Sept. 24, 2021: Lightning on Earth is getting weirder and weirder. On the evening of Sept. 20th, Puerto Rican photographer Frankie Lucena pointed his Sony A7s camera at an offshore electrical storm. This is what he saw:

“This Gigantic Jet plasma event occurred over a very powerful thunderstorm near the Virgin Islands just ahead of Tropical Storm Peter,” says Lucena.  “I can’t believe I was able to capture such amazing details.”

Indeed, this is one of the best-ever photos of a Gigantic Jet. Sometimes called “Earth’s tallest lightning” because they reach the ionosphere more than 50 miles high, the towering forms were discovered near Taiwan and Puerto Rico in 2001-2002. Since then, only dozens of Gigantic Jets have been photographed. They seem to love storms over water and are famous for surprising passengers onboard commercial aircraft. 

In 2017 and 2018, lightning researcher Oscar van der Velde of the Universitat Politècnica de Catalunya set up high speed cameras on the northern coast of Colombia in a dedicated campaign to capture Gigantic Jets. In three months of observing time he managed to capture only 12. That’s how elusive they are.

“Frankie has photographed a rare Gigantic Jet with ‘carrot’ morphology, first reported by Su et al (2003),” notes van der Velde. “The other, more common type of jet has a ‘tree’ morphology.” Here is a comparison: trees vs. carrots.

“Carrot jets” are remarkable for their internal beads–that is, bright balls of light hundreds of meters wide. Lucena caught dozens of them illuminating the jet’s midsection. They might be places where streamers inside the jet are intersecting, or regions of enhanced heating.

“We don’t know,” says van der Velde. “Gigantic Jets are not easily placed in front of a spectrograph.”

Meanwhile, Lucena is still marveling at what happened. “This is the brightest Gigantic Jet I have ever seen. It was truly remarkable.”

https://spaceweatherarchive.com/2021/09/26/a-gigantic-jet-with-fireballs/

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/

This could be NASA's most exciting mission--ever. The space agency announced yesterday that they will send a heliocopter to Titan, Saturn's largest moon. Titan is in many ways more like Earth than any other place in the solar system. It has rivers and lakes, a thick atmosphere, and organic compounds that could support the genesis of life. The quad-chopper, named "Dragonfly," will fly between sites on interest, covering more than twice the distance of every Mars rover combined. Get the full story from nasa.gov.
www.spaceweather.com

MIT Technology Review; Fri, 21 Jun 2019 18:43 UTC

The Tibetan Plateau is a vast elevated plain almost five kilometers above sea level, sometimes called the Roof of the World. It is bordered to the south by the world's highest mountain range and to the north by desert lands. It is one of the most isolated places on Earth.

But the extreme altitude makes it a useful place for scientists. In 1990, they built an observatory here to study the showers of subatomic particles that rain down from the upper atmosphere whenever it is hit by a high-energy cosmic ray. This work is better done at high altitude because there is less atmosphere to absorb the particles.

Since then, the so-called Tibet Air Shower Array has recorded vast numbers of high-energy cosmic rays, particles accelerated to huge energies by astrophysical phenomena such as supernovas, active galactic nuclei, and mysterious as-yet-unidentified sources.

But the array also picks up air showers caused by a different source - high-energy photons. These mysterious photons are also created by astrophysical phenomena such as the interaction between high-energy particles and the cosmic microwave background. Consequently, they can provide a unique insight into these processes and the environments in which they occur.

Over the years, the Tibet Air Shower Array has spotted plenty of these photons with energies up to dozens of teraelectronvolts (TeV 1012). That's roughly equivalent to the highest-energy photons that can be created on Earth. But nobody has ever observed more powerful photons.

Until now. Today, researchers from the Tibet Air Shower Gamma Collaboration say they have observed photons with energies above 100 TeV for the first time, including a remarkable photon with an energy of almost 500 TeV. This single photon has about the same energy as a falling Ping-Pong ball and is the highest-energy photon ever recorded.

The collaboration has also worked out where these photons are coming from: the Crab Nebula, the remnants of a supernova that occurred in 1054 AD in the Perseus Arm of the Milky Way, some 6,500 light-years from Earth.

.... read more at https://www.sott.net/article/415559-Earth-hit-by-highest-energy-photons-ever-recorded-from-the-Crab-Nebula

NASA has clocked up numerous amazing technological feats of engineering and ingenuity for decades, but a recent video from the space agency shows just how much work they have cut out for them.

In just the last few years, NASA has provided some incredible perspectives on our own planet, including stunning images of some of the Earth's most majestic natural phenomena.

