Scientists build a 'mini-sun' at a university campus to study solar wind
It's always sunny in Wisconsin.
Jackson RyanFormer Science Editor
Jackson Ryan was CNET's science editor, and a multiple award-winning one at that. Earlier, he'd been a scientist, but he realized he wasn't very happy sitting at a lab bench all day. Science writing, he realized, was the best job in the world -- it let him tell stories about space, the planet, climate change and the people working at the frontiers of human knowledge. He also owns a lot of ugly Christmas sweaters.
The sun, at about 1.4 million kilometers wide, is a huge ball of plasma at the center of our solar system. We've studied it for millennia, dating back to ancient history, and now we're even sending probes to touch it. One of the most intriguing aspects of the sun is how its magnetic field influences the entire solar system. Researchers at the University of Wisconsin-Madison wanted to better understand this process and so they went full Hollywood mad scientist and built their own "mini-sun."
They've dubbed it the Big Red Ball. The researchers pump in helium gas (which is present in the actual sun) and turn it into plasma. A magnet at the center of the Ball creates a magnetic field and once the team applies an electric current to the machine it accurately mimics how the real sun's plasma and magnetic fields usually operate.
Watch this: NASA's Parker Probe: Everything you need to know about the plan to 'touch the sun'
"Satellite missions have documented pretty well where the fast wind comes from," said Ethan Peterson, lead author on the study and a graduate student at UW-Madison, in a press release. "We were trying to study specifically how the slow solar wind is generated and how it evolves as it travels toward Earth."
They turned their attention toward the solar wind, particles that stream out from the sun and into the solar system. Within the Ball, they were able to recreate the Parker Spiral, the magnetic field that twists out from the sun through the entirety of the solar system. Peterson dubs the team's recreation as a "large-scale map" of the spiral and confirms how it is created by the sun's plasma flows.
In addition, the researchers also identified plasma "burps," which are huge ejections of plasma that stream out of the sun and sometimes fuel the solar wind. With probes inside the Ball monitoring the work, the team could see how they moved and how fast the plasma was spinning.
"These ejections are observed by satellites, but no one knows what drives them," Peterson said. "We ended up seeing very similar burps in our experiment, and identified how they develop."