aads

Does space weather threaten high-tech life?

A coronal mass ejection erupts from the sun in 2012. Image via NASA.

By Roger Dube, Rochester Institute of Technology

Shortly after 4 a.m. on a crisp, cloudless September morning in 1859, the sky above what is currently Colorado erupted in bright red and green colors. Fooled by the brightness into thinking it was an early dawn, gold-rush miners in the mountainous region of what was then called the Kansas Territory woke up and started making breakfast. What happened in more developed regions was even more disorienting, and carries a warning for the wired high-tech world of the 21st century.

As the sky lit up over the nighttime side of the Earth, telegraph systems worldwide went berserk, clacking nonsense code and emitting large sparks that ignited fires in nearby piles of paper tape. Telegraph operators suffered electrical burns. Even disconnecting the telegraph units from their power sources didn’t stop the frenzy, because the transmission wires themselves were carrying huge electrical currents. Modern technology had just been humbled by a fierce space weather storm that had arrived from the sun, the largest ever recorded – and more than twice as powerful as a storm nine years earlier, which had itself been the largest in known history.

My seven years of research on predicting solar storms, combined with my decades using GPS satellite signals under various solar storm conditions, indicate that today’s even more sensitive electronics and satellites would be devastated should an event of that magnitude occur again. In 2008, a panel of experts commissioned by the National Academy of Sciences issued a detailed report with a sobering conclusion: The world would be thrown back to the life of the early 1800s, and it would take years – or even a decade – to recover from an event that large.

A solar explosion

Space weather storms have happened since the birth of the solar system, and have hit Earth many times, both before and after that massive event in 1859, which was named the Carrington event after a British astronomer who recorded his observations of the sun at the time. They’re caused by huge electromagnetic explosions on the surface of the sun, called coronal mass ejections. Each explosion sends billions of protons and electrons, in a superheated ball of plasma, out into the solar system.

About one in every 20 coronal mass ejections heads in a direction that intersects Earth’s orbit. Around three days later, our planet experiences what is called a space weather storm or a geomagnetic storm.

While these events are described using terms like “weather” and “storm,” they do not affect whether it’s rainy or sunny, hot or cold, or other aspects of what it’s like outdoors on any given day. Their effects are not meteorological, but only electromagnetic.

Image via NASA/Terry Zaperach.

Hitting Earth

When the coronal mass ejection arrives at Earth, the charged particles collide with air molecules in the upper atmosphere, generating heat and light called aurora.

Also, as happens anytime moving electrical charges encounter a magnetic field, the interaction creates a spontaneous electrical current in any conductor that’s available. If the plasma ball is big enough, its interaction with Earth’s magnetic field can induce large currents on long wires on the ground, like the one that overloaded telegraph circuits in 1859.

On March 13, 1989, a storm only about one-fifth as strong as the Carrington event hit Earth. It induced a large surge of current in the long power lines of the Hydro-Quebec power grid, causing physical damage to transmission equipment and leaving 6 million people without power for nine hours. Another storm-induced power surge destroyed a large transformer at a New Jersey nuclear plant. Even though a spare transformer was nearby, it still took six months to remove and replace the melted unit. Some people worried that the bright auroral lights meant nuclear war had broken out.

And in October 2003, a rapid series of solar storms affected Earth. Collectively called the Halloween solar storm, this series caused surges that threatened the North American power grid. Its effects on satellites made GPS navigation erratic and interrupted communications connections during the peak of the storm.

Larger storms will have wider effects, cause more damage and take longer to recover from.

Wide-reaching effects

Geomagnetic storms attack the lifeblood of modern technology: electricity. A space weather storm typically lasts for two or three days, during which the entire planet is subjected to powerful electromagnetic forces. The National Academy of Sciences study concluded that an especially massive storm would damage and shut down power grids and communications networks worldwide.

Electricity, shown in the upper right, is integrated into every aspect of modern life. Image via Federal Communications Commission.

After the storm passed, there would be no simple way to restore power. Manufacturing plants that build replacements for burned-out lines or power transformers would have no electricity themselves. Trucks needed to deliver raw materials and finished equipment wouldn’t be able to fuel up, either: Gas pumps run on electricity. And what pumps were running would soon dry up, because electricity also runs the machinery that extracts oil from the ground and refines it into usable fuel.