Not content with studying our own backyard, the agency has beamed back photos and videos from Mars thanks to its now-deceased rover, not to mention orbiting far-flung asteroids to try and understand the origins of the universe itself.

In an attempt to explain the vastness of their field of study, NASA helpfully put together a short explainer video showcasing the mindblowing scale of the Milky Way galaxy.

Friday night (April 5th) in Norway, researchers at the Andøya Space Center launched two sounding rockets into a minor geomagnetic storm. The results were out of this world. Aurora tour guide Kim Hartviksen photographed glowing blobs of blue and purple caused by the rockets dumping chemical powders into the storm:

"Residents for hundreds of miles were taken by surprise by these strange lights, which prompted calls to the police and 'The aliens are coming!' hysteria!" says Chris Nation who runs the Aurora Addicts guiding service.

When the night began, Nation, Hartviksen, and their clients were treated to a display of auroras, ignited by a stream of solar wind buffeting Earth's magnetic field. "As the auroras started to ebb away, our friends at Andøya launched their rockets into the fading lights," says Nation. "The show began anew as the rockets released their payload into the upper atmosphere."

An automated webcam operated by Chad Blakely of Lights over Lapland in Abisko, Sweden, caught the first puffs of powder emerging from the rockets. "It looked like an invasion of UFOs," says Blakley.

"Soon the glowing blobs evolved into more complicated structures--like two giant squid dancing in the northern sky with an impressive aurora display as its backdrop," decribes Blakley. "Our webcam has been taking a picture every five minutes for nearly 10 years. These images are by far the most exciting I've ever seen it record."

The name of the sounding rocket mission is AZURE--short for Auroral Zone Upwelling Rocket Experiment. Its goal is to measure winds and currents in the ionosphere, a electrically-charged layer of the Earth's atmosphere where auroras appear. Specifically, the researchers are interested in discovering how auroral energy might percolate down toward Earth to influence the lower atmosphere.

The twin rockets deployed two chemical tracers: trimethyl aluminum (TMA) and a barium/strontium mixture. These mixtures create colorful clouds that allow researchers to visually track the flow of neutral and charged particles, respectively. According to NASA, which funded the mission, the chemicals pose no hazard to residents in the region.

Update--a movie! "Here is my realtime video of the surprise rocket launch last night from NASA/ASC," reports Ole Salomonsen of Tromsø, Norway. "I was shocked when I saw this in the night sky facing north, I was not aware of the launch.
www.spaceweather.com

When a stream of solar wind hits Earth's magnetic field, magnetometers around the Arctic Circle normally go a bit haywire, with their needles swinging chaotically as the buffeting ensues. Rob Stammes of the Polarlightcenter, a magnetic observatory in Norway, sees such disordered behavior all the time. But on Nov. 18th something quite different happened. The solar wind produced a pure sine wave:

"A very stable ~15 second magnetic oscillation appeared in my recordings, and lasted for several hours," he says. "The magnetic field was swinging back and forth by 0.06 degrees, peak to peak."
Imagine blowing across a piece of paper, making it flutter with your breath. The solar wind can have a similar effect Earth's magnetic field. The waves Stammes recorded are essentially flutters propagating down the flanks of our planet's magnetosphere excited by the breath of the sun. Researchers call them "pulsations continuous" -- or "Pc" for short..
"A sensitive magnetometer is required to record these waves," says Stammes. "I use a mechanical magnetometer with bar magnets suspended from a special wire. LEDs and light detectors in an isolated dark box record the motion of the magnets, while vanes in oil damp out non-magnetic interference."
Pc waves are classified into 5 types depending on their period. The Nov. 18th waves fall into category Pc3. Researchers have found that Pc3 waves sometimes flow around Earth's magnetic field and cause a "tearing instability" in our planet's magnetic tail. This, in turn, sets the stage for an explosion as magnetic fields in the tail reconnect.

A quartet of NASA spacecraft recently flew through just such an explosion. Last week, researchers from the University of New Hampshire reported that four Magnetospheric Multiscale (MMS) spacecraft spent several seconds inside a magnetic reconnection event as they were orbiting through Earth's magnetic tail. Sensors on the spacecraft recorded jets of high energy particles emerging from the blast site. One jet was aimed squarely at Earth and probably sparked auroras when it hit the upper atmosphere.
Stammes has recorded many Pc waves in the past, "but this is the first time I have detected category Pc3," he says. "This was a very rare episode indeed."
www.spaceweather.com

Laura Geggel; Live Science; Wed, 07 Nov 2018 09:34 UTC

An eerie, marmalade-colored light show made Earth look like a gigantic orange lollipop, prompting an astronaut aboard the International Space Station to snap a photo of it on Oct. 7. And yesterday, NASA shared the glorious shot with Earthlings down below.

