anomaly.

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<v Speaker 2>So the core is basically fighting itself in these specific locations.

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<v Speaker 3>In a sense, yes, it's an internal cancelation process.

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<v Speaker 2>Which means if we can track where these reverse flux

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<v Speaker 2>patches are and where they're going, we.

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<v Speaker 3>Can understand and maybe even predict how the SAA will evolve.

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<v Speaker 3>And swarm Stata has been absolutely crucial for tracking the movement,

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<v Speaker 3>the dynamics of these patches.

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<v Speaker 2>And what has swarms shown about their movement.

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<v Speaker 3>The analysis confirms that the accelerated weakening we see southwest

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<v Speaker 3>of Africa is directly tied to the migration of one

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<v Speaker 3>of these patches. We can see a prominent reverse flux

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<v Speaker 3>patch moving westward underneath the African continent westward. Why westward,

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<v Speaker 3>It's consistent with a known phenomenon called the westerly drift

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<v Speaker 3>of the magnetic field. It suggests the overall large scale

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<v Speaker 3>rotation of the liquid outer core. This slow turbulent churning

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<v Speaker 3>carry these patches along with it.

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<v Speaker 2>So we're literally watching via swarm the deep Earth currents

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<v Speaker 2>shift and seeing the direct consequence and a growing hole

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<v Speaker 2>in our magnetic shield above Africa.

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<v Speaker 3>That's the picture emerging. Yes, we're observing dynamics three thousand

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<v Speaker 3>kilometers down manifesting is a clear and present danger to satellites.

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<v Speaker 2>How sure are scientists that this westward patch migration is

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<v Speaker 2>the main driver, especially for that intense spot near Africa?

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<v Speaker 2>Could other things be involved?

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<v Speaker 3>The link between the patches and the localized weakening, especially

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<v Speaker 3>the post twenty twenty acceleration near Africa, seems very strong

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<v Speaker 3>based on the data. These patches appear to be the

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<v Speaker 3>primary cause of where and how intensely the field is weakening, but.

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<v Speaker 2>Maybe not why the patch is formed there in the

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<v Speaker 2>first place.

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<v Speaker 3>Exactly what triggers the core flow to generate these reverse

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<v Speaker 3>patches in the specific region is still a big research question.

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<v Speaker 3>It might be related to how heat flows across the

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<v Speaker 3>core mantle boundary may be influenced by structures in the

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<v Speaker 3>deep mantle itself. Swarm shows us the what and where

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<v Speaker 3>the why is the next frontier for geodynamo modeling.

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<v Speaker 2>Okay, so the ESSAA is clearly a major focus, but

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<v Speaker 2>you mentioned the entire field is dynamic. Let's broaden the view.

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<v Speaker 2>What else did SWARM reveal about global changes?

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<v Speaker 3>This is crucial because focusing only on the SAA misses

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<v Speaker 3>half the story. The Earth's field is constantly changing shape

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<v Speaker 3>and strength globally, and it's definitely not symmetrical.

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<v Speaker 2>We talked about the simple bar magnet idea being wrong.

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<v Speaker 3>Right, It's much more complex. Non dipolar is the term

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<v Speaker 3>often used. We need satellites like SWARM to map this

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<v Speaker 3>intricate shifting structure properly.

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<v Speaker 2>So where are the strong points of the field the

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<v Speaker 2>opposite of the SAA globally?

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<v Speaker 3>The analysis shows two main areas of high intensity, both

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<v Speaker 3>in the northern hemisphere. There's one centered roughly over Canada

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<v Speaker 3>and another one over.

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<v Speaker 2>Siberia, the twin pillars of the Northern Shield, you could say.

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<v Speaker 3>A good way to put it. But Swarm's data over

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<v Speaker 3>the last decades shows these pillars are behaving very, very differently.

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<v Speaker 3>There's a major asymmetry developing.

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<v Speaker 2>Okay, how so well, the.

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<v Speaker 3>Magnetic field over Siberia has actually gotten stronger since SWARM

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<v Speaker 3>launched in twenty thirteen.

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<v Speaker 2>Consider stronger stronger while the SAA weakens.

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<v Speaker 3>Yes, And that Siberian strong region has physically grown in

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<v Speaker 3>surface area by about zero point four to two percent

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<v Speaker 3>of the entire Earth's surface.

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<v Speaker 2>Okay, point four to two percent. What does that translate

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<v Speaker 2>to in real terms?

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<v Speaker 3>It's an area comparable to the size of Greenland.

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<v Speaker 2>Wow, so Siberia's magnetic pillar has gained Greenland size territory.

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<v Speaker 2>What about the Canadian one.

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<v Speaker 3>It's doing the exact opposite. The strong field region over

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<v Speaker 3>Canada has weakened significantly and it is shrunken area by

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<v Speaker 3>about zero point six five percent of Earth's surface.

