OrbitalHub

NASA dicit:

In pursuit of understanding why the Sun’s atmosphere is so much hotter than the surface, and to help differentiate between a host of theories about what causes this heating, researchers turn to NASA’s Interface Region Imaging Spectrograph (IRIS) mission. IRIS was finely tuned with a high-resolution imager to zoom in on specific hard-to-see events on the Sun.

A paper published in Nature on September 21, 2020, reports on the first ever clear images of nanojets — bright, thin lights that travel perpendicular to magnetic structures in the solar atmosphere called the corona — in a process that reveals the existence of one of the potential coronal heating candidates: nanoflares.

Video credit: NASA’s Goddard Space Flight Center/Scientific Visualization Studio/Scientist: Patrick Antolin (Northumbria University)/Data Visualizer: Tom Bridgman (GST)/Producer: Joy Ng (USRA)/Writer: Susannah Darling (ADNET)

NASA dixit:

“At any given moment, as many as 10 million wild jets of solar material burst from the sun’s surface. They erupt as fast as 60 miles per second, and can reach lengths of 6,000 miles before collapsing. These are spicules, and despite their grass-like abundance, scientists didn’t understand how they form. Now, for the first time, a computer simulation — so detailed it took a full year to run — shows how spicules form, helping scientists understand how spicules can break free of the sun’s surface and surge upward so quickly.

This work relied upon high-cadence observations from NASA’s Interface Region Imaging Spectrograph, or IRIS, and the Swedish 1-meter Solar Telescope in La Palma. Together, the spacecraft and telescope peer into the lower layers of the sun’s atmosphere, known as the interface region, where spicules form.”

Music credit: ‘Solar Dust’ by Laurent Levesque [SACEM], ‘Games Show Sphere 05’ by Anselm Kreuzer [GEMA] from Killer Tracks

Video credit: NASA’s Goddard Space Flight Center/CI Lab