The enveloping orange hue is known as airglow - a mesmerizing luminescence caused by chemical reactions high in Earth's atmosphere, NASA reported. This ghostly glow usually happens when ultraviolet radiation from sunlight energizes molecules of nitrogen, oxygen, sodium and ozone in the atmosphere. These energized molecules then bump into each other and lose energy as they collide, resulting in a faint but spectacular afterglow, NASA said.

Airglow is best seen at night, as it's 1 billion times fainter than sunlight, NASA said. This particular photo was taken at an altitude of more than 250 miles (about 400 kilometers) above Australia.

The radiating blush, also known as chemiluminescence, is comparable to glowing chemical reactions here on Earth, including those seen in children's toys such as glow sticks and glow-in-the-dark silly putty, NASA added.

But airglow is more than an entrancing light attraction. It can also teach scientists about the workings of the upper atmosphere. For instance, it can shed light on how particles near the interface of Earth and space move, including how space weather and Earth weather are connected, NASA said.

Researchers are already using satellites - such as NASA's Ionospheric Connection Explorer (ICON) - to study this dynamic zone.

Although this airglow emanated orange, the phenomenon isn't always the color of the snack food Doritos. In 2016, a photographer in the Azores islands in the Atlantic Ocean took a photo of a rainbow-colored airglow, according to Space.com, a sister site of Live Science.

The Parker Solar Probe has just radioed NASA with good news. The spacecraft survived its close approach to the sun on Nov. 5th. Because the sun is a giant natural source of broadband radio noise, Parker cannot transmit complicated data streams through the interference. Images and data won't arrive until early December when the probe has reached a sufficient distance from the sun again. For now, mission controllers are happy to have received a simple beacon saying the spacecraft is okay.

Earlier this week, Parker screamed around the sun at 213,200 mph only 15 million miles from the stellar surface--shattering old records for both speed and distance. Intense sunlight raised the temperature of the probe's heat shield to about 820 degrees Fahrenheit. All the while, instruments and systems behind the shield kept cool in the mid-80s F.

Mission controllers at the Johns Hopkins University Applied Physics Lab received the status beacon at 4:46 p.m. EST on Nov. 7, 2018. It indicated, simply, "A" — the best of all four possible status signals, meaning that the probe is operating well with all instruments running and collecting science data and, if there were any minor issues, they were resolved autonomously by the spacecraft. Stay tuned for "first light" science results about one month from now.
www.spaceweather.com

NASA's Parker Solar Probe is now closer to the sun than any other spacecraft in history, shattering the previous record of 26.6 million miles set by the Helios 2 spacecraft in 1976. The probe is now well inside the orbit of Mercury."It's a proud moment for our team," says Project Manager Andy Driesman of the Johns Hopkins Applied Physics Laboratory.

Count to 3. Parker just broke the record again. The spacecraft is accelerating sunward for the mission's first perihelion on Nov. 5th. At closest approach, the solar disk will seem 6 times wider than it does on Earth as the probe is hit by "brutal heat and radiation" (NASA's words). Parker's carbon-composite heat shield is expected to heat up to a sizzling 2000 deg. F.
Parker's prime mission is to investigate the origin of the solar wind--a project best done uncomfortably close to the star. Parker will trace the solar wind back to its source and find out how it escapes the sun's gravity and magnetic confinement.
Russell Howard of the Naval Research Laboratory expects to learn a lot from this encounter. "We might detect magnetic islands in the solar wind, which have been theoretically predicted. And if a CME (solar explosion) happens or a comet passes through the sun's atmosphere while we are so nearby, it could be spectacular."

Howard is the principal investigator for WISPR, the probe's wide-field camera system. WISPR can actually see the solar wind, allowing it to image clouds and shock waves as they approach and pass the spacecraft. Other sensors on the spacecraft will sample the structures that WISPR sees, making measurements of particles and fields that researchers can use to test competing theories.
"We lose communication with the spacecraft during the perihelion period which begins next week," notes Howard. "This is because there isn't sufficient power to drive both the instruments and the transmitter. The first dump of data will occur in early December." Stay tuned for that.
Parker will plunge toward the sun 24 more times in the next 8 years, breaking many records en route. Here's the timeline.
www.spaceweather.com

The sun is entering a deep Solar Minimum, and Earth's upper atmosphere is responding. Data from NASA's TIMED satellite show that the thermosphere (the uppermost layer of air around our planet) is cooling and shrinking, literally decreasing the radius of the atmosphere. If current trends continue, the thermosphere could set a Space Age record for cold in the months ahead: Full story.
www.spaceweather.co

NASA's Cassini spacecraft captured an incredible final image of Earth from 1.4 billion km away during its orbit of Saturn's rings.  The space probe was facing Earth's Southern Atlantic Ocean, some 870 million miles (1.4 billion km) away, when the image of earth was captured on April 12, says NASA.

