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. Today we are strapping in

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<v Speaker 2>for a pretty wild ride. We're exploring the most powerful

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<v Speaker 2>space weather event we've seen in more than two decades.

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<v Speaker 3>We really are. This was a true cosmic punch that

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<v Speaker 3>Earth took back in May of twenty twenty four, right, And.

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<v Speaker 2>It wasn't just spectacular to look at. I mean, the

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<v Speaker 2>photos were incredible, but it was scientifically just a gold.

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<v Speaker 3>Mine, a total gold mine. We're unpacking a whole stack

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<v Speaker 3>of sources today, all focused on what's called the Mother's

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<v Speaker 3>Day storm. It happened on May tenth and eleventh, and.

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<v Speaker 2>Space weather scientists have a name for it, right, Superstorm Gannon.

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<v Speaker 3>That's the one Superstorm Gannon. It was classified as a

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<v Speaker 3>G five storm, which is the absolute highest level of

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<v Speaker 3>geomagnetic activity you can have and the data gave us.

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<v Speaker 3>It's fundamentally shifting how we think about planetary defense.

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<v Speaker 2>I think we all saw the headlines, and maybe some

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<v Speaker 2>of you even saw the auroras, which were stunning. But

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<v Speaker 2>the real story, the one we're digging into, happened in

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<v Speaker 2>the invisible shields around our planet exactly.

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<v Speaker 3>Our mission today is to figure out why this storm,

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<v Speaker 3>the strongest in over twenty years, gave us a data

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<v Speaker 3>set we've just never had before.

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<v Speaker 2>It's not just about the storm's initial hit, is.

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<v Speaker 3>It, No, not at all. The core mystery here isn't

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<v Speaker 3>just the immediate violence of it, but the lingering aftermath.

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<v Speaker 3>For the first time, we have this incredibly detailed look

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<v Speaker 3>at how the superstorm assaulted Earth's protective.

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<v Speaker 2>Layers, specifically the plasmosphere.

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<v Speaker 3>The plasmosphere exactly. The initial compression was just brutal. We're

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<v Speaker 3>talking nine hours of intense pressure, but then the recovery

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<v Speaker 3>was so star rangely slow. It took four.

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<v Speaker 2>Days and four days of disruption. That means four days

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<v Speaker 2>where our satellites her infrastructure are vulnerable.

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<v Speaker 3>That's the risk.

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<v Speaker 2>So we're going to walk you through that timeline first.

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<v Speaker 2>How this huge protective layer got squeezed to about one

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<v Speaker 2>fifth its normal size. And then the really critical part,

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<v Speaker 2>how these invisible chemistry problems in the atmosphere, a thing

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<v Speaker 2>called a negative storm created this massive four day supply

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<v Speaker 2>chain problem that left our technology totally compromised.

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<v Speaker 3>It's a fascinating story of physics and chemistry on a

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<v Speaker 3>planetary scale.

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<v Speaker 2>Okay, so let's set the stage here, superstorm Gannon. When

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<v Speaker 2>we talk about a geomagnetic superstorm, we're really talking about

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<v Speaker 2>something at the extreme end of the scale. How rare

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<v Speaker 2>was an event like this?

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<v Speaker 3>I mean truly truly rare? Based on all the historical data,

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<v Speaker 3>A G five level storm which this was, happens on

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<v Speaker 3>average only about once every twenty to twenty five years.

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<v Speaker 2>Wow.

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<v Speaker 3>Yeah, we haven't seen anything this intent since the famous

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<v Speaker 3>Halloween storms back in two thousand and three.

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<v Speaker 2>And I remember those They took out a bunch of satellites, right.

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<v Speaker 3>They did, cause all sorts of problems. Yeah, So this

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<v Speaker 3>caannon EVET was in that same leak.

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<v Speaker 2>So that establishes the rarity. Now let's get into the cause.

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<v Speaker 2>What was it on the Sun that shot this this

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<v Speaker 2>once in a generation blast of energy right at us.

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<v Speaker 2>It's not just a solar flare, is it.

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<v Speaker 3>No, it's much much more than that. The storm was

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<v Speaker 3>triggered by a whole series of massive, powerful eruptions from

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<v Speaker 3>the Sun's atmosphere, and they were all timed very closely.

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<v Speaker 2>Together, eruptions of what exactly we.

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<v Speaker 3>Call them coronal mass ejections or CMEs. You have to

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<v Speaker 3>picture these colossal bursts of material. Basically, the Sun just

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<v Speaker 3>hurled billions of tons of highly charged magnetized plasma straight

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<v Speaker 3>towards Earth.

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<v Speaker 2>Okay, so what's the difference between a normal CME one

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<v Speaker 2>that just gives us some nice auroras up north and

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<v Speaker 2>this kind of monster that can compress our entire magnetic field?

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<v Speaker 1>Right?

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<v Speaker 3>It really comes down to a few key ingredients. First,

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<v Speaker 3>you need speed speed the CMEs that create again, and

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<v Speaker 3>we're moving incredibly fast, well over one thousand kilometers per second.

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<v Speaker 3>That speed creates this immense pressure when it hits our magnetosphere.

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<v Speaker 2>Okay, so speed is one second.

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<v Speaker 3>You need mass. It was billions of tons of this stuff,

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<v Speaker 3>which ensures it's not just a quick hit, it's a

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<v Speaker 3>sustained push.

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<v Speaker 2>But there's a third thing, right, the really critical factor

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<v Speaker 2>that turns a fast CME into a crushing storm. It's

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<v Speaker 2>about the magnetic field, isn't it.

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<v Speaker 3>Absolutely, It's all about the magnetic field orientation of that

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<v Speaker 3>incoming plasma cloud. We call it the Bled's component.

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<v Speaker 2>The Bledze component.

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<v Speaker 3>So the Sun has its own magnetic field and it's

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<v Speaker 3>embedded in this CME cloud. Now, if that cloud's magnetic

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<v Speaker 3>field lines are pointing north, they line up with Earth's

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<v Speaker 3>magnetic field, and things are, you know, relatively calm.

