In the sun's southern hemisphere, a large sunspot is turning toward Earth: movie. Sunspot 4197 is about 1/3rd the size of Carrington's sunspot. It looks even bigger though, because it is surrounded by a coterie of smaller spots. The crowd has a complex magnetic field that poses a threat for X-class solar flares. Solar flare alerts: SMS Text

SUNSPOTS AT SUNSET:
Sunspot 4197 is so large, it's altering the appearance of the setting sun. On Aug. 27th, Wolfgang Ott photographed the phenomenon as the sun dipped into the North Sea near St. Peter Ording, Germany:

"We were treated to a beautiful sunset this evening," says Ott. "The individual sunspot groups were easy to recognize."
The solar disk itself looks unusual--slightly squashed, almost egg-shaped. This is an effect of refraction. Thick layers of air near the horizon bend sunlight unevenly, distorting the sun’s outline.
The same thick air that deforms the sun also dims it, making the sunspots easier to see. However, don't let that lure you into staring. Even a dim sun can hurt your eyes, especially when it is magnified by optics. If you want to photograph the sunset as Ott did, please use the camera's LCD screen for safe viewfinding.
https://spaceweather.com/

It never made sense. On Feb. 3rd, 2022, SpaceX launched a batch of 49 Starlinks to low-Earth orbit--something they had done many times before. This time was different, though. Almost immediately, dozens of the new satellites began to fall out of the sky.

At the time, SpaceX offered this explanation: "Unfortunately, the satellites deployed on Thursday (Feb. 3rd) were significantly impacted by a geomagnetic storm on Friday, (Feb. 4th)."

A more accurate statement might have read "...impacted by a very minor geomagnetic storm." The satellites flew into a storm that barely registered on NOAA scales: It was a G1, the weakest possible, unlikely to cause a mass decay of satellites. Something about "The Starlink Incident" was not adding up.

Space scientists Scott McIntosh and Robert Leamon of Lynker Space, Inc., have a new and different idea: "The Terminator did it," says McIntosh.

Not to be confused with the killer robot, McIntosh's Terminator is an event on the sun that helps explain the mysterious progression of solar cycles. Four centuries after Galileo discovered sunspots, researchers still cannot accurately predict the timing and strength of the sun's 11-year solar cycle. Even "11 years" isn't real; observed cycles vary from less than 9 years to more than 14 years long.

McIntosh and Leamon realized that forecasters had been overlooking something. There is a moment that happens every 11 years or so when opposing magnetic fields from the sun's previous and upcoming solar cycles collide and cancel (see the animation, above). They called this moment, which signals the death of the old cycle, "The Termination Event."
After a Termination Event, the sun roars to life–"like a hot stove where someone suddenly turns the burner on," McIntosh likes to say. Solar ultraviolet radiation abruptly jumps to a higher level, heating the upper atmosphere and dramatically increasing aerodynamic drag on satellites.
This plot supports what McIntosh and Leamon are saying:

The histogram shows the number of objects falling out of Earth orbit each year since 1975. Vertical dashed lines mark Termination Events. There's an uptick in satellite decay around the time of every Terminator, none bigger than 2022.
As SpaceX was assembling the doomed Starlinks of Group 4-7 in early 2022, they had no idea that the Terminator Event had, in fact, just happened. Unwittingly, they launched the satellites into a radically altered near-space environment. "Some of our satellite partners said it was just pea soup up there," says Leamon.
SpaceX wasn't the only company hit hard. Capella Space also struggled in 2022 to keep its constellation of Synthetic Aperture Radar (SAR) satellites in orbit.
“The atmospheric density in low Earth orbit was 2 to 3 times more than expected,” wrote Capella Space's Scott Shambaugh in a paper entitled Doing Battle With the Sun. “This increase in drag threatened to prematurely de-orbit some of our spacecraft." Indeed, many did deorbit earlier than their 3-year design lifetimes.
The Terminator did it? It makes more sense than a minor storm.

