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Interface Region Imaging Spectrograph

IRIS is a NASA Small Explorer solar observatory that combines ultraviolet imaging and spectroscopy to resolve the Sun's chromosphere and transition region. Its measurements trace how plasma, magnetic fields, and energy move through the lower solar atmosphere, addressing how the corona is heated and how the solar wind and eruptive activity are powered.

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Identity

Aliases
IRISExplorer 942013-033A
Name
Interface Region Imaging Spectrograph
Slug
interface-region-imaging-spectrograph
Status
active

Details

Astronauts
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Description
IRIS is a NASA Small Explorer solar observatory that combines ultraviolet imaging and spectroscopy to resolve the Sun's chromosphere and transition region. Its measurements trace how plasma, magnetic fields, and energy move through the lower solar atmosphere, addressing how the corona is heated and how the solar wind and eruptive activity are powered.
Launch Site
Outcome
IRIS entered its planned Sun-synchronous low Earth orbit and began science observations in July 2013. It completed its two-year prime mission and continues extended operations, producing high-resolution spectra and images that reveal fine structure, rapid heating, and mass and energy transport in the Sun's interface region.
Program
Small Explorer
Start Date
2013-06-27
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Assets & Meta

Creation Time
July 18, 2026 at 18:11:10 UTC
Updated Time
July 18, 2026 at 18:11:10 UTC

Other

Affiliations
Space Stations
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Vehicles
Interface Region Imaging Spectrograph - AeroVia