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  • Traveling at the near speed of light, energetic particles shooting out from the sun can zip

  • through space, smack into our planet’s atmosphere, and cause incredible disruptions. And one

  • of the biggest impacts we know of happened during the tail end of the Vietnam WarPresident

  • Nixon really wanted to pull us out, but wanted to do it sort of saving face, and decided

  • that the best way to do that was to stop the flow of war material into North Vietnam. The

  • decision was to mine Haiphong Harbor, and many of the smaller harbors to the South.

  • This is Delores Knipp, a space weather scientist and former officer in the US Air Force. She

  • likes digging into dusty archives, and uncovered a war mystery that’s now connected to a

  • major solar eventSpace weather forecasters had noticed that there was one region on the

  • Sun that appeared to be a little more active than anticipated. They kept watching it, and

  • then when it came around in late July 1972 on the east limb of the Sun it was already

  • large. It did start producing solar flares, producing coronal mass ejections but at that

  • time we didn't have those wordsWe didn't really understand the concept of the Sun actually

  • throwing mass, and magnetic material out. We had a general sense that something like

  • a plasma cloud was coming at us, but our ideas were that, "Well, okay it might get here in

  • a couple three days." As a matter of fact, it got here in 14.6 hours. Typically, the

  • solar wind is moving at about 400 kilometers per second, which is supersonic, but very,

  • very tenuous. But this particular event in 1972 traveled at about 2,800 kilometers per

  • second, so seven times faster than the norm, and carrying tremendous magnetic field, and

  • mass with it. And when that hit, our magnetic shield virtually buckled. We had no idea that

  • something could come from the Sun that fast. We were pretty much unprepared. And when it

  • hit earth, those sea mines blew up. Those mines were what the president was relying

  • on to keep the pressure on in the war. And suddenly the whole mine field had been swept

  • by nature, by the Sun, by a CME. That created probably one of the largest solar energetic

  • particle events in recorded history. The naval observers who were up at the time, it was

  • just past dawn, noted that there were a half-dozen sea mines that blew within 30 seconds. And

  • they go, "Whoa! Did we do that?" It was a furious time in terms of the Navy records,

  • trying to figure out what had happenedIn these declassified reports, Delores found

  • just a few lines that had basically said, "Yes, in August of 1972 "a solar storm swept

  • the sea mines in Haiphong Harbor." And so I go, "Oh, it looks like something did happen." There

  • were and are many impacts that have not been adequately described. And they're just now

  • starting to come to light. Our sun is a huge ball of magnetized gas and plasma, and it’s

  • activity goes through a roughly 11 year cycleWe know whether were in a solar maximum or

  • solar minimum by counting the number of sunspots on the surfaceThese spots are indicators

  • for giant eruptions, like solar flares, which are sudden outbursts of energy and coronal

  • mass ejections, which are even larger but slower eruptions from the Sun’s coronaThey

  • can increase during the sun’s cycle, but luckily, we have some built in protection.

  • We can think of Earth's magnetic field as being kind of a magnetic cocoon that keeps

  • most of the solar winds, magnetic field, and the plasma outside of Earth's atmosphere.

  • But when the sun decides to launch a really big ejection, sometimes the magnetic field

  • has to deform so dramatically that currents are generated, and those currents can actually

  • flow along the magnetic field lines down to Earth's surfaceAnd that's one of our biggest

  • concerns. If those extra currents are flowing in the ground, they're always looking for

  • the path of least resistanceAnd when they find a path along a long conducting pipe,

  • or in older times, telegraph wires, or now in our power grid, they will take that pathWe're

  • starting to understand that these are not once in a century events. These probably occur

  • more often than we thinkWe're in solar minimum now, we're kind of relaxed the next

  • solar maximum was forecast to be not too spectacularThe August '72 event came out of small sunspot

  • cycles. So we can't just take the sunspot count as the, oh, we don't have to worry about

