The region located between the surface of the sun and its atmosphere has been revealed as a more violent place than
previously1 understood, according to images and data from NASA's newest solar
observatory2, the
Interface3 Region Imaging Spectrograph, or
IRIS4. Solar
observatories5 look at the sun in layers. By capturing light emitted by atoms of different temperatures, they can focus in on different heights above the sun's surface extending well out into the solar atmosphere, the
corona6(日冕). On June 27, 2013, IRIS, was launched, to study what's known as the interface region -- a layer between the sun's surface and corona that previously was not well observed.
Over its first six months, IRIS has thrilled scientists with
detailed7 images of the interface region, finding even more
turbulence8(动荡) and
complexity9 than expected. IRIS scientists presented the mission's early observations at a press conference at the Fall American Geophysical Union meeting on Dec. 9, 2013.
"The quality of images and
spectra10 we are receiving from IRIS is amazing," said Alan Title, IRIS principal
investigator11 at Lockheed Martin in Palo Alto, Calif. "And we're getting this kind of quality from a smaller, less expensive mission, which took only 44 months to build."
For the first time, IRIS is making it possible to study the explosive
phenomena12 in the interface region in sufficient detail to determine their role in heating the outer solar atmosphere. The mission's observations also open a new window into the
dynamics13 of the low solar atmosphere that play a
pivotal(关键的) role in accelerating the solar wind and driving solar eruptive events.
Tracking the complex processes in the interface region requires instrument and modeling
capabilities14 that are only now within our
technological15 reach. IRIS captures both images and what's known as spectra, which display how much of any given
wavelength16 of light is present. This, in turn, corresponds to how much material in the solar atmosphere is present at specific
velocities17, temperatures and
densities18. IRIS's success is due not only to its high
spatial19 and temporal resolution, but also because of parallel development of advanced computer models. The combined images and spectra have provided new imagery of a region that was always known to be dynamic, but shows it to be even more violent and turbulent than imagined.
"We are seeing rich and
unprecedented20 images of violent events in which gases are accelerated to very high velocities while being rapidly heated to hundreds of thousands of degrees," said Bart De Pontieu, the IRIS science lead at Lockheed Martin. "These types of observations present significant challenges to current theoretical models."