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<v Speaker 2>This sort of glands off each other.

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<v Speaker 3>More or less. But if the cloud's magnetic field, the

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<v Speaker 3>brass component, is pointing south, it directly opposes Earth's northward

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<v Speaker 3>pointing field lines.

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<v Speaker 2>And when those opposite fields meet, they don't just bounce.

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<v Speaker 3>No, that's when the fireworks happen. They undergo this violent

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<v Speaker 3>process called magnetic reconnection.

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<v Speaker 2>Which is like what a short circuit.

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<v Speaker 3>It's exactly like a short circuit, but on a planetary scale.

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<v Speaker 3>This reconnection just rips open the boundary of our magnetosphere.

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<v Speaker 3>It's like opening a door and letting a massive amount

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<v Speaker 3>of solar energy, momentum and charge particles poured directly into

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<v Speaker 3>our environment.

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<v Speaker 2>And the Gannon storm had that southward bruss.

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<v Speaker 3>It had a sustained, powerful southward pointing bruhs, and that's

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<v Speaker 3>what allowed for the maximum let's call it coupling between

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<v Speaker 3>the solar wind and our magnetosphere. It was the perfect storm.

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<v Speaker 2>So the store hits on May tenth, twenty twenty four,

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<v Speaker 2>and this intense magnetized plasma just slams into us, and

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<v Speaker 2>our protective layers react pretty much instantly.

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<v Speaker 3>Almost instantly. The major compression phase, the big squeeze only

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<v Speaker 3>lasted about nine hours.

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<v Speaker 2>Nine hours. That rapid energy transfer just tells you how

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<v Speaker 2>powerful that southward bruise must have been.

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<v Speaker 3>It really does. But before we get into the details

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<v Speaker 3>of the squeeze, we should probably define what exactly got squeeze.

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<v Speaker 3>We need to talk about the plasmosphere, right.

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<v Speaker 2>And for everyone listening, this isn't the same thing as

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<v Speaker 2>the magnetosphere itself, right, It's a structure inside of.

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<v Speaker 3>It, exactly. It's an infrastructure, but it's vital for our protection.

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<v Speaker 2>Okay, So let's break down the shield. What's the plasmosphere

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<v Speaker 2>made of and why do we care so much if

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<v Speaker 2>it gets damaged.

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<v Speaker 3>The plasmosphere is this dense, kind of doughnut shaped region

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<v Speaker 3>of pretty cold plasma, so low energy charged particles mostly hydrogen,

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<v Speaker 3>ions and electrons. It sits deep inside the magnetosphere and

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<v Speaker 3>it co rotates.

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<v Speaker 2>With the Earth, and its job is what a buffer.

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<v Speaker 3>A buffer is a perfect way to put it. It

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<v Speaker 3>stabilizes the electric and magnetic fields in that inner region,

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<v Speaker 3>and critically, it absorbs and sort of neutralizes a lot

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<v Speaker 3>of the less energetic particles that try to get into

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<v Speaker 3>our environment. It's a key part of our fielding.

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<v Speaker 2>So what happens to all our satellites that live in

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<v Speaker 2>or near that region If the plasmosphere is compromised.

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<v Speaker 3>Two bad things happen. First, the protective environment is just gone,

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<v Speaker 3>so satellites are exposed to much higher energy particle radiation

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<v Speaker 3>that normally gets filtered out. And the second thing, the

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<v Speaker 3>second is often more insidious. The outer boundary of the plasmosphere,

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<v Speaker 3>we call it the plasmo pause, is a region of instability.

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<v Speaker 3>When that gets compressed, it moves closer to all those

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<v Speaker 3>vital geosynchronous orbits.

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<v Speaker 2>Where our communications satellites are exactly and the extreme changes

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<v Speaker 2>in the electric fields there can cause something called satellite

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<v Speaker 2>surface charging.

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<v Speaker 3>It's like giving the satellite a dangerous static electricity jolt.

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<v Speaker 3>It can totally disrupt its electronics.

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<v Speaker 2>So Superstorm Gannon was basically a brutal real world stress

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<v Speaker 2>test for this entire.

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<v Speaker 3>Region, the ultimate stress test.

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<v Speaker 2>Okay, so let's unpack that stress test. We know the

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<v Speaker 2>plasmasphere is this vast charge bubble in its normal state.

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<v Speaker 2>Let's get into the specifics. What are the baseline measurements?

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<v Speaker 2>How big is it normally.

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<v Speaker 3>Under normal quiet conditions? It's huge. We define its outer boundary,

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<v Speaker 3>the plasmo pause, as the point where that plasma density

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<v Speaker 3>just drops off sharply.

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<v Speaker 2>And where is that?

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<v Speaker 3>Usually that boundary typically sits about forty four thousand kilometers

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<v Speaker 3>above the Earth surface.

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<v Speaker 2>Forty four thousand kilometers right.

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<v Speaker 3>It's about six point six earth RADII. It's a really

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<v Speaker 3>comfortable commence buffer zone.

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<v Speaker 2>And just for context, that forty four thousand kilometer baseline

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<v Speaker 2>is well beyond the orbits of our most crucial communication

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<v Speaker 2>satellites geosynchronous orbit is what around thirty six thousand kilometer.

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<v Speaker 3>That's right about thirty five thousand, seven hundred and eighty

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<v Speaker 3>six to be precise. So the plasma pause normally provides

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<v Speaker 3>this crucial protection around that whole geo belt of satellites,

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<v Speaker 3>But during Gannon that high speed southward magnetized CME just

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<v Speaker 3>crushed it, violently crushed it inward.

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<v Speaker 2>So how far inward are we talking? Give us the

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<v Speaker 2>numbers again, because they're just staggering.

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<v Speaker 3>The outer boundary was force fully compressed down to an

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<v Speaker 3>altitude of just nine thousand, six hundred kilometers above the

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<v Speaker 3>Earth's surface.

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<v Speaker 2>Nine thousand, six hundred that's it's.