With transportation stalled, food wouldn’t get from farms to stores. Even systems that seem non-technological, like public water supplies, would shut down: Their pumps and purification systems need electricity. People in developed countries would find themselves with no running water, no sewage systems, no refrigerated food, and no way to get any food or other necessities transported from far away. People in places with more basic economies would also be without needed supplies from afar.

It could take between four and 10 years to repair all the damage. In the meantime, people would need to grow their own food, find and carry and purify water, and cook meals over fires.

Some systems would continue to operate, of course: bicycles, horse-drawn carriages and sailing ships. But another type of equipment that would keep working provides a clue to preventing this type of disaster: Electric cars would continue to work, but only in places where there were solar panels and wind turbines to recharge them.

Preparing and protecting

Geomagnetic storms would affect those small-scale installations far less than grid-scale systems. It’s a basic principle of electricity and magnetism that the longer a wire that’s exposed to a moving magnetic field, the larger the current that’s induced in that wire.

In 1859, the telegraph system was so profoundly affected because it had wires stretching from city to city across the U.S. Those very long wires had to handle enormous amounts of energy all at once, and failed. Today, there are long runs of wires connecting power generators to consumers – such as from Niagara Falls to New York City – that would be similarly susceptible to large induced currents.

The only way to reduce vulnerability to geomagnetic storms is to substantially revamp the power grid. Now, it is a vast web of wires that effectively spans continents. Governments, businesses and communities need to work together to split it into much smaller components, each serving a town or perhaps even a neighborhood – or an individual house. These “microgrids” can be connected to each other, but should have protections built in to allow them to be disconnected quickly when a storm approaches. That way, the length of wires affected by the storm will be shorter, reducing the potential for damage.

A family using solar panels and batteries for storage and an electric car to get around would likely find its water supply, natural gas or internet service disrupted. But their freedom to travel, and to use electric lights to work after dark, would provide a much better chance at survival.

When will the next storm hit?

People should start preparing today. It’s impossible to know when a major storm will hit next: The most we’ll get is a three-day warning when something happens on the surface of the sun. It’s really only a matter of time before there is another one like the Carrington event.

Solar astrophysicists are also studying the sun to identify any events or conditions that might herald a coronal mass ejection. They’re collecting enormous amounts of data about the sun and using computer analysis to try to connect that information to geomagnetic storms on Earth. This work is underway and will become more refined over time. The research has not yet yielded a reliable prediction of a coming solar storm before an ejection occurs, but it improves each year.

The ConversationIn my view, the safest course of action involves developing microgrids based on renewable energy. That would not only improve people’s quality of life around the planet right now, but also provide the best opportunity to maintain that lifestyle when adverse events happen.

Roger Dube, Research Professor of Imaging Science, Rochester Institute of Technology

This article was originally published on The Conversation. Read the original article.

Bottom line: According to a scientist who studies solar storms, the wired Earth of the 21st century is at the mercy of the volatile nature of the sun.



from EarthSky https://ift.tt/2GAVDFK

A coronal mass ejection erupts from the sun in 2012. Image via NASA.

By Roger Dube, Rochester Institute of Technology

Shortly after 4 a.m. on a crisp, cloudless September morning in 1859, the sky above what is currently Colorado erupted in bright red and green colors. Fooled by the brightness into thinking it was an early dawn, gold-rush miners in the mountainous region of what was then called the Kansas Territory woke up and started making breakfast. What happened in more developed regions was even more disorienting, and carries a warning for the wired high-tech world of the 21st century.

As the sky lit up over the nighttime side of the Earth, telegraph systems worldwide went berserk, clacking nonsense code and emitting large sparks that ignited fires in nearby piles of paper tape. Telegraph operators suffered electrical burns. Even disconnecting the telegraph units from their power sources didn’t stop the frenzy, because the transmission wires themselves were carrying huge electrical currents. Modern technology had just been humbled by a fierce space weather storm that had arrived from the sun, the largest ever recorded – and more than twice as powerful as a storm nine years earlier, which had itself been the largest in known history.

My seven years of research on predicting solar storms, combined with my decades using GPS satellite signals under various solar storm conditions, indicate that today’s even more sensitive electronics and satellites would be devastated should an event of that magnitude occur again. In 2008, a panel of experts commissioned by the National Academy of Sciences issued a detailed report with a sobering conclusion: The world would be thrown back to the life of the early 1800s, and it would take years – or even a decade – to recover from an event that large.

