Interface Region Imaging Spectrograph
The Interface Region Imaging Spectrograph
|Mission type||Solar UV astronomy|
|Mission duration||2 years (planned)|
|Launch mass||183 kg (403 lb)|
|Start of mission|
|Launch date||27 June 2013, 02:27:46UTC|
|Launch site||Stargazer, Vandenberg|
|Semi-major axis||7,016.11 km (4,359.61 mi)|
|Perigee||625 km (388 mi)|
|Apogee||664 km (413 mi)|
|Epoch||29 November 2014, 12:17:18 UTC|
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.
- Science results 1
- IRIS team 2
- References 3
- External links 4
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.
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
- "Interface Region Imaging Spectrograph (IRIS)". NASA. 16 August 2013.
- "IRIS Satellite details 2013-033A NORAD 39197". N2YO. 29 November 2014. Retrieved 30 November 2014.
- Harrington, J. D. (29 May 2008). "NASA Selects Small Explorer Investigations for Concept Studies". NASA.gov.
- Harrington, J. D. (19 June 2009). "NASA Awards Two Small Explorer Development Contracts". NASA.gov.
- Hendrix, Susan; Diller, George (17 April 2013). "NASA'S Newest Solar Satellite Arrives at Vandenberg AFB for Launch". NASA.gov.
- "IRIS Solar Observatory Launches, Begins Mission". NASA.gov. 28 June 2013.
- Fox, Karen C. (25 July 2013). "NASA's IRIS Telescope Offers First Glimpse of Sun's Mysterious Atmosphere". NASA.gov. Retrieved 29 July 2013.
- "Interface Region Imaging Spectrograph". Lockheed Martin Solar and Astrophysics Laboratory.
- De Pontieu, B.; Title, A. M.; Lemen, J.; Kushner, G. D.; Akin, D. J. et al. (July 2014). "The Interface Region Imaging Spectrograph (IRIS)".
- De Pontieu, B.; Rouppe van der Voort, L.; McIntosh, S. W.; Pereira, T. M. D.; Carlsson, M. et al. (October 2014). "On the prevalence of small-scale twist in the solar chromosphere and transition region".
- IRIS website by Lockheed Martin
- IRIS website by NASA