Tuesday, September 3, 2024

4546 - SOLAR FLARES and the damage they cause?

 

-    4546 -  SOLAR  FLARES  and the damage they cause?  -   The sun is on the verge of a significant event called a “magnetic field reversal”.   This phenomenon happens roughly every 11 years and marks an important stage in the solar cycle. The shift in polarity indicates the halfway point of solar maximum, the height of solar activity, and the beginning of the shift toward solar minimum.



----------------------------------  4546  -  SOLAR  FLARES  and the damage they cause?

-    The last time the sun's magnetic field flipped was toward the end of 2013.   To understand the magnetic field's reversal, it's important to be familiar with the solar cycle. This approximately 11-year cycle of solar activity is driven by the sun's magnetic field and is indicated by the frequency and intensity of sunspots visible on the surface. The height of solar activity during a given solar cycle is known as solar maximum, and current estimates predict it will occur between late 2024 and early 2026.

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-    A lesser-known cycle that encapsulates two 11-year solar cycles. Known as the “Hale cycle”, this magnetic cycle lasts approximately 22 years, through which the sun's magnetic field reverses and then reverts to its original state.

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-    During solar minimum, the sun's magnetic field is close to a dipole, with one north pole and one south pole, similar to Earth's magnetic field. But as we shift toward solar maximum, the sun's magnetic field becomes more complex, without a clear north-south pole separation. By the time solar maximum passes and solar minimum arrives, the sun has returned to a dipole,  with a flipped polarity.

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-    The upcoming switch in polarity will be from the northern to southern magnetic field in the Northern Hemisphere and vice versa in the Southern Hemisphere.  This will bring it to a similar magnetic orientation to Earth, which also has its southern-pointing magnetic field in the Northern Hemisphere.

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-    The reversal is driven by sunspots, magnetically complex regions of the sun's surface that can spawn significant solar events, such as solar flares and “coronal mass ejections” (CMEs), large blasts of plasma and magnetic field.

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-   As sunspots emerge close to the equator, they will have an orientation matching the old magnetic field, while sunspots forming closer to the poles will have a magnetic field matching the incoming magnetic orientation. This is called “Hale's law”.

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-    The magnetic field from active regions makes its way toward the poles and eventually causes the reversal.  But the exact underlying cause of such a flip in polarity remains mysterious.

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-    What we do know is that the solar magnetic field flip is not instantaneous. It's a gradual transition from a dipole to a complex magnetic field, to a reversed dipole over the entire 11-year solar cycle. "In short, there is no specific 'moment' in which the sun's poles flip.    It's not like the Earth, where the flip is measured by the migration of the North/South pole.

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-   It generally takes a year or two for a complete reversal, but it can vary significantly.  The north polar field of Solar Cycle 24, which ended in December 2019, took nearly five years to reverse.

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-    How does the sun's magnetic flip affect us?    There is no doubt that the sun has been incredibly active recently, firing out numerous powerful solar flares and CMEs, triggering strong geomagnetic storms on Earth, which, in turn, have produced some incredible auroral displays.

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-    Space weather is typically the strongest during solar maximum, when the sun's magnetic field is also the most complex.   One side effect of the magnetic field shift is slight but primarily beneficial.  It can help shield Earth from galactic cosmic rays which are high-energy subatomic particles that travel at near light speed and can damage spacecraft and harm orbiting astronauts who are outside Earth's protective atmosphere.

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-   As the sun's magnetic field shifts, the "current sheet", a sprawling surface that radiates billions of miles outward from the sun's equator, becomes very wavy, providing a better barrier against cosmic rays. 

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-     When giant solar storms hit Earth, they trigger beautiful auroral displays high in Earth’s atmosphere. There’s a dark side to this solar activity, though. The “space weather” it sets off also threatens our technology. The potential for damage is why we need highly accurate predictions of just when these storms will impact our planet’s magnetosphere.

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-   The specific places on the Sun where these storms erupt are called “coronal mass ejections” (CMEs). They’re huge explosions of magnetically charged particles and gases from the Sun. They travel through space and hit whatever is in their way, including planets.

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-    When that cloud of charged particles hits our magnetic field, it sets off a chain reaction of events.   It creates beautiful auroral displays, northern and southern lights that dance in the skies. But, they also slam into and can damage orbiting satellites, including all our telecommunications and navigation systems for planes, boats, and trains.

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-    The danger is even greater for astronauts aboard orbiting space stations because radiation is a constant threat to human life. On Earth, those storms can cause huge circulating electrical currents that can damage electric power grids. The damage to technology just ripples across the planet.

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-    This is why satellite operators and others want more accurate predictions of just when a space weather event triggered by a CME will hit us. To figure that out, solar physicists have to look back at the Sun and the sequence of events that cause CMEs.

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-     CMEs emanate from active regions on the Sun. These are places with very strong magnetic fields. The magnetic field lines form loops that get twisted and eventually, they break. When that happens, there’s a huge outburst of material, the CME. Typically, they travel out from the Sun at anywhere from 100 km/sec to 3,000 km/sec. That large uncertainty makes it tough to predict when the solar cloud will hit Earth.

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-   The height above the Sun where the magnetic field becomes unstable is called the “critical height” and it can help scientists predict the speed and arrival time of a coronal mass ejection.

By measuring how the strength of the magnetic field decreases with height, we can determine this critical height.  This data can then be used along with a geometric model which is used to track the true speed of CMEs in three dimensions, rather than just two, which is essential for precise predictions.

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-    Knowing the actual speed of the CME to a higher degree of accuracy will let solar physicists predict when it will hit Earth. That, in turn, will allow satellite operators, grid owners, space agencies, and others to prepare for the action and protect their assets.

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-    Our Sun goes through periods where it is more “outbursty” than others. Some of the strongest solar storms occur during the solar maximum part of the Sun’s 11-year sunspot cycle. Whenever they happen they can cause a lot of damage.

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-    One famous storm occurred on March 13, 1989. It was a combo of two CMEs that lifted off the Sun on March 10th and March 12th. They stirred up currents low in Earth’s atmosphere at the same time they triggered auroral displays. At the time, power grids were not necessarily “hardened” against such events. As a result, the Hydro-Quebec power grid shut down and suffered tremendous damage. The power was out for days across eastern Canada and parts of the United States.

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-    Another huge storm hit around Halloween in 2003. It affected satellite systems, cut off communications, some power systems shut down, and people around the world saw a dazzling display of aurorae. In space, the SOHO solar satellite shut down briefly. Astronauts onboard the ISS had to take shelter in a safe place aboard the station.

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-    Today, we’re in another cycle of heightened solar activity. We’ve already seen strong storms in May of 2024, and more will surely occur. So far they haven’t caused much damage, and they’ve given us some lovely auroral displays. Luckily, advanced research on these solar storms has helped technology operators and space agencies “harden” their systems.

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-     However, there’s only so much they can do to protect their assets. Having highly accurate advance predictions of just when a CME will impact our planet is a big step forward. At the very least, these operators will be able to reposition satellites, strengthen their power grids and other communications technology, and give astronauts in space advance warning. In future years, when we have people on the Moon or on their way to Mars, such predictions will help keep them safe, too.

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August 31, 2024     SOLAR  FLARES  and the damage they cause?           4546

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--------------------- ---  Tuesday, September 3, 2024  ---------------------------------

 

 

 

 

 

           

 

 

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