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<v Speaker 3>An astonishingly low altitude. To put that in perspective, that's

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<v Speaker 3>barely above medium Earth Orbit MOO, which is where a

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<v Speaker 3>lot of our key GPS satellites operate.

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<v Speaker 2>So if I'm doing the math right, thelo asmosphere's radius

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<v Speaker 2>shrank by over seventy five percent. The whole protective layer

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<v Speaker 2>collapse to about one fifth of its normal.

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<v Speaker 3>Size, about a fifth of its volume.

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<v Speaker 2>Yes, in just nine hours. Does the data give us

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<v Speaker 2>any insight into the physics that drove that incredibly fast collapse.

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<v Speaker 3>It does. It's driven by something called the enhanced convection

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<v Speaker 3>electric field.

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<v Speaker 2>Okay, what's that.

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<v Speaker 3>It's generated by that magnetic reconnection we talked about. When

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<v Speaker 3>the southward BROS tears open the magnetosphere, it drives this

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<v Speaker 3>massive short circuit current across the polar caps and that

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<v Speaker 3>creates these incredibly powerful electric.

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<v Speaker 2>Fields, and those electric fields are what stripped the plasma

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<v Speaker 2>away exactly.

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<v Speaker 3>They act like a massive centrifuge. Plasma inside the magnetosphere

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<v Speaker 3>gets caught in this flow and is rapidly spun towards

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<v Speaker 3>the outer boundary where it just gets stripped away by

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<v Speaker 3>the solar winds.

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<v Speaker 2>So the boundary gets pushed dramatically.

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<v Speaker 3>Inward, dramatically it carves out that immense plasma layer and

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<v Speaker 3>just leaves this depleted inner region. The fact that it

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<v Speaker 3>happened in only nine hours, it just shows you the

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<v Speaker 3>incredible strength of those storm time electric fields.

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<v Speaker 2>And this isn't just a theory, right, this is a

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<v Speaker 2>measured physical reality. This is the big scientific achievement here,

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<v Speaker 2>moving from models to direct measurement.

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<v Speaker 3>That's the leap forward. Before Ganon, we had data from

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<v Speaker 3>smaller storms, sure, but getting continuous high res institute measurements

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<v Speaker 3>from inside the collapsing plasmosphere during a G five event

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<v Speaker 3>that was basically impossible.

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<v Speaker 2>The satellites were in the wrong place, or we didn't

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<v Speaker 2>have the right instrument precisely.

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<v Speaker 3>The Gannon event just provided this unprecedented level of detail.

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<v Speaker 2>And having that detail knowing exactly how that boundary moves

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<v Speaker 2>and how fast. That's absolutely critical for future planning, isn't it.

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<v Speaker 3>It's the difference between guessing and predicting. It really is

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<v Speaker 3>knowing a storm this intense can drive the plasma pause

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<v Speaker 3>down to nine thy six hundred kilometers right into key

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<v Speaker 3>operational orbits that lets engineers build better resilience into future satellites.

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<v Speaker 2>So it tells you how much radiation shielding you need

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<v Speaker 2>where you're likely to get these electrical surges exactly.

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<v Speaker 3>It moves space weather forecasting from a sort of qualitative hey,

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<v Speaker 3>a storm is coming, to a quantitative risk assessment tool.

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<v Speaker 3>The risk at this orbit will be x for y

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<v Speaker 3>number of hours. That's the goal.

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<v Speaker 2>The success of this study really seems to hinge on

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<v Speaker 2>just being in the right place at the right time,

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<v Speaker 2>hitting a scientific lottery almost.

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<v Speaker 3>That's a good way to put it. A twenty year

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<v Speaker 3>storm hits right when you have the perfect instruments in

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<v Speaker 3>the perfect position.

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<v Speaker 2>So let's talk about the key instrument here, the Erase satellite.

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<v Speaker 3>The Erase satellite was the hero of this whole observation.

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<v Speaker 3>It's a JAXA mission launched back in twenty sixteen.

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<v Speaker 2>JAXA is the Japanese space agency right.

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<v Speaker 3>And its name ERASE actually means rough C or stormy C.

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<v Speaker 3>How fitting, incredibly fitting. Its whole mission is specialized. It

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<v Speaker 3>flies in this elliptical orbit that dips low through the

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<v Speaker 3>inner magnetosphere and then swings way out through the heart

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<v Speaker 3>of the plasmosphere. It's designed specifically to study how this

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<v Speaker 3>region responds to storms.

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<v Speaker 2>So what instruments on a Race actually confirmed that the

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<v Speaker 2>boundary collapsed from forty four thousand kilometers down to nine thousand,

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<v Speaker 2>six hundred.

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<v Speaker 3>The most critical data came from its suite of plasma

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<v Speaker 3>and wave instruments, specifically the Plasma Wave Experiment and the

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<v Speaker 3>soft Electron and ion spectrometer.

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<v Speaker 2>And what do those do?

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<v Speaker 3>They're designed to measure the density, the temperature, and the

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<v Speaker 3>composition of the plasma in real time. So as that

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<v Speaker 3>plasma pause swept past a Rase's orbit, the satellite recorded

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<v Speaker 3>this abrupt several orders of magnitude drop in the cold

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<v Speaker 3>plasma density.

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<v Speaker 2>So it flew right through the boundary.

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<v Speaker 3>It flew right through it and measured the cliff edge

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<v Speaker 3>drop that confirmed the boundary had retreated sharply to an

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<v Speaker 3>altitude below its position.

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<v Speaker 2>So a rice gave us the direct in place evidence

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<v Speaker 2>of the shield collapsing. But the team at Nagoya University,

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<v Speaker 2>led by doctor at Suki Shinbori, they did more than that.

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<v Speaker 2>They synchronized the satellite data with ground based measurements.

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<v Speaker 3>Yes, and that dual approach is what made this study

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<v Speaker 3>so powerful, especially when it came to understanding the recovery

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<v Speaker 3>how so well. They used a RAISE to track the plasmosphere,

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<v Speaker 3>but at the same time they were monitoring the ionosphere

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<v Speaker 3>that's the layer below the plasmosphere, using a huge network

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<v Speaker 3>of ground based GPS receivers.

