Sun  ID: 13691

NASA’s IRIS spots Nanojets: Shining light on heating the solar corona

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 Sept. 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.
 

Source Material


Credits

Scientist:
Patrick Antolin (Northumbria University)

Data Visualizer:
Tom Bridgman (GST)

Producer:
Joy Ng (USRA)

Writer:
Susannah Darling (ADNET)

Please give credit for this item to:
NASA's Goddard Space Flight Center

Short URL to share this page:
https://svs.gsfc.nasa.gov/13691

Mission:
IRIS: Interface Region Imaging Spectrograph

Keywords:
NASA Science >> Sun
SVS >> IRIS Mission
SVS >> Nanoflare
SVS >> Coronal Heating