Giant sunspot AR3664 is no longer facing Earth. That makes it extra dangerous. The Carrington-class sunspot is passing over the sun's western limb--a region of the sun that is magnetically connected to our planet. Indeed, we are feeling the effects of that connection right now; take a look at this map of ongoing radio blackouts:

Red zones in the map show where shortwave radio signals are being absorbed. Inside the Arctic Circle, frequencies below 30 MHz are almost completely blacked out, a nuisance for polar aviators and ham radio operators.
What's causing this? Protons accelerated by solar flares in the magnetic canopy of AR3664 are following the Parker Spiral back to Earth. Think of it as a magnetic superhighway. The arriving particles are funneled by our planet's magnetic field toward the poles where they ionize the atmosphere and interfere with the normal transmission of shortwave radio.
This polar cap absorption event could last for days, especially if it is boosted by more flares from AR3664. You can can monitor its progress here.
https://spaceweather.com/

Giant sunspot AR3664 is no longer facing Earth. That makes it extra dangerous. Right now, the Carrington-class sunspot is passing over the sun's western limb--a region of the sun that is magnetically connected to our planet. Indeed, we are feeling the effects of that connection; take a look at this map of ongoing radio blackouts:

Red zones in the map show where shortwave radio signals are being absorbed. Frequencies below 20 MHz are almost completely blacked out, a nuisance for long-distance aviators and ham radio operators.
What's causing this? Protons accelerated by solar flares in the magnetic canopy of AR3664 are following the Parker Spiral back to Earth. Think of it as a magnetic superhighway. Arriving particles are funneled by our planet's magnetic field toward the poles where they ionize the atmosphere and interfere with the transmission of shortwave radio signals.
This polar cap absorption event could last for days, especially if it is boosted by more flares from AR3664. You can can monitor its progress here.
https://spaceweather.com/

The first of six CMEs hurled toward Earth by giant sunspot AR3664 hit our planet's magnetic field today. The impact on May 10th at 1645 UT jolted magnetometers around the world and sparked a severe (G4-class) geomagnetic storm. This storm is underway now. More CMEs are following close behind and their arrival could extend the storm into the weekend. Sign up for Space Weather Alerts to receive instant text messages when the CMEs arrive.
The ongoing storm is producing low-latitude auroras in the southern hemisphere. Ken James sends this picture from the Snake Valley Observatory in Victoria, Australia:

"The red, yellow and green colours were easily visible to my naked eye," says James.
Readers in the USA should note that the southern latitude of Victoria, Australia, 37 degrees, is the same as the northern latitude of central California. That's how far down auroras could be seen if it were dark instead of daylight in North America.
Why is this storm so severe? Take a look at the solar wind data from NOAA's DSCOVR spacecraft:

After the CME struck, the speed of the solar wind blowing around our planet abruptly increased to more than 700 km/s. More importantly, south-pointing magnetic fields from the sun washed over the Earth, opening a crack in our planet's magnetosphere. Solar wind poured through the gap to turbo-charge the storm.
https://spaceweather.com/

Big sunspot AR3590 is as dangerous as it looks. Late yesterday (Feb. 21 @ 2307 UT), the active region produced a powerful X1.8-class solar flare with a shortwave radio blackout over the western USA and Pacific Ocean. NASA's Solar Dynamics Observatory recorded the extreme ultraviolet flash:

Hours later (Feb. 22 @ 0635), the sunspot erupted again, producing an almost identical X1.7-class flare. Neither explosion produced a bright CME. This means the double flares will *not* cause a geomagnetic storm on Earth.
More explosions are in the offing. AR3590 has an unstable 'beta-gamma-delta' magnetic field that harbors energy for additional X-class explosions.
https://spaceweather.com

NOAA models confirm that a Cannibal CME will strike our planet on Dec. 1st. Cannibal CMEs form when a fast CME sweeps up a slower CME ahead of it. The combination contains intense, tangled magnetic fields that can do a good job sparking auroras when they reach Earth. If a Cannibal CME strikes Earth on Dec. 1st, as predicted, geomagnetic storm levels could reach category G3 (Strong). If so, here's what we can expect. The last G3-class storm on Nov. 5th sparked not only bright auroras, but also deep-red SAR arcs around the world. Greg Redfern photographed this example from the Shenandoah National Park in Virginia:

"I didn't realize I had photographed an SAR arc until I processed my images the next day, stitching two of them together to reveal its shape," says Redfern.
SAR arcs look like auroras, but they are not. They are the glow of heat energy leaking into the upper atmosphere from Earth's ring current system–a donut-shaped circuit carrying millions of amps around our planet. During the Nov. 5th geomagnetic storm, these red arcs were observed as far south as Texas and California.
Auroras were observed as well -- "and they were INSANE," says Janne Maj Nagelsen, who watched the display from Stamnes, Vaksdal, Norway:

"I have never seen such strong auroras," says Nagelsen. "Not to mention the colors. I mean look at the picture! They were totally, literally insane."