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<v Speaker 2>How can you use GPS to monitor the ionosphere?

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<v Speaker 3>It's actually a really clever method. We can figure out

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<v Speaker 3>the state of the ionosphere by measuring something called the

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<v Speaker 3>total electron content.

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<v Speaker 2>Or tech total electron content.

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<v Speaker 3>Right, GPS signals have to travel through the ionosphere to

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<v Speaker 3>get to a receiver on the ground. The free electrons

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<v Speaker 3>in the ionosphere cause a tiny but measurable delay in

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<v Speaker 3>that signal's travel time.

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<v Speaker 2>So you measure the delay and that tells you how

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<v Speaker 2>many electrons are up there exactly.

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<v Speaker 3>Using very precise dual frequency GPS receivers, scientists can calculate

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<v Speaker 3>that time delay and from that they can quantify the tech.

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<v Speaker 3>So if the ionosphere is full of electrons and ions,

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<v Speaker 3>the delay is high. If it's depleted, the delay is low.

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<v Speaker 2>And that's the key link here. The ionosphere is the

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<v Speaker 2>supply chain.

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<v Speaker 3>It's the supply chain. It's where the charged particles that

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00:14:01.039 --> 00:14:04.600
<v Speaker 3>are needed to refill the plasmosphere, those hydrogen ions are

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00:14:04.639 --> 00:14:06.559
<v Speaker 3>generated and stream upwards.

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<v Speaker 2>So if your GPS data shows that the tech is

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00:14:09.039 --> 00:14:10.600
<v Speaker 2>dropping everywhere.

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00:14:10.279 --> 00:14:13.919
<v Speaker 3>It means your source material for refilling the plasmosphere is compromised.

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00:14:14.279 --> 00:14:18.559
<v Speaker 3>And the Nagoya team perfectly synchronized the erase density measurements

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00:14:18.559 --> 00:14:22.399
<v Speaker 3>from space with the ground based tech measurements. They proved

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00:14:22.399 --> 00:14:24.919
<v Speaker 3>that the long recovery delay up in space was directly

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<v Speaker 3>caused by this massive drop in the particles supplied from below.

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00:14:27.879 --> 00:14:31.600
<v Speaker 2>That's incredible, connecting a satellite flying thousands of kilometers up

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00:14:31.600 --> 00:14:34.080
<v Speaker 2>with a receiver on the ground, all through a tiny

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00:14:34.159 --> 00:14:37.960
<v Speaker 2>signal delay. It shows just how complex space weather observation

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00:14:38.039 --> 00:14:38.519
<v Speaker 2>has become.

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00:14:38.679 --> 00:14:41.720
<v Speaker 3>It really does. It's not about isolated observations anymore. It's

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00:14:41.720 --> 00:14:43.759
<v Speaker 3>about a unified system wide.

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00:14:43.559 --> 00:14:47.159
<v Speaker 2>Analysis, and that brings us right to the central mystery

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00:14:47.279 --> 00:14:52.559
<v Speaker 2>of the Gannon storm. The nine hour compression violent but

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00:14:52.639 --> 00:14:55.799
<v Speaker 2>sort of expected for a storm this big. What wasn't

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00:14:55.840 --> 00:14:59.919
<v Speaker 2>expected was how sluggish the recovery was. The shield broke fast,

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<v Speaker 2>but the repair job took forever. What's the normal recovery time?

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<v Speaker 3>Historically for a moderate or even a strong storm, the

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00:15:08.279 --> 00:15:11.639
<v Speaker 3>plasma sphere starts to refill pretty quickly. It usually gets

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<v Speaker 3>back to pre storm density levels within say.

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00:15:14.279 --> 00:15:16.399
<v Speaker 2>A day or two, so twenty four to forty eight

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00:15:16.440 --> 00:15:17.240
<v Speaker 2>hours about that.

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00:15:17.320 --> 00:15:21.120
<v Speaker 3>Yeah, The magnetic field bounces back, the electric field weakens,

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00:15:21.159 --> 00:15:23.919
<v Speaker 3>and the natural flow of plasma from the ionosphere starts

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00:15:23.919 --> 00:15:25.919
<v Speaker 3>replenishing those depleted regions.

320
00:15:26.000 --> 00:15:29.000
<v Speaker 2>But with Gannon, that process stretched over four full days.

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00:15:29.039 --> 00:15:32.120
<v Speaker 3>Four days, which is at least double the typical recovery time.

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00:15:32.320 --> 00:15:34.919
<v Speaker 3>It's the longest sustained depletion that a RaSE has observed

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00:15:34.919 --> 00:15:36.799
<v Speaker 3>since its mission began in twenty seventeen.

324
00:15:37.000 --> 00:15:39.639
<v Speaker 2>So why why did the supply changes dry up for

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00:15:39.679 --> 00:15:40.159
<v Speaker 2>so long?

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00:15:40.320 --> 00:15:42.279
<v Speaker 3>This is where the physics of the compression gives way

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00:15:42.320 --> 00:15:46.080
<v Speaker 3>to the invisible but incredibly powerful chemistry of the upper atmosphere.

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00:15:46.159 --> 00:15:47.840
<v Speaker 2>Chemistry not physics, right.

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00:15:48.240 --> 00:15:51.399
<v Speaker 3>The critical mechanism delaying everything is a phenomenon. We call

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<v Speaker 3>the negative storm.

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00:15:52.440 --> 00:15:56.080
<v Speaker 2>Okay, a negative storm, let's define that because it sounds

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00:15:56.080 --> 00:15:58.720
<v Speaker 2>like a particle drought. But you're saying it's caused by

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00:15:58.720 --> 00:16:00.759
<v Speaker 2>the storm's energy, not a lack of it.