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<v Speaker 2>And point sixty five percent.

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<v Speaker 3>Is roughly the size of India.

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<v Speaker 2>Good grief. So let me get this straight. In the north,

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<v Speaker 2>the Siberian strong spot gains a Greenlands worth of area,

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<v Speaker 2>while the Canadian spot loses in India's worth.

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<v Speaker 3>That's the dynamic swarm has measured. We're seeing this massive

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<v Speaker 3>eastward shift, a transfer of magnetic dominance from Canada towards

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<v Speaker 3>Siberia in the northern hemisphere.

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<v Speaker 2>What are the implications of this, this magnetic tug of

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<v Speaker 2>war in the north combined with the SAA in the south.

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<v Speaker 3>The most immediate consequence relates to the position of the

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<v Speaker 3>magnetic north.

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00:15:08.320 --> 00:15:10.960
<v Speaker 2>Pole, right the point your compass needle actually points.

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<v Speaker 3>To exactly Because the Canadian field is weakening and the

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<v Speaker 3>Siberian one is strengthening. The magnetic North poles drift towards

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<v Speaker 3>Siberia has accelerated quite dramatically in recent years, and.

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<v Speaker 2>That matters for navigation, doesn't it hugely.

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<v Speaker 3>Think about the World Magnetic Model the WMM. It's the

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<v Speaker 3>standard map of Earth's magnetic field used by well practically everyone,

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<v Speaker 3>military navigation, aviation, maritime shipping, even the compass app on

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<v Speaker 3>your smartphone.

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00:15:37.440 --> 00:15:39.879
<v Speaker 2>They all rely on knowing where magnetic North is, and.

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<v Speaker 3>The WMM has to be updated regularly, typically every five years,

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<v Speaker 3>to account for the pole's natural drift. But the core

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00:15:46.919 --> 00:15:50.440
<v Speaker 3>dynamics this rapid shift driven by the Canada Siberia changes

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00:15:50.480 --> 00:15:54.240
<v Speaker 3>that swarm measured made the drift so fast and unpredictable that.

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<v Speaker 2>The five year updates weren't enough precisely.

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<v Speaker 3>For the first time ever, scientists had to issue an

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00:15:58.840 --> 00:16:02.080
<v Speaker 3>emergency out of sight update to the WMM in early

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00:16:02.159 --> 00:16:05.399
<v Speaker 3>twenty nineteen. The magnetic poll was moving away from the

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00:16:05.399 --> 00:16:06.919
<v Speaker 3>model faster than expected.

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00:16:07.159 --> 00:16:09.879
<v Speaker 2>An emergency update to the world's magnetic map that really

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00:16:09.879 --> 00:16:12.919
<v Speaker 2>brings home how dynamic this system is. The core is

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00:16:13.000 --> 00:16:15.320
<v Speaker 2>literally rewriting the map faster than we plan for.

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<v Speaker 3>It underscores why continuous monitoring with SWARM is so vital.

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<v Speaker 3>If our navigation models become outdated too quickly because the

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00:16:23.039 --> 00:16:28.360
<v Speaker 3>core is being well uncooperative, then accuracy degrades, especially at

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00:16:28.399 --> 00:16:32.480
<v Speaker 3>high latitudes where the field lines converge. This shifting balance

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00:16:32.519 --> 00:16:35.320
<v Speaker 3>is making the poles dand faster, and SWARM is keeping

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<v Speaker 3>our maps in sync with reality.

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<v Speaker 2>It's amazing how physics three thousand kilometers down directly impacts

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00:16:40.600 --> 00:16:43.440
<v Speaker 2>technology we use every single day. There really is so

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00:16:43.480 --> 00:16:45.919
<v Speaker 2>looking back. SWARM has been up there over eleven years now,

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00:16:46.360 --> 00:16:48.840
<v Speaker 2>that's quite a run. What's its legacy?

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00:16:49.279 --> 00:16:51.840
<v Speaker 3>I think the longevity and the sheer consistency of the

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00:16:51.919 --> 00:16:55.480
<v Speaker 3>data record are incredible. It's the longest continuous set of

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00:16:55.559 --> 00:16:58.519
<v Speaker 3>high precision magnetic field measurements we've ever had from space.

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<v Speaker 3>That alone is a mind mental achievement.

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00:17:00.960 --> 00:17:03.320
<v Speaker 2>It started as more of a tech demonstrator, right.

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00:17:03.159 --> 00:17:05.920
<v Speaker 3>It did, yeah, part of the Earth Explorer program designed

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00:17:05.920 --> 00:17:09.599
<v Speaker 3>to pioneer new observation techniques, but it's completely surpassed that

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00:17:09.640 --> 00:17:10.279
<v Speaker 3>original goal.

