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SEVERE GEOMAGNETIC STORM: Forecasters did not see this one coming. On March 23-24, auroras spread into the United States as far south as New Mexico (+32.8N) during a severe (category G4) geomagnetic storm--the most intense in nearly 6 years. The cause of the storm is still unclear; it may have been the ripple effect of a near-miss CME on March 23rd.
"Aurora pillars were visible from Shenandoah National Park in Central Virginia," says Peter Forister, who photographed the light show at latitude +38.7 degrees:

"Beautiful red and green colors were visible to the naked eye around 11 pm local time," he says. Other notable low-latitude sightings were made in Colorado (+38.7N), Missouri (+40.2N), Colorado again (+38.3N), Nebraska (+41N) and North Carolina (+36.2N). More than half of all US states were in range of the display.
Not every light in the sky was the aurora borealis, however. There was also STEVE:

Joseph Shaw photographed the luminous ribbon over Bozeman, Montana. It also appeared over South Dakota, Washington State, Idaho, Montana again, and Scotland.
STEVE (Strong Thermal Emission Velocity Enhancement) looks like an aurora, but it is not. The phenomenon is caused by hot (3000°C) ribbons of gas flowing through Earth’s magnetosphere at speeds exceeding 6 km/s (13,000 mph). These ribbons appear during strong geomagnetic storms, revealing themselves by their soft purple glow.
This remarkable and surprising storm began on March 23rd when magnetic fields in the space around Earth suddenly shifted. In the jargon of space weather forecasting "BsubZ tipped south." South-pointing magnetic fields can open a crack in Earth's magnetosphere and, indeed, that's what happened. Earth's "shields were down" for almost 24 hours, allowing solar wind to penetrate and the storm to build to category G4.
These developments may have been caused the close passage of an unexpected CME. The storm cloud could have left the sun on March 20-21 when SOHO coronagraph data were unusually sparse. We didn't know it was coming. For aurora watchers, it was a welcome surprise. Aurora alerts: SMS Text.
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AMBER BUMBLEBEE SPACE PENDANT: Bumblebees don't usually fly so high. On Oct 15, 2022, the students of Earth to Sky Calculus launched this one to the stratosphere onboard a cosmic ray research balloon. Here it is floating 115,158 feet above California's Sierra Nevada:

You can have it for $179.95. This bee is made of genuine Baltic Amber with a sterling silver exoskeleton. The rich Cognac-colored pendant measures 3/4 inch and comes with a matching 18-inch sterling silver chain.
The students are selling these unique pendants to support their cosmic ray ballooning program. Each one comes with a greeting card showing the bumblebee in flight and telling the story of its trip to the stratosphere and back again.
Far Out Gifts: Earth to Sky Store
All sales support hands-on STEM education
A SOLAR RADIO BURST AT NIGHT: Something rare and strange happened last month. On Feb. 23rd, growing sunspot AR3234 produced an M-class solar flare. It was nearly midnight in Florida when the explosion occurred, so you'd expect no one there to notice. On the contrary, in the community of High Springs, FL, amateur radio astronomer Dave Typinski recorded a strong shortwave radio burst.
"You CAN see the sun at midnight in Florida... sometimes," says Typinski. This is what his instruments recorded while the flare was underway:

A double wave of static washed over Florida, filling the radio spectrum with noise at all frequencies below 25 MHz. "The Sun was 69° below the horizon when this happened," he marvels.
How is this possible? The entire body of our planet was blocking the event from Typinski's antenna. It's called "antipodal focusing." First postulated by Marconi more than 100 years ago, antipodal focusing is a mode of radio propagation in which a signal starts out on one side of the planet, gets trapped between Earth's surface and the ionosphere, and travels to the opposite hemisphere. Waves converging at the antipode can create a surprisingly strong signal.
Right: This diagram from a declassified US Gov.report shows the basic geometry of antipodal focusing.
"This is the second or maybe third midnight solar radio burst I've seen in ten years, but it's by far the strongest," says Typinski. "The previous events happened at the height of Solar Cycle 24. They're quite rare."
Pause: Yes, solar flares can produce radio signals. Typinski's midnight burst was a "Type V," caused by streams of electrons shooting through the sun's atmosphere in the aftermath of the flare. Plasma waves rippling away from the streams emited intense bursts of natural radio static. The burst was first observed in broad daylight at the Learmonth Solar Observatory in Australia, then it curved around Earth to reach Typinski.

Above: An example of antipodal focusing of seismic waves caused by the Chicxulub asteroid impact. The geometry is the same as for radio waves. [more].
"This propagation mode was used during the Cold War," notes Typinski. "The U.S. would park a SIGINT ship in the south Pacific to grab signals from the Eastern Bloc. The Soviets probably did the same thing, parking in the southern Indian ocean."
Turns out, this method of spying works for radio astronomers, too. Would you like to record an event like this? NASA's Radio JOVE program makes it easy. Off-the-shelf radio telescope kits allow even novices to monitor radio outbursts from the sun, which are becoming more frequent as Solar Cycle 25 intensifies.
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