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00:16:01.279 --> 00:16:04.600
<v Speaker 3>That's the paradox of it. The superstorm injects an immense

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00:16:04.639 --> 00:16:08.080
<v Speaker 3>amount of energy into the polar regions. That energy is

336
00:16:08.120 --> 00:16:12.200
<v Speaker 3>mostly from accelerated particles and strong electric currents. It intensely

337
00:16:12.279 --> 00:16:16.320
<v Speaker 3>heats the upper layer of the atmosphere, the thermosphere. That

338
00:16:16.440 --> 00:16:17.799
<v Speaker 3>heating is the trigger.

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00:16:17.919 --> 00:16:21.679
<v Speaker 2>How does heating the atmosphere cause a drought of charged particles?

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00:16:21.679 --> 00:16:23.120
<v Speaker 2>It feels counterintuitive.

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00:16:23.279 --> 00:16:27.200
<v Speaker 3>It does. The heating fundamentally changes the atmosphere composition. It's

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00:16:27.200 --> 00:16:31.279
<v Speaker 3>a process called upwelling. Normally, the ionosphere is dominated by

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00:16:31.399 --> 00:16:34.759
<v Speaker 3>lighter atoms like atomic oxygen and hydrogen, but the intense

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00:16:34.799 --> 00:16:38.320
<v Speaker 3>heating near the poles causes that neutral atmosphere to expand

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00:16:38.399 --> 00:16:41.679
<v Speaker 3>and rise, and as it rises, it drags up heavier

346
00:16:41.679 --> 00:16:45.600
<v Speaker 3>molecular gases from lower altitudes, mostly molecular nitrogen end to

347
00:16:45.879 --> 00:16:47.440
<v Speaker 3>and molecular oxygen O two.

348
00:16:47.679 --> 00:16:51.000
<v Speaker 2>So the storm basically pumps heavy gas molecules up into

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00:16:51.000 --> 00:16:53.559
<v Speaker 2>a region where they don't normally belong exactly.

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00:16:53.600 --> 00:16:57.519
<v Speaker 3>It completely changes the chemical balance, and these heavier molecules

351
00:16:57.759 --> 00:17:02.120
<v Speaker 3>into and OH two the incredibly effective at capturing free electrons.

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00:17:02.200 --> 00:17:04.359
<v Speaker 3>It's a process called recombination.

353
00:17:04.119 --> 00:17:06.160
<v Speaker 2>So they basically mop up all the free charges.

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00:17:06.359 --> 00:17:09.640
<v Speaker 3>They act like a massive chemical drain. The rate at

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00:17:09.680 --> 00:17:15.200
<v Speaker 3>which free electrons recombine with positive ions just accelerates dramatically,

356
00:17:15.559 --> 00:17:17.759
<v Speaker 3>so all the electrons and positive ions that should be

357
00:17:17.839 --> 00:17:21.920
<v Speaker 3>available to stream up and refill the plasmisphere you're just

358
00:17:22.119 --> 00:17:25.400
<v Speaker 3>rapidly getting neutralized back into plain old gas molecules.

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00:17:25.559 --> 00:17:27.759
<v Speaker 2>So, just to be clear, if the storm had only

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00:17:27.799 --> 00:17:30.559
<v Speaker 2>compressed the magnetic field, the recovery would have been pretty quick.

361
00:17:30.720 --> 00:17:33.400
<v Speaker 2>It would have been but because the storm also caused

362
00:17:33.440 --> 00:17:36.920
<v Speaker 2>this chemical shift, this upwelling of heavy gas, it broke

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00:17:37.000 --> 00:17:38.319
<v Speaker 2>the particle production line.

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00:17:38.359 --> 00:17:40.960
<v Speaker 3>It broke the supply chain by destroying the raw materials.

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00:17:41.359 --> 00:17:44.559
<v Speaker 3>The key raw material for refilling the plasmosphere is the

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00:17:44.599 --> 00:17:48.640
<v Speaker 3>atomic oxygen ion O plus, and oplus reacts with hydrogen

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00:17:48.720 --> 00:17:51.519
<v Speaker 3>to produce the lighter hydrogen ions H plus meat that

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00:17:51.720 --> 00:17:55.039
<v Speaker 3>stream upward. But when the ionospheres is suddenly flooded with

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00:17:55.200 --> 00:17:58.119
<v Speaker 3>N two and O two, the oplus ions just rapidly

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00:17:58.160 --> 00:18:00.720
<v Speaker 3>recombined with them. Instead, it stops the from producing the

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00:18:00.839 --> 00:18:02.039
<v Speaker 3>hplus needed for the refill.

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00:18:02.160 --> 00:18:04.559
<v Speaker 2>And this negative storm effect, it wasn't just at the polls,

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00:18:04.680 --> 00:18:04.920
<v Speaker 2>was it.

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00:18:04.920 --> 00:18:08.480
<v Speaker 3>It spread, It spread globally. The data shows that the

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00:18:08.559 --> 00:18:12.119
<v Speaker 3>changes in atmospheric circulation driven by that intense polar heating

376
00:18:12.599 --> 00:18:16.680
<v Speaker 3>rapidly transported this chemically altered air mass across vast areas

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00:18:17.039 --> 00:18:17.839
<v Speaker 3>down towards the.

378
00:18:17.799 --> 00:18:20.720
<v Speaker 2>Equator, which is why the GPS network saw that tech

379
00:18:20.920 --> 00:18:22.160
<v Speaker 2>drop everywhere.

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00:18:22.200 --> 00:18:26.920
<v Speaker 3>Precisely. That widespread depletion ensured that the plasmosphere's refill mechanism

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00:18:27.000 --> 00:18:31.079
<v Speaker 3>was compromised, not just locally, but globally for four straight days.

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00:18:31.160 --> 00:18:33.920
<v Speaker 2>And this link. This is the big takeaway, isn't it.

383
00:18:33.960 --> 00:18:38.160
<v Speaker 2>Had we ever empirically documented this exact sequence before the heating,

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00:18:38.240 --> 00:18:42.039
<v Speaker 2>the upwelling, the recombination leading to a four day depletion.