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00:17:10.400 --> 00:17:11.400
<v Speaker 2>It became foundational.

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<v Speaker 3>Absolutely. These Explorer missions often perform way beyond their design life,

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00:17:15.799 --> 00:17:19.200
<v Speaker 3>but SWARM has become indispensable. It feeds data into critical

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00:17:19.240 --> 00:17:21.160
<v Speaker 3>operational systems used worldwide.

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00:17:21.480 --> 00:17:25.519
<v Speaker 2>We talked about the navigation models. What other real world

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00:17:25.640 --> 00:17:28.119
<v Speaker 2>uses does the SWARM data have right now?

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00:17:28.440 --> 00:17:32.240
<v Speaker 3>Well beyond the magnetic models. It's crucial for understanding space.

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<v Speaker 2>Weather how the Sun affects us exactly.

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<v Speaker 3>By tracking how the solar wind, that stream of particles

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00:17:37.599 --> 00:17:41.759
<v Speaker 3>from the Sun interacts with and distorts our magnetosphere, SWARM

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00:17:42.000 --> 00:17:45.759
<v Speaker 3>helps improve forecasts for geomagnetic storms.

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<v Speaker 2>Which can affect power grids and things on Earth.

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00:17:48.440 --> 00:17:53.640
<v Speaker 3>Yes, power grids, pipelines, communications, satellite operations themselves. SWARM gives

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00:17:53.720 --> 00:17:56.720
<v Speaker 3>us this comprehensive view from the deep core, through the

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00:17:56.839 --> 00:17:59.759
<v Speaker 3>crust and mantle, the oceans, the atmosphere, all the way

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<v Speaker 3>out to space. It connects all these layers, and.

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<v Speaker 2>The satellites themselves are still going strong. What's the future

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00:18:05.240 --> 00:18:06.000
<v Speaker 2>hope for the mission?

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00:18:06.319 --> 00:18:09.799
<v Speaker 3>According to ESA's mission manager and just Strom, Yes, the

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<v Speaker 3>three satellites are remarkably healthy and still delivering excellent quality data.

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<v Speaker 3>That's great news, it is, and it fuels the big

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00:18:16.960 --> 00:18:20.680
<v Speaker 3>hope scientifically speaking, to extend the mission well beyond its

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<v Speaker 3>current timeline, ideally past twenty thirty.

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<v Speaker 2>Is there a specific reason for targeting past twenty thirty.

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00:18:25.839 --> 00:18:29.039
<v Speaker 3>Yes, it relates to the Sun's activity cycle. The Sun

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00:18:29.079 --> 00:18:32.839
<v Speaker 3>goes through roughly eleven year cycles of high and low activity.

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00:18:32.880 --> 00:18:36.319
<v Speaker 3>Extending swarm beyond twenty thirty would mean collecting data through

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<v Speaker 3>the next predicted solar minimum, a period when the Sun

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<v Speaker 3>is relatively quiet.

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<v Speaker 2>Less solar wind, less noise from external magnetic sources.

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<v Speaker 3>Exactly during solar maximum, the intense solar activity creates a

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<v Speaker 3>lot of magnetic disturbances in the ionosphere and magnetosphere. It's harder,

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00:18:53.039 --> 00:18:57.039
<v Speaker 3>though not impossible, to perfectly isolate the signal coming purely

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<v Speaker 3>from the Earth's core.

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00:18:58.720 --> 00:19:01.519
<v Speaker 2>So a solar minimum divides a cleaner window into the

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<v Speaker 2>core's behavior.

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00:19:02.759 --> 00:19:06.680
<v Speaker 3>Precisely. Collecting this ultra precise data during a solar quiet

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00:19:06.680 --> 00:19:09.839
<v Speaker 3>period would give scientists the clearest possible view of the

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00:19:09.880 --> 00:19:14.079
<v Speaker 3>internal geodynamal processes, the ones creating those reverse flex patches

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00:19:14.480 --> 00:19:17.799
<v Speaker 3>and driving the global field shifts with minimal interference from

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00:19:17.799 --> 00:19:18.079
<v Speaker 3>the Sun.

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00:19:18.200 --> 00:19:22.079
<v Speaker 2>Getting almost two full decades of continuous data would be unprecedented.

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00:19:22.119 --> 00:19:25.599
<v Speaker 3>Then it would be revolutionary for the field of geomagnetism.

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00:19:26.279 --> 00:19:28.359
<v Speaker 3>It would allow us to study these changes with the

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00:19:28.440 --> 00:19:31.400
<v Speaker 3>level of detail and over a time span that simply

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00:19:31.440 --> 00:19:34.559
<v Speaker 3>hasn't been possible before. We're really just starting to scratch

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00:19:34.599 --> 00:19:37.599
<v Speaker 3>the surface of understanding these deep earth dynamics.