Auroras are caused by charged particles raining from space down upon Earth's atmosphere. Unlike SAR arcs, which are pure red, auroras can have a rich and stunning variety of colors. Both phenomena may be photographed on Dec. 1, 2023, when a Cannibal CME is expected to hit Earth.
https://spaceweather.com/

When Vincent van Gogh painted "The Starry Night" in 1889, little did he know he was working at the forefront of 21st century astrophysics. A paper recently published in Nature Communications reveals that the same kind of waves pictured in the famous painting can cause geomagnetic storms on Earth.

Physicists call them "Kelvin Helmholtz waves". They ripple into existence when streams of gas flow past each other at different velocities. Van Gogh saw them in high clouds outside the window of his asylum in Saint-Rémy, France. They also form in space where the solar wind flows around Earth's magnetic field.

"We have found Kelvin-Helmholtz waves rippling down the flanks of Earth's magnetosphere", says Shiva Kavosi of Embry–Riddle Aeronautical University, lead author of the Nature paper. "NASA spacecraft are surfing the waves, and directly measuring their properties".

This was first suspected in the 1950s by theoreticians who made mathematical models of solar wind hitting Earth's magnetic field. However, until recently it was just an idea; there was no proof the waves existed. When Kavosi's team looked at data collected by NASA's THEMIS and MMS spacecraft since 2007, they saw clear evidence of Kelvin Helmholtz instabilities.

"The waves are huge" says Kavosi. "They are 2 to 6 Earth radii in wavelength and as much as 4 Earth radii in amplitude."

Imagine a wave taller than Earth curling over and breaking. That's exactly what happens. Kelvin-Helmholtz waves naturally break onto Earth's magnetic field, propelling energetic particles deep into the magnetosphere. This revs up Earth's radiation belts, triggering geomagnetic storms and auroras.

A key finding of Kavosi's paper is that the waves prefer equinoxes. They appear 3 times more frequently around the start of spring and fall than summer and winter. Researchers have long known that geomagnetic activity is highest around equinoxes. Kelvin-Helmholtz wave activity could be one reason why.

Our planet's seasonal dependence of geomagnetic activity has always been a bit of a puzzle. After all, the sun doesn't know when it's autumn on Earth. One idea holds that, around the time of the equinoxes, Earth's magnetic field links to the sun's because of the tilt of Earth's magnetic poles. This is called the Russell-McPherron effect after the researchers who first described it in 1973. Kavosi's research shows that Kelvin-Helmholtz waves might be important, too.

Northern autumn has just begun, which means Kelvin Helmholtz waves are rippling around our planet, stirring up "Starry Night" auroras. Happy autumn!
www.spaceweather.com

Europeans are still trying to wrap their minds around what happened after sunset on April 23, 2023. Everyone knew that a CME was coming; photographers were already outside waiting for auroras. But when the auroras appeared, they were very strange."I had never seen anything quite like it," says Heiko Ulbricht of Saxony, Germany. "The auroras began to tear themselves apart, pulsating as they formed individual blobs that floated high in the sky."

"It literally took my breath away," he says. "My pulse was still racing hours later!" The same blobs were sighted in France and Poland, and in Denmark they were caught flashing like a disco strobe light.  Ordinary auroras don't act like this.

Indeed, "these were not ordinary auroras," confirms space physicist Toshi Nishimura of Boston University. "They are called 'proton auroras,' and they come from Earth's ring current system."

Most people don't realize that Earth has rings. Unlike Saturn's rings, which are vast disks of glittering ice, Earth's rings are invisible to the naked eye. They are made of electricity--a donut-shaped circuit carrying millions of amps around our planet. The ring current skims the orbits of geosynchronous satellites and plays a huge role in determining the severity of geomagnetic storms.