385
00:18:41.960 --> 00:18:44.559
<v Speaker 3>We had theoretical models that suggested this could happen, but

386
00:18:44.599 --> 00:18:48.960
<v Speaker 3>the Gannin storm provided the definitive, continuous, multilayer.

387
00:18:48.400 --> 00:18:49.720
<v Speaker 2>Proof, the smoking gun.

388
00:18:49.880 --> 00:18:53.039
<v Speaker 3>The smoking gun, the simultaneous data from a race in

389
00:18:53.119 --> 00:18:57.519
<v Speaker 3>space and the GPS network on the ground offered irrefutable proof.

390
00:18:58.160 --> 00:19:02.079
<v Speaker 3>It's the negative storm's chemical can over the system's recovery speed.

391
00:19:02.519 --> 00:19:05.720
<v Speaker 3>And this is a huge realization for space weather forecasting.

392
00:19:05.920 --> 00:19:09.640
<v Speaker 3>Why because means the threat level stays high long after

393
00:19:09.680 --> 00:19:12.920
<v Speaker 3>the initial solar shock has passed. The true duration of

394
00:19:13.000 --> 00:19:17.160
<v Speaker 3>risk is dictated by upper atmosphere chemistry, not just plasma physics.

395
00:19:17.279 --> 00:19:20.000
<v Speaker 2>Okay, so let's shift from that invisible chemistry to the

396
00:19:20.480 --> 00:19:24.079
<v Speaker 2>visible drama and the real world damage. The compression of

397
00:19:24.119 --> 00:19:26.960
<v Speaker 2>the shield was so extreme that millions of people got

398
00:19:26.960 --> 00:19:31.279
<v Speaker 2>this breath taking spectacle auroras way outside their normal homes.

399
00:19:31.519 --> 00:19:34.519
<v Speaker 3>That was the most obvious sign of this form's intensity. Normally,

400
00:19:34.599 --> 00:19:37.000
<v Speaker 3>you know, auroras are confined to these narrow bands around

401
00:19:37.039 --> 00:19:40.319
<v Speaker 3>the magnetic poles, usually above sixty degrees latitude, the auroral

402
00:19:40.359 --> 00:19:44.599
<v Speaker 3>ovals exactly. That's because the magnetic field funnels the incoming

403
00:19:44.680 --> 00:19:48.119
<v Speaker 3>charged particles into the atmosphere at those specific points.

404
00:19:48.279 --> 00:19:51.200
<v Speaker 2>But during Gannon, the field was so compressed that it

405
00:19:51.240 --> 00:19:54.000
<v Speaker 2>allowed those particles to get in much deeper, much closer

406
00:19:54.000 --> 00:19:54.680
<v Speaker 2>to the equator.

407
00:19:54.920 --> 00:19:57.400
<v Speaker 3>That's right, When the field is squashed down to nine

408
00:19:57.880 --> 00:20:01.519
<v Speaker 3>six hundred kilometers, the field lines get warped and stretched,

409
00:20:01.920 --> 00:20:04.799
<v Speaker 3>and it effectively widens the area where particles can rain

410
00:20:04.920 --> 00:20:06.759
<v Speaker 3>down into the atmosphere.

411
00:20:06.119 --> 00:20:09.200
<v Speaker 2>And that led to photos of auroras in places like.

412
00:20:09.200 --> 00:20:12.960
<v Speaker 3>We saw reports and incredible photos from places like Rikubetsu

413
00:20:13.000 --> 00:20:16.559
<v Speaker 3>in Japan, which is mid latitude, even as far south

414
00:20:16.599 --> 00:20:18.319
<v Speaker 3>as Mexico and across southern.

415
00:20:18.119 --> 00:20:19.759
<v Speaker 2>Europe, which is just unheard of.

416
00:20:20.000 --> 00:20:22.880
<v Speaker 3>It's a clear historical marker when you see red and

417
00:20:22.920 --> 00:20:26.000
<v Speaker 3>green aurora displays from those regions, it tells you one thing.

418
00:20:26.319 --> 00:20:29.359
<v Speaker 3>The farther the aurora travels from the poles, the stronger

419
00:20:29.400 --> 00:20:30.680
<v Speaker 3>the geomagnetic storm was.

420
00:20:30.759 --> 00:20:33.559
<v Speaker 2>Okay, so that's a beautiful visible side. Now let's talk

421
00:20:33.559 --> 00:20:38.079
<v Speaker 2>about the ugly invisible technological impact that lasted for that

422
00:20:38.160 --> 00:20:39.680
<v Speaker 2>whole four day recovery.

423
00:20:39.960 --> 00:20:43.039
<v Speaker 3>Right when the plasmasphere is gone and the ionosphere is

424
00:20:43.119 --> 00:20:46.640
<v Speaker 3>chemically compromised, our technology is put under serious stress.

425
00:20:47.000 --> 00:20:49.079
<v Speaker 2>Let's start with satellites. What happened to them?

426
00:20:49.119 --> 00:20:52.000
<v Speaker 3>The stress was widespread. Satellites in low and medium Earth

427
00:20:52.079 --> 00:20:56.440
<v Speaker 3>orbit experienced significant electrical issues. When that shield collapses, the

428
00:20:56.480 --> 00:20:58.440
<v Speaker 3>flux of high energy particles.

429
00:20:58.000 --> 00:21:00.079
<v Speaker 2>Just shoots up and that causes it leads to.

430
00:21:00.000 --> 00:21:03.559
<v Speaker 3>The surface charging and internal charging of satellite components. This

431
00:21:03.640 --> 00:21:07.480
<v Speaker 3>can cause electrical glitches, system resets, and in some severe

432
00:21:07.519 --> 00:21:12.359
<v Speaker 3>cases reported during gannon satellites just temporarily stop transmitting data altogether.

433
00:21:12.480 --> 00:21:15.200
<v Speaker 2>And that heating of the thermosphere we talked about that

434
00:21:15.240 --> 00:21:16.960
<v Speaker 2>has a physical effect too, right.