A solar explosion

Space weather storms have happened since the birth of the solar system, and have hit Earth many times, both before and after that massive event in 1859, which was named the Carrington event after a British astronomer who recorded his observations of the sun at the time. They’re caused by huge electromagnetic explosions on the surface of the sun, called coronal mass ejections. Each explosion sends billions of protons and electrons, in a superheated ball of plasma, out into the solar system.

About one in every 20 coronal mass ejections heads in a direction that intersects Earth’s orbit. Around three days later, our planet experiences what is called a space weather storm or a geomagnetic storm.

While these events are described using terms like “weather” and “storm,” they do not affect whether it’s rainy or sunny, hot or cold, or other aspects of what it’s like outdoors on any given day. Their effects are not meteorological, but only electromagnetic.

Image via NASA/Terry Zaperach.

Hitting Earth

When the coronal mass ejection arrives at Earth, the charged particles collide with air molecules in the upper atmosphere, generating heat and light called aurora.

Also, as happens anytime moving electrical charges encounter a magnetic field, the interaction creates a spontaneous electrical current in any conductor that’s available. If the plasma ball is big enough, its interaction with Earth’s magnetic field can induce large currents on long wires on the ground, like the one that overloaded telegraph circuits in 1859.

On March 13, 1989, a storm only about one-fifth as strong as the Carrington event hit Earth. It induced a large surge of current in the long power lines of the Hydro-Quebec power grid, causing physical damage to transmission equipment and leaving 6 million people without power for nine hours. Another storm-induced power surge destroyed a large transformer at a New Jersey nuclear plant. Even though a spare transformer was nearby, it still took six months to remove and replace the melted unit. Some people worried that the bright auroral lights meant nuclear war had broken out.

And in October 2003, a rapid series of solar storms affected Earth. Collectively called the Halloween solar storm, this series caused surges that threatened the North American power grid. Its effects on satellites made GPS navigation erratic and interrupted communications connections during the peak of the storm.

Larger storms will have wider effects, cause more damage and take longer to recover from.

Wide-reaching effects

Geomagnetic storms attack the lifeblood of modern technology: electricity. A space weather storm typically lasts for two or three days, during which the entire planet is subjected to powerful electromagnetic forces. The National Academy of Sciences study concluded that an especially massive storm would damage and shut down power grids and communications networks worldwide.

Electricity, shown in the upper right, is integrated into every aspect of modern life. Image via Federal Communications Commission.

After the storm passed, there would be no simple way to restore power. Manufacturing plants that build replacements for burned-out lines or power transformers would have no electricity themselves. Trucks needed to deliver raw materials and finished equipment wouldn’t be able to fuel up, either: Gas pumps run on electricity. And what pumps were running would soon dry up, because electricity also runs the machinery that extracts oil from the ground and refines it into usable fuel.

With transportation stalled, food wouldn’t get from farms to stores. Even systems that seem non-technological, like public water supplies, would shut down: Their pumps and purification systems need electricity. People in developed countries would find themselves with no running water, no sewage systems, no refrigerated food, and no way to get any food or other necessities transported from far away. People in places with more basic economies would also be without needed supplies from afar.

It could take between four and 10 years to repair all the damage. In the meantime, people would need to grow their own food, find and carry and purify water, and cook meals over fires.

Some systems would continue to operate, of course: bicycles, horse-drawn carriages and sailing ships. But another type of equipment that would keep working provides a clue to preventing this type of disaster: Electric cars would continue to work, but only in places where there were solar panels and wind turbines to recharge them.

Preparing and protecting

Geomagnetic storms would affect those small-scale installations far less than grid-scale systems. It’s a basic principle of electricity and magnetism that the longer a wire that’s exposed to a moving magnetic field, the larger the current that’s induced in that wire.

In 1859, the telegraph system was so profoundly affected because it had wires stretching from city to city across the U.S. Those very long wires had to handle enormous amounts of energy all at once, and failed. Today, there are long runs of wires connecting power generators to consumers – such as from Niagara Falls to New York City – that would be similarly susceptible to large induced currents.

