Rare 'polar rain' aurora seen from Earth for the first time
An eerie green glow formed during Christmas 2022, and now scientists know why.
A remarkably smooth and puzzling Christmas Day aurora observed over the Arctic in 2022 was the result of a 'rainstorm' of electrons direct from the sun, says Japanese and US-based researchers.
It is the first time that a rare aurora of this kind has been seen from the ground, and it came at a time when the gusts of the solar wind had almost completely dropped off, leaving a region of calm around the Earth.
Normally the aurora displays, like the ones seen around the world in May, move and pulsate, with clearly discernible shapes in the sky. These auroral displays are powered by electrons from the solar wind — a stream of charged particles that flow from the sun — that become trapped in an extension of Earth's magnetic field called the magnetotail. When space weather becomes extreme, such as when a coronal mass ejection (CME) — a large ejection of plasma and magnetic field from the sun— is released, the magnetotail can be pinched off (don't worry, it regrows). The electrons trapped there flow down Earth's magnetic field lines to the poles. As they do so, they encounter molecules in Earth's atmosphere, colliding with them and prompting them to glow in the colors of the aurora (blue for nitrogen emission, green or red for oxygen depending on its altitude).
However, the smooth aurora of 25–26 December 2022 was very different. Imaged by an All-Sky Electron Multiplying Charge-Coupled Device (EMCCD) camera in Longyearbyen in Norway, the aurora was a faint, featureless glow that spanned 2,485 miles (4,000 kilometers) in extent. It had no structure, no pulsing or varying brightness. No type of aurora like it had ever been seen from Earth before. . . .
The satellites saw the aurora from above, finding that it had all the hallmarks of a rare type of aurora called polar rain aurora, which had only ever been seen from space before.
The regular solar wind travels about 250 miles (400 km) per second. However, the sun's hot corona is full of holes, particularly at higher solar latitudes from which an exceptionally 'fast' solar wind moving up to 500 miles (800 km) per second streams out. Sometimes these coronal holes can appear at lower latitudes, and that is what happened over Christmas of 2022 while coinciding with a cessation of the regular solar wind.
At the location of coronal holes, the sun's magnetic field lines are open — they don't loop back onto the sun's surface, the photosphere. As the open magnetic field lines extend out into space the coronal hole forms the base of a magnetic funnel out of which stream high-energy electrons.
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