435
00:21:16.920 --> 00:21:20.200
<v Speaker 3>It absolutely does. When the thermosphere heats up, it expands,

436
00:21:20.599 --> 00:21:24.440
<v Speaker 3>which increases the atmospheric density at those low orbit altitudes,

437
00:21:24.519 --> 00:21:28.160
<v Speaker 3>which means more drags, significantly more atmospheric drag. For these

438
00:21:28.240 --> 00:21:31.920
<v Speaker 3>huge satellite constellations, that drag forces them to burn more

439
00:21:31.960 --> 00:21:35.279
<v Speaker 3>fuel to stay in orbit, which shortens their lifespan. It

440
00:21:35.319 --> 00:21:37.720
<v Speaker 3>also makes collision avoidants much more complicated.

441
00:21:37.960 --> 00:21:42.279
<v Speaker 2>Now, let's talk about the service we all rely on constantly, GPS.

442
00:21:43.359 --> 00:21:46.480
<v Speaker 2>People talk about GPS disruption, but what was the specific

443
00:21:46.759 --> 00:21:51.200
<v Speaker 2>measurable effect of that four day negative storm on navigation accuracy?

444
00:21:51.359 --> 00:21:54.839
<v Speaker 3>The impact was very real and measurable. GPS and other

445
00:21:54.960 --> 00:21:59.000
<v Speaker 3>navigation systems they rely on incredibly precise timing to calculate

446
00:21:59.039 --> 00:22:01.440
<v Speaker 3>your location, and that timing has to be corrected for

447
00:22:01.480 --> 00:22:04.200
<v Speaker 3>the signal delay caused by the total electron content in

448
00:22:04.240 --> 00:22:05.160
<v Speaker 3>the ionosphere.

449
00:22:05.359 --> 00:22:09.279
<v Speaker 2>So if the tech suddenly plummets during a negative storm,

450
00:22:09.759 --> 00:22:13.440
<v Speaker 2>the standard models that the GPS system uses to calculate

451
00:22:13.480 --> 00:22:16.400
<v Speaker 2>that delay, they become totally wrong.

452
00:22:16.599 --> 00:22:19.839
<v Speaker 3>Wildly inaccurate during the gannin storm and for days after,

453
00:22:19.960 --> 00:22:23.920
<v Speaker 3>the models, which are designed for normal conditions, were overestimating

454
00:22:23.960 --> 00:22:27.000
<v Speaker 3>the correction needed because the ononosphere was so depleted.

455
00:22:26.680 --> 00:22:28.400
<v Speaker 2>And that caused ranging errors.

456
00:22:28.240 --> 00:22:30.960
<v Speaker 3>Significant ranging errors. For your phone, maybe it means a

457
00:22:30.960 --> 00:22:34.839
<v Speaker 3>little inaccuracy you miss a turn, but for high precision applications,

458
00:22:34.839 --> 00:22:40.440
<v Speaker 3>commercial aviation, autonomous tractors, and farming, which need centimeter level accuracy,

459
00:22:41.039 --> 00:22:46.160
<v Speaker 3>that error margin just ballooned to completely unacceptable levels.

460
00:22:46.240 --> 00:22:49.000
<v Speaker 2>And this degradation was measured across the planet for the

461
00:22:49.039 --> 00:22:50.279
<v Speaker 2>full four days.

462
00:22:50.039 --> 00:22:51.640
<v Speaker 3>For the entire duration of the negative storm.

463
00:22:51.680 --> 00:22:54.440
<v Speaker 2>Yes, and what about radio, Things like high frequency radio

464
00:22:54.599 --> 00:22:57.400
<v Speaker 2>use for long distance communication also broadly affected.

465
00:22:57.519 --> 00:23:00.480
<v Speaker 3>The ionosphere is what reflects HF radio waves back to Earth,

466
00:23:00.599 --> 00:23:03.559
<v Speaker 3>allowing you to communicate over the horizon. When the chemical

467
00:23:03.640 --> 00:23:07.160
<v Speaker 3>balance is disrupted and the particle density changes so dramatically

468
00:23:07.440 --> 00:23:11.039
<v Speaker 3>the reflective properties of the ionosphere change, you get blackouts,

469
00:23:11.200 --> 00:23:16.119
<v Speaker 3>you get signal fading dropouts, temporary blackouts across key frequency bands.

470
00:23:16.480 --> 00:23:20.200
<v Speaker 3>And because the recovery was so slow, these communication issues

471
00:23:20.359 --> 00:23:24.000
<v Speaker 3>were persistent and really hard to mitigate for four days.

472
00:23:23.839 --> 00:23:26.720
<v Speaker 2>Which brings us back to the real importance of these findings.

473
00:23:27.319 --> 00:23:30.160
<v Speaker 2>Knowing that your technological environment is going to be hostile

474
00:23:30.200 --> 00:23:34.160
<v Speaker 2>for four plus days after a major strike, that's crucial information.

475
00:23:34.319 --> 00:23:37.839
<v Speaker 3>It completely transforms risk assessment. Before this, we might have

476
00:23:37.960 --> 00:23:41.160
<v Speaker 3>estimated the risk period to be forty eight hours. Now

477
00:23:41.200 --> 00:23:44.000
<v Speaker 3>we have empirical evidence that for a G five event,

478
00:23:44.279 --> 00:23:48.599
<v Speaker 3>the chemical fallout prolongs that vulnerability period to at least

479
00:23:48.680 --> 00:23:49.599
<v Speaker 3>ninety six hours.

480
00:23:49.880 --> 00:23:53.079
<v Speaker 2>So satellite operators need to have contingency plans that last

481
00:23:53.480 --> 00:23:54.640
<v Speaker 2>much longer.

482
00:23:54.480 --> 00:23:56.559
<v Speaker 3>Much longer. It means they need to be prepared for

483
00:23:56.599 --> 00:23:59.720
<v Speaker 3>a longer period of risk, maybe initiate protective maneuvers for

484
00:23:59.799 --> 00:24:02.880
<v Speaker 3>laws longer than they previously thought necessary. This new clarity

485
00:24:02.880 --> 00:24:05.960
<v Speaker 3>on the chemistry is essential preparation for the next big one.