The only way to reduce vulnerability to geomagnetic storms is to substantially revamp the power grid. Now, it is a vast web of wires that effectively spans continents. Governments, businesses and communities need to work together to split it into much smaller components, each serving a town or perhaps even a neighborhood – or an individual house. These “microgrids” can be connected to each other, but should have protections built in to allow them to be disconnected quickly when a storm approaches. That way, the length of wires affected by the storm will be shorter, reducing the potential for damage.

A family using solar panels and batteries for storage and an electric car to get around would likely find its water supply, natural gas or internet service disrupted. But their freedom to travel, and to use electric lights to work after dark, would provide a much better chance at survival.

When will the next storm hit?

People should start preparing today. It’s impossible to know when a major storm will hit next: The most we’ll get is a three-day warning when something happens on the surface of the sun. It’s really only a matter of time before there is another one like the Carrington event.

Solar astrophysicists are also studying the sun to identify any events or conditions that might herald a coronal mass ejection. They’re collecting enormous amounts of data about the sun and using computer analysis to try to connect that information to geomagnetic storms on Earth. This work is underway and will become more refined over time. The research has not yet yielded a reliable prediction of a coming solar storm before an ejection occurs, but it improves each year.

The ConversationIn my view, the safest course of action involves developing microgrids based on renewable energy. That would not only improve people’s quality of life around the planet right now, but also provide the best opportunity to maintain that lifestyle when adverse events happen.

Roger Dube, Research Professor of Imaging Science, Rochester Institute of Technology

This article was originally published on The Conversation. Read the original article.

Bottom line: According to a scientist who studies solar storms, the wired Earth of the 21st century is at the mercy of the volatile nature of the sun.



from EarthSky https://ift.tt/2GAVDFK

Last night’s moon and Jupiter

Martin Marthadinata in Surabaya, East Java, Indonesia caught the moon and Jupiter on April 3, 2018. From his location, he said, the moon rose at 7:53 p.m. local time.

The bright moon swept past bright Jupiter this week. They were closest on the nights of April 2 and 3, but people around the globe are still seeing them – ascending in the eastern part of the sky beginning around mid- to late evening, well up before dawn – and you can see them, too. Just watch for the moon! The bright object nearby is Jupiter.

Moon and Jupiter on April 3, 2018 from Joey Zahari on Penang Island, Malaysia.

Bottom line: Photos of the moon and Jupiter, April 2018.



from EarthSky https://ift.tt/2GwlOkZ

Martin Marthadinata in Surabaya, East Java, Indonesia caught the moon and Jupiter on April 3, 2018. From his location, he said, the moon rose at 7:53 p.m. local time.

The bright moon swept past bright Jupiter this week. They were closest on the nights of April 2 and 3, but people around the globe are still seeing them – ascending in the eastern part of the sky beginning around mid- to late evening, well up before dawn – and you can see them, too. Just watch for the moon! The bright object nearby is Jupiter.

Moon and Jupiter on April 3, 2018 from Joey Zahari on Penang Island, Malaysia.

Bottom line: Photos of the moon and Jupiter, April 2018.



from EarthSky https://ift.tt/2GwlOkZ

Get to know Earth’s magnetosphere

Scientists say our magnetosphere was key to helping Earth develop into a habitable planet. This magnetic bubble deflects most of the solar material sweeping towards us from our star at 1 million miles (1.6 million km) per hour or more. Without the magnetosphere, the relentless action of these solar particles could strip the Earth of the protective layers that shield us from the sun’s ultraviolet radiation.

Bottom line: NASA ScienceCasts video on Earth’s magnetosphere.

Read more from NASA



from EarthSky https://ift.tt/2GW0wNe

Scientists say our magnetosphere was key to helping Earth develop into a habitable planet. This magnetic bubble deflects most of the solar material sweeping towards us from our star at 1 million miles (1.6 million km) per hour or more. Without the magnetosphere, the relentless action of these solar particles could strip the Earth of the protective layers that shield us from the sun’s ultraviolet radiation.

Bottom line: NASA ScienceCasts video on Earth’s magnetosphere.

Read more from NASA



from EarthSky https://ift.tt/2GW0wNe

Antarctic ice grounding lines are shifting

View larger. | Illustration of the rates of grounding line migration around Antarctica between 2010 and 2016, via ESA.