  • it situation. We actually have to be monitoring the Sun 24/7. Today at NOAA’s Space Weather

  • Prediction Center, we have more eyes on the sun and better models to help us predict space

  • weather, which is affecting our magnetosphere, it's creating the Aurora, it's also energizing

  • particles and creating radiation environment that can affect satellites, it affects the

  • ionosphere in those regions and that impacts airlines that have flights from New York to

  • Beijing. There are several things that are really important for conducting space weather

  • operationsThe first are satellites, which serve as sentinels out in the abyssThe

  • GOES satellites give you the daily weather that you see on the news at night. But in

  • additionthe space weather observations consist of monitoring the energetic particles

  • in Earth's radiation belt at geosynchronous orbitThey also monitor the earth's magnetic

  • field and its variations. There's solar observations that are looking at the Sun in x-rays, in

  • extreme ultraviolet to give us information about activity on the sun. Activity like coronal

  • mass ejections and solar flares, which have different lead times once they eruptWe

  • classify solar flares here starting with what we call A. And then we have the B level and

  • then C level and then M’s and then X’s. And each one of those categories is ten times

  • more intense than the other. The 1972 event that blew up a bunch of sea mines were connected

  • to X class flaresWe have instruments measuring the intensity of the solar radiation and it

  • appears very quickly in near real time in front of our forecasters and then they could

  • use that information to provide their warnings and alerts. The other type of major event

  • is this coronal mass ejection, it’s moving much slower. Right now we're using coronagraphs

  • that are on a NASA satelliteIt takes as short as maybe 14 hours for a very fast eventbut

  • it can take more normally several days to reach usWe have a little bit more lead

  • time..to say something about how fast is it moving? When do we expect it at Earth? How

  • long do we expect it to last?" We've got another satellite that's entirely outside of earth's

  • magnetosphere in a location between Earth and the Sun called the Lagrange point L1.

  • That's a stable place where both the gravity and the centrifugal force of the satellite

  • balance out the earth's gravitational force and it's always there as a buoy upstream to

  • give us a warning of what's coming at EarthAnother key piece of their operations are models,

  • which are constantly evolving to improve predictionsThe Wang Sheeley Arge Enlil model shows us where

  • there's high speed solar wind coming at us, where there's low speed solar wind coming

  • at us, the density of that solar windWhen there's a large eruption on the sun of a coronal

  • mass ejection. The Wang Sheeley Arge Enlil model.. takes that coronal mass ejection and

  • puts it through that system and then it tells us what's going to arrive at EarthThe Geospace

  • model is telling us about magnetic variations in the vicinity of Earth and those magnetic

  • variations can cause geo electric fields. Those geo electric fields can drive currents

  • and power lines and disrupt power grids. Models are only as good as our understanding and

  • models don't catch everything and there are times where we have been surprisedThere

  • are a lot of features about the sun that we still don't understand. We need to be able

  • to model how the Sun's interior works the solar atmosphere. We need to be able to monitor

  • active regions of the sun and how they formThere is a huge concerns at the highest levels in

  • government to be able to better prepare for a large event to better mitigate the effects. I'm

  • optimistic about all of these new advances that are coming in and all of these things

  • which are going to contribute to our preparedness for the things the Sun is throwing at us.

  • It's a real sense of adventure. It's like you can realize that you're a part of something

  • that is developing. The Sun, it's so far away and yet, within a short amount of time, it

  • can have this amazing impactAnd it's not just oh yeah, the sun warms us up and we have

  • seasons, there's a lot more going on, and it's a very connected system. Even though

  • some of these stories have been hidden these things have actually happened, and there's

  • a potential for it to happen again.

Traveling at the near speed of light, energetic particles shooting out from the sun can zip

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地球の磁場が太陽嵐でどのようにゆがんで座屈するのか (How Earth's Magnetic Field Twists and Buckles During Solar Storms)

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    林宜悉 に公開 2021 年 01 月 14 日
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