486
00:24:06.160 --> 00:24:08.680
<v Speaker 2>This has been just an incredible deep dive. We've traced

487
00:24:08.680 --> 00:24:11.319
<v Speaker 2>this path all the way from a massive solar eruption

488
00:24:11.920 --> 00:24:15.519
<v Speaker 2>down to the invisible molecular chemistry that dictates how fast

489
00:24:15.599 --> 00:24:17.119
<v Speaker 2>our global technology can recover.

490
00:24:17.279 --> 00:24:18.200
<v Speaker 3>It's quite a journey.

491
00:24:18.279 --> 00:24:21.920
<v Speaker 2>We started with that violent instantaneous compression of Superstorm Gannon,

492
00:24:22.160 --> 00:24:25.599
<v Speaker 2>where Earth's plasma shield just collapsed from forty four thousand

493
00:24:25.640 --> 00:24:29.279
<v Speaker 2>kilometers down to nine thousand, six hundred in only nine hours.

494
00:24:29.119 --> 00:24:33.559
<v Speaker 3>And we ended up understanding this profound vulnerability that was

495
00:24:33.640 --> 00:24:37.599
<v Speaker 3>hidden in the aftermath. The real scientific revelation of this

496
00:24:37.720 --> 00:24:41.240
<v Speaker 3>storm wasn't just the strength of the punch. It was

497
00:24:41.359 --> 00:24:43.279
<v Speaker 3>the sluggishness of the recovery.

498
00:24:43.400 --> 00:24:45.440
<v Speaker 2>That four day delay, That four day.

499
00:24:45.319 --> 00:24:48.559
<v Speaker 3>Delay, the longest we've observed since twenty seventeen, was directly

500
00:24:48.559 --> 00:24:52.720
<v Speaker 3>because of the negative storm, the massive widespread chemical depletion

501
00:24:52.839 --> 00:24:53.880
<v Speaker 3>of the ionosphere.

502
00:24:53.960 --> 00:24:56.119
<v Speaker 2>So to put it simply, the physics of the storm

503
00:24:56.160 --> 00:24:58.440
<v Speaker 2>broke the shield fast, but it was the chemistry of

504
00:24:58.480 --> 00:25:01.680
<v Speaker 2>the upper atmosphere that delayed the r It just choked

505
00:25:01.720 --> 00:25:03.960
<v Speaker 2>off the supply line of particles needed to refill that

506
00:25:04.000 --> 00:25:04.799
<v Speaker 2>protective bubble.

507
00:25:05.039 --> 00:25:07.279
<v Speaker 3>And the study gives us the clearest picture we've ever had,

508
00:25:07.680 --> 00:25:10.000
<v Speaker 3>thanks to that combined data from the ERASE satellite and

509
00:25:10.039 --> 00:25:13.039
<v Speaker 3>the ground based GPS network, of the precise link between

510
00:25:13.240 --> 00:25:17.039
<v Speaker 3>solar energy, atmosphere chemical changes, and the multi day vulnerability

511
00:25:17.079 --> 00:25:19.519
<v Speaker 3>of our protective environment. It really does alter how we

512
00:25:19.599 --> 00:25:20.799
<v Speaker 3>define space weather risk.

513
00:25:21.160 --> 00:25:23.880
<v Speaker 2>So what does this all mean for you listening right now?

514
00:25:24.279 --> 00:25:27.319
<v Speaker 2>It means that when scientists talk about space weather, they're

515
00:25:27.359 --> 00:25:30.519
<v Speaker 2>not just talking about magnetic fields anymore. They are talking

516
00:25:30.559 --> 00:25:34.200
<v Speaker 2>about atmospheric chemistry that directly affects the stability of your

517
00:25:34.240 --> 00:25:36.640
<v Speaker 2>GPS and your communication systems.

518
00:25:37.000 --> 00:25:39.200
<v Speaker 3>Yeah, the protection of our modern world isn't just about

519
00:25:39.200 --> 00:25:42.119
<v Speaker 3>how strong the initial shield is. It's about how quickly

520
00:25:42.200 --> 00:25:44.359
<v Speaker 3>that particle supply chain can be restored.

521
00:25:44.519 --> 00:25:46.200
<v Speaker 2>So let's leave you with a final thought on that.

522
00:25:46.559 --> 00:25:50.440
<v Speaker 3>If a superstorm that happens only once every twenty to

523
00:25:50.480 --> 00:25:54.200
<v Speaker 3>twenty five years can cause these measurable multi day disruptions

524
00:25:54.200 --> 00:25:59.240
<v Speaker 3>to essential services, just consider this. What would the impact

525
00:25:59.279 --> 00:26:01.480
<v Speaker 3>look like if we were hit by an even rarer,

526
00:26:02.000 --> 00:26:05.759
<v Speaker 3>truly historic event, something like the eighteen fifty nine Carrington event,

527
00:26:05.920 --> 00:26:08.000
<v Speaker 3>a storm maybe ten times stronger than Gannon.

528
00:26:08.240 --> 00:26:11.440
<v Speaker 2>Given that our society is just exponentially more reliant on precise,

529
00:26:11.519 --> 00:26:14.680
<v Speaker 2>uninterrupted satellite technology today than we were even twenty five

530
00:26:14.720 --> 00:26:17.440
<v Speaker 2>years ago, that four day lag time could easily become

531
00:26:17.480 --> 00:26:19.920
<v Speaker 2>a two week lag time after a major event, and.

532
00:26:19.880 --> 00:26:22.480
<v Speaker 3>That becomes a truly existential infrastructure risk.

533
00:26:22.640 --> 00:26:24.839
<v Speaker 2>Something tom all over the next time you rely on

534
00:26:24.839 --> 00:26:26.599
<v Speaker 2>your GPS to get you somewhere.

535
00:27:00.559 --> 00:28:03.359
<v Speaker 4>People most nations, said the School da
