Jump to content

Daniel K. Inouye Solar Telescope: Difference between revisions

Coordinates: 20°42′24″N 156°15′22″W / 20.7068°N 156.2561°W / 20.7068; -156.2561
From Wikipedia, the free encyclopedia
No edit summary
Ender8282 (talk | contribs)
m Ender8282 moved page Advanced Technology Solar Telescope to Daniel K. Inouye Solar Telescope: As noted on talk page the telsecope has changed is name
(No difference)

Revision as of 21:25, 25 April 2014

Daniel K. Inouye Solar Telescope (DKIST)
Alternative namesDKIST Edit this at Wikidata
Named afterDaniel Inouye Edit this on Wikidata
Part ofHaleakalā Observatory Edit this on Wikidata
Location(s)Haleakalā Observatory, Haleakalā, Maui County, Hawaii
Coordinates20°42′24″N 156°15′22″W / 20.7068°N 156.2561°W / 20.7068; -156.2561
OrganizationNSO, HAO, NJIT, UH IfA and UChicago
Wavelength300nm – 12µm
First lightDecember 2019 Edit this on Wikidata
Telescope styleOff-axis, all-reflecting Gregorian telescope
Diameter400 cm
Illuminated diameter4 m (13 ft 1 in) Edit this at Wikidata
Angular resolution0.023 arcsec at 400 nm
MountingAlt-az
Websitehttp://dkist.nso.edu/
Daniel K. Inouye Solar Telescope is located in the United States
Daniel K. Inouye Solar Telescope
Location of Daniel K. Inouye Solar Telescope (DKIST)
  Related media on Commons

The Daniel K. Inouye Solar Telescope (DKIST), formerly Advanced Technology Solar Telescope (ATST), is a large domed[1] solar telescope facility that is under construction[2] by the National Solar Observatory atop the Haleakala volcano on the Pacific island of Maui. The telescope was officially named after Daniel K. Inouye on Dec 15, 2013.

DKIST features an off-axis, clear aperture design to allow for observations with unprecedented spatial, spectral and temporal resolution. Avoiding a central obstruction is important to minimize scattered light when observing the faint solar corona, but it also eases operation of adaptive optics and post-facto image reconstruction such as speckle imaging.

The site on Haleakala was selected for its clear daytime atmospheric seeing conditions, which will enable study of the solar corona. The DKIST enclosure will house a 4-meter diameter solar telescope capable of observing objects on the Sun that are 30 km across.

Work on the telescope housing was reported complete in September, 2013.[3]

References

  1. ^ "ATST Schematic". Archived from the original on 1 February 2009. Retrieved 2009-02-12. {{cite web}}: Unknown parameter |deadurl= ignored (|url-status= suggested) (help)
  2. ^ "The Advanced Technology Solar Telescope". Retrieved 2013-09-26.
  3. ^ Durand, Pierrot (2013-09-21), "Work on Dome Completed, say Spanish Companies", French Tribune, retrieved 2013-09-26. Note that the illustration accompanying the article is a 2012 artists' rendering of the Thirty Meter Telescope calotte dome, and looks nothing like the actual ATST enclosure.

See also