Interface Region Imaging Spectrograph

Not to be confused with Infrared Astronomical Satellite (IRAS).

IRIS

The Interface Region Imaging Spectrograph
Mission type	Solar UV astronomy
Operator	NASA
COSPAR ID	2013-033A
SATCAT №	39197
Mission duration	2 years (planned)
Spacecraft properties
Manufacturer	Lockheed Martin
Launch mass	183 kg (403 lb)
Start of mission
Launch date	27 June 2013, 02:27:46 UTC (2013-06-27UTC02:27:46Z)
Rocket	Pegasus-XL F42
Launch site	Stargazer, Vandenberg
Contractor	Orbital Sciences
Orbital parameters
Reference system	Geocentric
Regime	Sun-synchronous
Semi-major axis	7,015.38 km (4,359.16 mi)
Eccentricity	0.0029478
Perigee	623 km (387 mi)
Apogee	665 km (413 mi)
Inclination	97.90 degrees
Period	97.47 minutes
Epoch	24 January 2015, 02:50:49 UTC
---- Small Explorer program ← NuSTAR GEMS →

The Interface Region Imaging Spectrograph (IRIS) is a NASA solar observation satellite. The mission was funded through the Small Explorer program to investigate the physical conditions of the solar limb, particularly the chromosphere of the Sun. The spacecraft consists of a satellite bus and spectrometer built by the Lockheed Martin Solar and Astrophysics Laboratory (LMSAL), and a telescope provided by the Smithsonian Astrophysical Observatory. IRIS is operated by LMSAL and NASA's Ames Research Center.

The satellite's instrument is a high-frame-rate ultraviolet imaging spectrometer, providing one image per second at 0.3 arcsecond spatial resolution and sub-ångström spectral resolution.

NASA announced on 19 June 2009 that IRIS was selected from six Small Explorer mission candidates for further study, along with the Gravity and Extreme Magnetism (GEMS) space observatory.

The spacecraft arrived at Vandenberg Air Force Base, California, on 16 April 2013 and was successfully launched on 27 June 2013 by a Pegasus-XL rocket.

Science results

In this video, we will look at IRIS data from a solar flare on March 11, 2015.

IRIS achieved first light on 17 July 2013. NASA noted, "IRIS's first images showed a multitude of thin, fibril-like structures that have never been seen before, revealing enormous contrasts in density and temperature occur throughout this region even between neighboring loops that are only a few hundred miles apart." On 31 October 2013, calibrated IRIS data and images were released on the project website. A preprint describing the satellite and initial data has been released on the arXiv.

Data collected from the IRIS spacecraft has shown that the interface region of the sun is significantly more complex than previously known. This includes features described as solar heat bombs, high-speed plasma jets, nano-flares, and mini-tornadoes. These features are an important step in understanding the transfer of heat to the corona.

IRIS team

Science and engineering team members include:

• Lockheed Martin Solar and Astrophysics Lab
• Lockheed Martin Sensing and Exploration Systems
• Smithsonian Astrophysical Observatory
• Montana State University
• Institute for Theoretical Astrophysics, University of Oslo
• High Altitude Observatory, National Center for Atmospheric Research
• Stanford University
• NASA Ames Research Center
• NASA Goddard Space Flight Center
• National Solar Observatory
• Space Sciences Laboratory, University of California, Berkeley
• Princeton Plasma Physics Laboratory
• Sydney Institute for Astronomy, University of Sydney
• Center for Plasma Astrophysics, Catholic University of Leuven
• Mullard Space Science Laboratory
• Rutherford Appleton Laboratory
• European Space Agency
• Max Planck Institute for Solar System Research
• National Astronomical Observatory of Japan
• Niels Bohr Institute, University of Copenhagen

External links

• IRIS website by Lockheed Martin
• IRIS website by NASA

Template:Explorer program