Interface Region Imaging Spectrograph

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 angular 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.

• Name — Interface Region Imaging Spectrograph • Names List — Explorer 94 IRIS SMEX-12 • Mission Type — Heliophysics • Operator — NASA / Lockheed Martin • Cospar Id — 2013-033A • Satcat — 39197 • Mission Duration — 2 years (planned) 27 June 2013 02:27:46 (in progress) • Spacecraft — Explorer XCIV • Spacecraft Type — Interface Region Imaging Spectrograph • Spacecraft Bus — IRIS • Manufacturer — Lockheed Martin • Launch Date — 28 June 2013, 02:27:46 UTC • Launch Rocket — Pegasus-XL (F42) • Launch Site — Vandenberg, Stargazer • Launch Contractor — Orbital Sciences Corporation • Orbit Reference — Geocentric orbit • Orbit Regime — Sun-synchronous orbit • Orbit Inclination — 97.90° • Orbit Period — 97.47 minutes • Apsis — gee • Instruments — Interface Region Imaging Spectrograph (IRIS) • Programme — Explorer program • Previous Mission — NuSTAR (Explorer 93) • Next Mission — GEMS (Explorer)

IRIS is intended to advance Sun-Earth connection studies by tracing the flow of energy and plasma into the corona and heliosphere for which no suitable observations exist. To achieve this IRIS obtains a high-resolution UV spectra and images of the Sun's chromosphere, specifically on the non-thermal energy that creates the corona and the solar wind. IRIS seeks to determine: (1) the types of non-thermal energy which dominate in the chromosphere and beyond; (2) the means by which the chromosphere regulates mass and energy supply to the corona and heliosphere; and, (3) how magnetic flux and matter rise through the lower solar atmosphere, and the role played by flux emergence in flares and mass ejections. To answer these questions, IRIS utilize a single instrument, a multi-channel imaging spectrograph.

The spacecraft arrived at Vandenberg Air Force Base, California, on 16 April 2013 and was successfully deployed from an Orbital L-1011 carrier aircraft flying over the Pacific Ocean at an altitude of, roughly northwest of Vandenberg. The launch vehicle was dropped at 02:27:46 UTC on 28 June 2013 (7:27 p.m. PDT on 27 June 2013) by a Pegasus-XL launch vehicle.

The IRIS instrument is a multi-channel imaging spectrograph with a ultraviolet telescope. IRIS obtains a spectra along a slit (1/3 arcsecond wide), and slit-jaw images. The charge-coupled device (CCD) detectors has 1/6 arcsecond pixels. IRIS will have an effective spatial resolution between 0.33 and 0.40 arcsecond and a maximum field of view (FoV) of 120 arcseconds. The far-ultraviolet channel covers 133.2-135.8 nm and 139.0-140.6 nm with an 0.04 nm resolution and an effective area of. The near-ultraviolet channel covers 278.5-283.5 nm with an 0.08 nm resolution and an effective area of. Slit-jaw imaging has four passbands: 133.5 nm and 140.0 nm with a 4 nm bandpass each; and 279.6 nm and 283.1 nm with a 0.4 nm bandpass each. IRIS has a high data rate (0.7 Mbit/s on average) so that the baseline cadence is 5 seconds for slit-jaw images and 1 second for six spectral windows, including rapid rastering to map solar regions.

IRIS achieved first light on 17 July 2013. NASA noted that "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. An open-access article describing the satellite and initial data was published in the journal Solar Physics. Data collected from the IRIS spacecraft has shown that the interface region of the Sun is significantly more complex than previously thought. 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. In 2019, IRIS detected tadpole like jets coming out from the Sun according to NASA. • Illustration — Video of IRIS data from a solar flare on 11 March 2015 • Illustration — X-class solar flare on Sept. 10, 2014 • Illustration — IRIS captured several large solar prominences on the edge of the Sun • Illustration — IRIS view above the Sun's surface extending well out into the solar atmosphere

Science and engineering team members include: • Lockheed Martin Solar and Astrophysics Laboratory • 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