In a zoomed-in version of the image, Earth's moon is also clearly visible, seeming to float alongside our bright planet in the dark vastness of space.

The image marks Cassini's last view of Earth as the spacecraft prepares to end its mission by dramatically plunging into Saturn's atmosphere on September 15.  The probe's 'Grand Finale' mission begins on Friday when the spacecraft will complete a close flyby of Saturn's moon, Titan - passing a mere 600 miles above its surface - before beginning its final set of 22 orbits between Saturn and its rings.

Cassini, a $3.2 billion mission from NASA, the European Space Agency (ESA) and the Italian Space Agency, launched in 1997 and has delivered unprecedented data of Saturn and its moons.
You can see video from the mission here.

In a surprising development, NASA has regained contact with the STEREO-B spacecraft after two years of silence. STEREO-B, which can see the farside of the sun, went quiet in 2014 after mission controllers tested a communications reset procedure. Unfortunately, STEREO-B failed the test. Since then, NASA has regularly attempted to regain contact using the Deep Space Network. On Aug. 21st, they succeeded, managing to receive a downlink carrier for several hours. In the days and weeks ahead, engineers will take steps to assess the health of STEREO-B and return it to service.
www.spaceweather.com

NASA is advising the world to pack up and go hiking on the night of August 11-12 to watch a spectacular shooting star show, as the annual Perseid meteor shower is forecast to beat all records this year.

"Forecasters are predicting a Perseid outburst this year with double normal rates on the night of August 11-12," Bill Cooke, from NASA's Meteoroid Environments Office in Huntsville, Alabama, said on Tuesday. Cooke noted that under perfect conditions, we will be treated to up to 200 meteors every hour.

The "outburst" the NASA man is referring to means this year's cosmic dance is set to be far more crowded than usual. The last time the event happened on such a scale was 2009.

The Perseid meteor shower wows spectators with its swift and extremely bright meteors, traveling at a speed of 60km per second. A Perseid meteor is a small piece of debris left in the wake of the ancient Swift-Tuttle comet, which orbits the sun every 133 years. Despite these visits into the inner solar system being so rare, each of them gives off trillions of comet particles. When Earth passes through this trail of debris, the particles enter the planet's atmosphere and break up in bright specs of light.

From down here they seem to fly from the direction of the Perseus constellation, leading to the meteors being given the name "Perseids."

"Here's something to think about: The meteors you'll see this year are from comet flybys that occurred hundreds if not thousands of years ago. And they've traveled billions of miles before their kamikaze run into Earth's atmosphere," Cooke says.

Earth flies through the trail of these comet particles every August, usually grazing the edge of the debris stream. But its trajectory shifts somewhat every now and then thanks to Jupiter's gravity pull, and according to NASA experts this year our planet may be getting a seat in the front row, flying closer to the middle, where there are more particles. In fact, they claim that three or more debris trails will cross paths with Earth in but a few days.

According to NASA, the best opportunity to watch the Perseids will be between midnight and dawn on the morning of August 12. If you're not all that into getting out in the fresh air, the agency has also promised a live broadcast of the shooting star display on its Ustream channel starting at 2am GMT.

The Perseids are no danger to Earth, as even the largest ones mostly burn up in its atmosphere some 80km above the planet's surface. But the outburst could still land spacecraft in a spot of trouble: the bigger particles are capable of causing minor damage to the hulls of rockets and satellites.

Let's hope for the best though, and get the binoculars ready.

There's a new room on the International Space Station. NASA inflated it Saturday. The Bigelow Expandable Activity Module (BEAM) was filled with air by astronaut Jeff Williams as the ISS flew over the south Pacific, kicking off an experiment to learn how inflatable habitats perform in a microgravity environment. "I think I am the first amateur astronomer to photograph BEAM from Earth," says Philip Smith, who sends these before-and-after images from Manorville, New York:

"Using a backyard telescope, I tracked the ISS as it passed overhead on May 26th (before inflation) and May 28th (after)," says Smith. "The new addition was clearly visible in my images."

"The Bigelow Aerospace-built BEAM is a prototype space habitat for future space stations, moon colonies and moon bases," he adds. "I am glad to be a small part of that history."
BEAM will remain attached to station for a two-year test period. Astronauts will not occupy the new room, but they will enter from time to time and monitor its performance. For more information about BEAM, visit: www.nasa.gov/beam.                 www.spaceweather.com