The European Space Agency said on April 3, 2018 that its CryoSat satellite mission has revealed a shifting inward of the grounding lines of ice sheets in Antarctica. Over the last seven years, ESA said, Antarctica has lost an area of underwater ice nearly the size of Greater London (about 90 miles, or 140 km across, according to Britannica.com). ESA said the grounding lines – the place where the base of Antarctic ice sheets leave the seabed and begin to float – is shifting inward. ESA said:

… warm ocean water beneath the continent’s floating margins is eating away at the ice attached to the seabed.

ESA said that between 2010 and 2017, the Southern Ocean melted about 565 square miles (1463 sq km) of underwater ice. A paper describing these results is published in the peer-reviewed journal Nature Geoscience. The paper describes how CryoSat was used to map grounding-line motion along nearly 10,000 miles (16,000 km) of Antarctic coastline, over seven years.

Read more from the European Space Agency

Bottom line: Illustration of shifting grounding lines of Antarctic ice sheets, over the last seven years, with data provided by an ESA satellite.

Source: Net retreat of Antarctic glacier grounding lines



from EarthSky https://ift.tt/2Gwksqr

View larger. | Illustration of the rates of grounding line migration around Antarctica between 2010 and 2016, via ESA.

The European Space Agency said on April 3, 2018 that its CryoSat satellite mission has revealed a shifting inward of the grounding lines of ice sheets in Antarctica. Over the last seven years, ESA said, Antarctica has lost an area of underwater ice nearly the size of Greater London (about 90 miles, or 140 km across, according to Britannica.com). ESA said the grounding lines – the place where the base of Antarctic ice sheets leave the seabed and begin to float – is shifting inward. ESA said:

… warm ocean water beneath the continent’s floating margins is eating away at the ice attached to the seabed.

ESA said that between 2010 and 2017, the Southern Ocean melted about 565 square miles (1463 sq km) of underwater ice. A paper describing these results is published in the peer-reviewed journal Nature Geoscience. The paper describes how CryoSat was used to map grounding-line motion along nearly 10,000 miles (16,000 km) of Antarctic coastline, over seven years.

Read more from the European Space Agency

Bottom line: Illustration of shifting grounding lines of Antarctic ice sheets, over the last seven years, with data provided by an ESA satellite.

Source: Net retreat of Antarctic glacier grounding lines



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Use the Big Dipper to find the Little Dipper

So you say you can find the Big Dipper, but not the Little Dipper? This post is for you. Here’s the view northward on April evenings. At present the Big Dipper is high in the north during the evening hours. Notice the two outer stars in the bowl of the Big Dipper. These two stars – called Duhbe and Merak – always point to Polaris, the North Star. Find Polaris, and you can find the Little Dipper.

Polaris is special because Earth’s northern axis nearly points to its location in the sky. It’s the star around which the entire northern sky appears to turn.

Polaris is also fun to locate for another reason. It’s part of a famous – though elusive – star pattern, known as the Little Dipper.

So here it is! The Little Dipper! The North Star, Polaris, marks the end of its handle.

View larger. | You can use the Big Dipper to identify lots of other sky favorites, too. In this shot, taken around 3:30 a.m. in July 2013, Tom Wildoner shows how you can use the two outer stars in the bowl of the Big Dipper to find the North Star, Polaris. Thanks, Tom!

View larger. | No matter where you see the Big Dipper, the two outer stars in its bowl point to Polaris. In this shot, Tom Wildoner caught the Big Dipper and Polaris at around 3:30 a.m. in July 2013. Thanks, Tom!

By the way, Polaris is less than a degree away from the true north celestial pole on the sky’s dome now. It’ll be closest to true north – less than half a degree away – in the year 2102. The change is due to a motion of Earth called “precession,” which causes Earth’s axis to trace out a circle among the stars every 26,000 years.

By the way, thousands of years ago, Polaris was an ordinary star in the northern sky, known to the Greeks by the name Phoenice.

Other ordinary stars in the northern sky now – Kochab and Pherkad, the two outermost stars in the bowl of the Little Dipper (see chart below) – have had the honor of being pole stars.

Kochab and Pherkad served as twin pole stars from about 1500 BC to about 500 BC.

They’re still sometimes called the Guardians of the Pole.

