IRIS and Hinode: A Stellar research team
Tuesday, August 25, 2015 - 17:00
in Astronomy & Space
Modern telescopes and satellites have helped us measure the blazing hot temperatures of the sun from afar. Mostly the temperatures follow a clear pattern: The sun produces energy by fusing hydrogen in its core, so the layers surrounding the core generally get cooler as you move outwards—with one exception. Two NASA missions have just made a significant step towards understanding why the corona—the outermost, wispy layer of the sun's atmosphere —is hundreds of times hotter than the lower photosphere, which is the sun's visible surface.