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00:19:37.640 --> 00:19:40.440
<v Speaker 2>Okay, this has been fascinating. Let's try to quickly wrap

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00:19:40.559 --> 00:19:43.640
<v Speaker 2>up the key takeaways for everyone listening based on this

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00:19:43.839 --> 00:19:45.240
<v Speaker 2>amazing swarm data.

393
00:19:45.400 --> 00:19:49.240
<v Speaker 3>Right, So, the big ones are first the South Atlantic anomaly.

394
00:19:49.559 --> 00:19:52.839
<v Speaker 3>That weak spot is definitely expanding. It's grown by an

395
00:19:52.880 --> 00:19:55.720
<v Speaker 3>area about half the size of Europe since twenty fourteen.

396
00:19:55.480 --> 00:19:58.079
<v Speaker 2>Driven by those reverse flex patches deep in the core,

397
00:19:58.200 --> 00:19:59.960
<v Speaker 2>canceling out the field exactly.

398
00:20:00.160 --> 00:20:03.720
<v Speaker 3>And the weakening seems to be accelerating in a specific

399
00:20:03.799 --> 00:20:07.319
<v Speaker 3>zone southwest of Africa, linked to a westward moving patch.

400
00:20:07.839 --> 00:20:09.640
<v Speaker 3>This is a direct risk for satellites.

401
00:20:09.680 --> 00:20:12.000
<v Speaker 2>And second, it's not just the South. The North is

402
00:20:12.039 --> 00:20:14.559
<v Speaker 2>seeing a huge magnetic rebalancing act.

403
00:20:15.440 --> 00:20:18.640
<v Speaker 3>The strong field over Siberia has grown, gaining an area

404
00:20:18.720 --> 00:20:21.519
<v Speaker 3>like Greenland, while the one over Canada has shrunk, losing

405
00:20:21.559 --> 00:20:22.839
<v Speaker 3>an area like India.

406
00:20:22.519 --> 00:20:25.359
<v Speaker 2>Which is making the magnetic north pole race towards Siberia

407
00:20:25.400 --> 00:20:27.079
<v Speaker 2>and messing with navigation.

408
00:20:26.720 --> 00:20:31.160
<v Speaker 3>Models, forcing emergency updates. Even it really highlights the dynamism.

409
00:20:31.319 --> 00:20:33.400
<v Speaker 2>The core message seems to be that our shield is

410
00:20:33.440 --> 00:20:37.480
<v Speaker 2>constantly changing, driven by that chaotic churning iron deep below,

411
00:20:37.839 --> 00:20:40.440
<v Speaker 2>and we absolutely need satellites like SWARM to.

412
00:20:40.519 --> 00:20:44.759
<v Speaker 3>Keep watch, definitely and thinking bigger picture. The ongoing success

413
00:20:44.759 --> 00:20:48.839
<v Speaker 3>of SWARM, especially if it continues past twenty thirty, is crucial.

414
00:20:49.640 --> 00:20:52.119
<v Speaker 3>It leads to a really provocative thought for you, the listener.

415
00:20:52.559 --> 00:20:54.960
<v Speaker 3>If we do manage to get two full decades of

416
00:20:55.000 --> 00:20:59.079
<v Speaker 3>this continuous, high precision data stretching through a solar minimum,

417
00:21:00.000 --> 00:21:02.759
<v Speaker 3>what fundamental clues might we uncover about the really long

418
00:21:02.880 --> 00:21:06.119
<v Speaker 3>term behavior of the magnetic field. Could this data give

419
00:21:06.200 --> 00:21:09.079
<v Speaker 3>us insights into not just the current drift, but the

420
00:21:09.079 --> 00:21:13.920
<v Speaker 3>potential timing or mechanics of a future complete magnetic pole reversal.

421
00:21:14.039 --> 00:21:16.720
<v Speaker 2>Wow, Peering into the possibility of the poles flipping.

422
00:21:16.920 --> 00:21:19.400
<v Speaker 3>The longevity of this data set could fundamentally change our

423
00:21:19.480 --> 00:21:22.640
<v Speaker 3>understanding of Earth's deep processes and long term stability.

424
00:21:22.640 --> 00:21:26.079
<v Speaker 4>It's a big question, a very big question, indeed. Well,

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00:21:26.079 --> 00:21:29.240
<v Speaker 4>that's a perfect place to leave it for today. Thanks

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00:21:29.279 --> 00:21:31.920
<v Speaker 4>for joining us on this deep dive into our planet's invisible,

427
00:21:32.079 --> 00:21:35.559
<v Speaker 4>ever changing shield, Keep questioning, keep learning. We'll see you

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00:21:35.599 --> 00:22:01.200
<v Speaker 4>next time on the deep dives.

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00:22:20.119 --> 00:22:57.400
<v Speaker 3>Us Cho