Sometimes during strong geomagnetic storms, protons rain down from the ring system, causing a secondary shower of electrons, which strike the atmosphere and make auroras. Earth-orbiting satellites have actually seen these protons on their way down. Ordinary auroras, on the other hand, are caused by particles from more distant parts of Earth's magnetosphere and have nothing to do with Earth's ring current.Mystery solved? Not entirely. "We still don't know why proton auroras seem to tear themselves apart in such a dramatic way," says Nishimura. "This is a question for future research."

"It was very exciting to watch," says Ulbricht. "I definitely want to see them again."

Good, because they'll be back. Solar Cycle 25 ramping up to a potentially-strong Solar Maximum next year. Future storms will surely knock more protons loose from the ring current system.

Here's what to look for: (1) Proton auroras tend to appear around sunset. Why? Electric fields in Earth's magnetosphere push the protons toward the dusk not dawn side of our planet. (2) Proton auroras love to pulse--a sign of plasma wave activity in Earth's ring current. (3) Proton auroras are sometimes accompanied by deep red arcs of light (SARs), the glow of heat leaking from the ring current system. These red arcs were also seen on April 23rd.

Solar Max is coming. Let the proton rain begin!
https://spaceweather.com/

Last month, during the late hours of April 23rd, a CME hit Earth's magnetic field. The impact sparked a severe geomagnetic storm with auroras so bright they could be seen as far south as Texas. Invisible to the human eye, something else happened. There was a sudden decrease in cosmic radiation:

In a matter of hours, cosmic rays peppering Earth's atmosphere dropped to their lowest levels since 2015. Neutron monitors in Oulu, Finland, detected the drop, which lasted for days.
This is called a "Forbush decrease," named after American physicist Scott Forbush who studied cosmic rays in the early 20th century.  It happens when a coronal mass ejection (CME) sweeps past Earth and pushes galactic cosmic rays away from our planet. It sounds counterintuitive, but big solar storms can cause sharp decreases in space radiation.
This Forbush decrease is over, but more are in the offing. Solar Max is coming and soon the sun will be hurling many more CMEs in our direction. Their cumulative effect could create a sustained decrease in cosmic radiation, lowering dose rates for astronauts and air travelers. Stay tuned for updates.
https://spaceweather.com/

Cosmic rays reaching Earth just hit a six-year low. Neutron counters in Oulu, Finland, registered the sudden decrease on Dec. 26th when a coronal mass ejection (CME) hit Earth's magnetic field:

The CME swept aside galactic cosmic rays near our planet, abruptly reducing radiation levels. Researchers call this a "Forbush Decrease," after American physicist Scott Forbush, who studied cosmic rays in the early 20th century.
The Dec. 26th event continues a trend that began in 2020. Since then, cosmic ray fluxes have been fitfully decreasing as one CME after another hit Earth. The reason is Solar Cycle 25, which began around that time and has been gaining strength. The Forbush Decreases are adding up.
Scott Forbush was the first to notice the yin-yang relationship between solar activity and cosmic rays. When one goes up, the other goes down. CMEs play a big role in this relationship. The solar storm clouds contain tangled magnetic fields that do a good job scattering cosmic rays away from our planet.
A recent paper in the Astrophysical Journal looked at the last two solar cycles and compared the daily rate of CMEs to the strength of cosmic rays near Earth. This plot shows the results:

At the peak of Solar Cycle 24, the sun was producing more than 5 CMEs per day. At the same time, galactic cosmic rays (GCRs) dropped more than 60%.
Neutron counts are now at their lowest level since 2016. If current trends continue, cosmic ray levels will plunge even further in the years ahead, perhaps even lower than Solar Cycle 24. This is good news for astronauts and polar air travelers who will benefit from less radiation.
FAQ: Why neutrons? When cosmic rays strike Earth’s atmosphere, they produce a spray of secondary particles that rain down on Earth. Among these particles are neutrons, which can make it all the way down to Earth's surface. Researchers at the Sodankyla Geophysical Observatory in Oulu, Finland, have been counting neutrons every day since 1964, providing an unparalleled record of cosmic rays for almost 60 years.
www.spaceweather.com

1,310,462 views 14 Dec 2022
Nikola Tesla: "God Lives Here"
Thank you very much to this wonderful man, Michael Tellinger, who has been a revolutionary for years. Subscribe to his channel: https://www.youtube.com/channel/UCLF2... Visit his website: https://michaeltellinger.com/

September 20, 2021 / Dr.Tony Phillips - NASA

Sept. 24, 2021: No solar storms? No problem. Earth has learned to make its own auroras. New results from NASA’s THEMIS-ARTEMIS spacecraft show that a type of Northern Lights called “diffuse auroras” comes from our own planet – no solar storms required.

