tiny-solar-flares-may-explain-the-suns-ridiculously-hot-atmosphere

Tiny solar flares may explain the sun’s ridiculously hot atmosphere

New evidence suggests tiny solar flares heat the sun’s atmosphere to thousands of times the temperature of its surface.

Small loops of super hot plasma may underlie a mysterious feature of the sun: It’s outer atmosphere, or corona, is far hotter than its visible surface, called the photosphere. NASA recently announced the best evidence so far that nanoflares exist. These solar flares so small they aren’t detectable from Earth. The study results were published Oct. 9 in Nature Astronomy.

“If you’ve got a stove and you take your hand farther away, you don’t expect to feel hotter than when you were close,” coauthor Lindsay Glesener, experiment’s project manager at the University of Minnesota, said in the NASA statement.

The photosphere is a toasty 10,000 degrees Fahrenheit (5,500 degrees Celsius). However, the corona is regularly 1.8 million to 3.6 million degrees Fahrenheit (1 million to 2 million degrees Celsius), and can even climb to 72 million degrees Fahrenheit (40 million degrees Celsius).  The coronal heating problem has confounded scientists for years.

Astrophysicist think that tiny solar flares could be transferring energy from within the sun, through the photosphere, and releasing it as heat in the corona. Since the sun is far hotter than Earth, it’s magnetic field is far more dynamic. The flares, which are coils of plasma, follow the sun’s magnetic field, twisting and snapping as the field changes. This has the potential to transfer immense amounts of energy through the sun’s surface, and discharge it only in the corona. Collectively, these nanoflares could account for the corona’s million degree temperatures, according to the statement.

To test for these nanoflares, scientists launched the FOXSI instrument, short for Focusing Optics X-ray Solar Imager, on a 15-minute flight. The experiment—a collaboration between NASA, the Japan Aerospace Exploration Agency (JAXA), UC Berkeley and University of Minnesota—uses mirrors to detect very faint X-ray signals coming from the sun. These short missions don’t need to be sent into orbit; they just need to make it to space. NASA sends them up on small sounding rockets, and after a few minutes in space, they fall back to Earth, deploy their parachute, and make a soft landing.

Prev1 of 2Next

Leave a Reply

Your email address will not be published. Required fields are marked *