Kochab is located about 126 light-years away. Pherkad is more distant, at about 480 light-years by some estimates. Meanwhile, Polaris is a bit more than 400 light-years away.

Kochab and Pherkad are the 2 outermost stars in the bowl of the Little Dipper.

Bottom line: The Big Dipper is usually pretty easy to find, but the Little Dipper is less easy. This post tells you how to use the Big Dipper to find Polaris and the Little Dipper, plus how to recognize the stars Kochab and Pherkad.

Thuban: Past North Star

Star Errai: Future North Star

EarthSky astronomy kits are perfect for beginners. Order today from the EarthSky store

Donate: Your support means the world to us



from EarthSky https://ift.tt/1CyCBFv

So you say you can find the Big Dipper, but not the Little Dipper? This post is for you. Here’s the view northward on April evenings. At present the Big Dipper is high in the north during the evening hours. Notice the two outer stars in the bowl of the Big Dipper. These two stars – called Duhbe and Merak – always point to Polaris, the North Star. Find Polaris, and you can find the Little Dipper.

Polaris is special because Earth’s northern axis nearly points to its location in the sky. It’s the star around which the entire northern sky appears to turn.

Polaris is also fun to locate for another reason. It’s part of a famous – though elusive – star pattern, known as the Little Dipper.

So here it is! The Little Dipper! The North Star, Polaris, marks the end of its handle.

View larger. | You can use the Big Dipper to identify lots of other sky favorites, too. In this shot, taken around 3:30 a.m. in July 2013, Tom Wildoner shows how you can use the two outer stars in the bowl of the Big Dipper to find the North Star, Polaris. Thanks, Tom!

View larger. | No matter where you see the Big Dipper, the two outer stars in its bowl point to Polaris. In this shot, Tom Wildoner caught the Big Dipper and Polaris at around 3:30 a.m. in July 2013. Thanks, Tom!

By the way, Polaris is less than a degree away from the true north celestial pole on the sky’s dome now. It’ll be closest to true north – less than half a degree away – in the year 2102. The change is due to a motion of Earth called “precession,” which causes Earth’s axis to trace out a circle among the stars every 26,000 years.

By the way, thousands of years ago, Polaris was an ordinary star in the northern sky, known to the Greeks by the name Phoenice.

Other ordinary stars in the northern sky now – Kochab and Pherkad, the two outermost stars in the bowl of the Little Dipper (see chart below) – have had the honor of being pole stars.

Kochab and Pherkad served as twin pole stars from about 1500 BC to about 500 BC.

They’re still sometimes called the Guardians of the Pole.

Kochab is located about 126 light-years away. Pherkad is more distant, at about 480 light-years by some estimates. Meanwhile, Polaris is a bit more than 400 light-years away.

Kochab and Pherkad are the 2 outermost stars in the bowl of the Little Dipper.

Bottom line: The Big Dipper is usually pretty easy to find, but the Little Dipper is less easy. This post tells you how to use the Big Dipper to find Polaris and the Little Dipper, plus how to recognize the stars Kochab and Pherkad.

Thuban: Past North Star

Star Errai: Future North Star

EarthSky astronomy kits are perfect for beginners. Order today from the EarthSky store

Donate: Your support means the world to us



from EarthSky https://ift.tt/1CyCBFv

Unmanned Technology: Breaching the Battlefield with the Brits

Troops from the United Kingdom and U.S. observed and tested a series of unmanned, remote-controlled ground vehicles in Germany, benefiting warfighters from both nations.

from https://ift.tt/2GQ9R97
Troops from the United Kingdom and U.S. observed and tested a series of unmanned, remote-controlled ground vehicles in Germany, benefiting warfighters from both nations.

from https://ift.tt/2GQ9R97

Quantum (Network) Leap: Army Scientists Explore Fiber Optics

Einstein once called it, "spooky action at a distance." Quantum entanglement may lead to ultra-secure, futuristic networks and communications, and Army scientists are working hard to bring the potential of this science and technology to future military members.

from https://ift.tt/2H7yn3g
Einstein once called it, "spooky action at a distance." Quantum entanglement may lead to ultra-secure, futuristic networks and communications, and Army scientists are working hard to bring the potential of this science and technology to future military members.

from https://ift.tt/2H7yn3g

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