Diffuse auroras look a bit like pea soup. They spread across the sky in a dim green haze, sometimes rippling as if stirred by a spoon. They’re not as flamboyant as auroras caused by solar storms. Nevertheless, they are important because they represent a whopping 75% of the energy input into Earth’s upper atmosphere at night. Researchers have been struggling to understand them for decades.

Above: Diffuse auroras and the Big Dipper,
photographed by Emmanuel V. Masongsong in Fairbanks, AK

“We believe we have found the source of these auroras,” says UCLA space physicist Xu Zhang, lead author of papers reporting the results in the Journal of Geophysical Research: Space Physics and Physics of Plasmas.

It is Earth itself.

Earth performs this trick using electron beams. High above our planet’s poles, beams of negatively-charged particles shoot upward into space, accelerated by electric fields in Earth’s magnetosphere. Sounding rockets and satellites discovered the beams decades ago. It turns out, they can power the diffuse auroras.

The video below shows how it works. The beams travel in great arcs through the space near Earth. As they go, they excite ripples in the magnetosphere called Electron Cyclotron Harmonic (ECH) waves. Turn up the volume and listen to the waves recorded by THEMIS-ARTEMIS:

Above: A great electrical circuit in space powering diffuse auroras. ECH waves were sonified by NASA’s HARP (Heliophysics Audified: Resonances in Plasmas) software.

ECH waves, in turn, knock other electrons out of their orbits, forcing them to fall back down onto the atmosphere. This rain of secondary electrons powers the diffuse auroras.

“This is exciting,” says UCLA professor Vassilis Angelopoulos, a co-author of the papers and lead of the THEMIS-ARTEMIS mission. “We have found a totally new way that particle energy can be transferred from Earth’s own atmosphere out to the magnetosphere and back again, creating a giant feedback loop in space.”

According to Angelopoulos, Earth’s polar electron beams1 sometimes weaken but they never completely go away2, not even during periods of low solar activity. This means Earth can make auroras without solar storms.

The sun is currently experiencing periods of quiet as young Solar Cycle 25 sputters to life. Pea soup, anyone?  [Note: Solar Cycle 25 is accelerating.  MS}

End Notes:

(1) Why do these electron beams exist? Earth’s magnetosphere is buzzing with energetic particles. Many of them are captured from the solar wind. When these particles strike the top of Earth’s atmosphere (the ionosphere), they dislodge electrons. Electric fields, which form naturally in Earth’s spinning magnetosphere, grab the liberated electrons and accelerate them skyward in collimated beams.

(2) Why don’t the beams ever go away? Short answer: because the solar wind never stops blowing. Even when the sun is quiet, Earth’s magnetosphere is jostled and energized by the ever-present solar wind. As a result, electrons are always being knocked off the top of Earth’s atmosphere as described in Note #1. Although solar storms are not required for this process, solar storms can help. For instance, when a CME strikes Earth’s magnetosphere, the contents of the magnetosphere become extra-energized. Lots of particles furiously strike the top of Earth’s atmosphere, liberating even more electrons than usual. Earth’s electron beams can thus become super-charged. When the storm subsides, the electron beams may weaken, but they never vanish because even the quiet sun produces solar wind.

References:

Zhang, X., Angelopoulos, V., Artemyev, A. V., Zhang, X.-J. (2021), Beam-driven ECH waves: A parametric study, Phys. Plasmas, 28, 072902, https://doi.org/10.1063/5.0053187

Zhang, X., Angelopoulos, V., Artemyev, A. V., Zhang, X.‐J., Liu, J. (2021). Beam‐driven electron cyclotron harmonic waves in Earth’s magnetotail. Journal of Geophysical Research: Space Physics, 126, e2020JA028743. https://doi.org/10.1029/2020JA028743s

https://spaceweatherarchive.com/2021/09/20/earth-can-makes-its-own-auroras/