Email Print Share
August 3, 2017

The Daniel K. Inouye Solar Telescope will be observing the sun's corona, or outer atmosphere.

The Daniel K. Inouye Solar Telescope (DKIST) is under construction on the summit of Haleakalā on Maui, Hawaii. The site was chosen out of a world-wide search due to the exceptional "coronal sky." Since DKIST will be observing the sun’s corona, or outer atmosphere, the sky above the telescope needs to be as free of dust, aerosols and pollutants as possible. The isolated islands of Hawaii provide optimal conditions for clear, coronal skies. DKIST is funded by the National Science Foundation and operated by the National Solar Observatory.

Credit: NSO/AURA/NSF


Images credited to the National Science Foundation, a federal agency, are in the public domain. The images were created by employees of the United States Government as part of their official duties or prepared by contractors as "works for hire" for NSF. You may freely use NSF-credited images and, at your discretion, credit NSF with a "Courtesy: National Science Foundation" notation.

Additional information about general usage can be found in Conditions.

Also Available:
Download the high-resolution JPG version of the image. (10.5 MB)

Use your mouse to right-click (Mac users may need to Ctrl-click) the link above and choose the option that will save the file or target to your computer.

Related story: Primary mirror delivered to Daniel K. Inouye Solar Telescope