The Daniel K. Inouye Solar Telescope (DKIST) Cryogenic Near-Infrared Spectro-Polarimeter

The Cryogenic Near-Infrared Spectro-Polarimeter ( Cryo -NIRSP) is a combination slit-based spectrograph and context-imaging instrument designed and built for the National Science Foundation’s Daniel K. Inouye Solar Telescope (DKIST). It is optimized for polarimetric observations of spectral band-pas...

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Published inSolar physics Vol. 298; no. 1; p. 5
Main Authors Fehlmann, André, Kuhn, Jeffrey R., Schad, Thomas A., Scholl, Isabelle F., Williams, Rebecca, Agdinaoay, Rodell, Berst, D. Christopher, Craig, Simon C., Giebink, Cynthia, Goodrich, Bret, Hnat, Kirby, James, Don, Lockhart, Charles, Mickey, Donald L., Oswald, Daniel, Puentes, Myles M., Schickling, Richard, de Vanssay, Jean-Benoit, Warmbier, Eric A.
Format Journal Article
LanguageEnglish
Published Dordrecht Springer Netherlands 2023
Springer Nature B.V
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Abstract The Cryogenic Near-Infrared Spectro-Polarimeter ( Cryo -NIRSP) is a combination slit-based spectrograph and context-imaging instrument designed and built for the National Science Foundation’s Daniel K. Inouye Solar Telescope (DKIST). It is optimized for polarimetric observations of spectral band-passes between 1 and 5 microns, which makes it uniquely suited for polarimetric observations of the solar corona, while also enabling access to other important infrared diagnostics such as the CO fundamental band at 4.6 microns. Integration, testing, and commissioning occurred between 2019 and 2020, and it is now conducting science experiments as part of DKIST early operations. In this article, we discuss its science mission, the requirements driving the design, its fabrication and installation, current capabilities, and the first science data.
AbstractList Abstract The Cryogenic Near-Infrared Spectro-Polarimeter ( Cryo -NIRSP) is a combination slit-based spectrograph and context-imaging instrument designed and built for the National Science Foundation’s Daniel K. Inouye Solar Telescope (DKIST). It is optimized for polarimetric observations of spectral band-passes between 1 and 5 microns, which makes it uniquely suited for polarimetric observations of the solar corona, while also enabling access to other important infrared diagnostics such as the CO fundamental band at 4.6 microns. Integration, testing, and commissioning occurred between 2019 and 2020, and it is now conducting science experiments as part of DKIST early operations. In this article, we discuss its science mission, the requirements driving the design, its fabrication and installation, current capabilities, and the first science data.
The Cryogenic Near-Infrared Spectro-Polarimeter (Cryo-NIRSP) is a combination slit-based spectrograph and context-imaging instrument designed and built for the National Science Foundation’s Daniel K. Inouye Solar Telescope (DKIST). It is optimized for polarimetric observations of spectral band-passes between 1 and 5 microns, which makes it uniquely suited for polarimetric observations of the solar corona, while also enabling access to other important infrared diagnostics such as the CO fundamental band at 4.6 microns. Integration, testing, and commissioning occurred between 2019 and 2020, and it is now conducting science experiments as part of DKIST early operations. In this article, we discuss its science mission, the requirements driving the design, its fabrication and installation, current capabilities, and the first science data.
The Cryogenic Near-Infrared Spectro-Polarimeter ( Cryo -NIRSP) is a combination slit-based spectrograph and context-imaging instrument designed and built for the National Science Foundation’s Daniel K. Inouye Solar Telescope (DKIST). It is optimized for polarimetric observations of spectral band-passes between 1 and 5 microns, which makes it uniquely suited for polarimetric observations of the solar corona, while also enabling access to other important infrared diagnostics such as the CO fundamental band at 4.6 microns. Integration, testing, and commissioning occurred between 2019 and 2020, and it is now conducting science experiments as part of DKIST early operations. In this article, we discuss its science mission, the requirements driving the design, its fabrication and installation, current capabilities, and the first science data.
ArticleNumber 5
Author de Vanssay, Jean-Benoit
Berst, D. Christopher
Mickey, Donald L.
Puentes, Myles M.
Goodrich, Bret
Hnat, Kirby
Schickling, Richard
Schad, Thomas A.
Scholl, Isabelle F.
Giebink, Cynthia
Kuhn, Jeffrey R.
Warmbier, Eric A.
Williams, Rebecca
Oswald, Daniel
Lockhart, Charles
Craig, Simon C.
James, Don
Fehlmann, André
Agdinaoay, Rodell
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  surname: Warmbier
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  organization: Institute for Astronomy, University of Hawai´i
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Snippet The Cryogenic Near-Infrared Spectro-Polarimeter ( Cryo -NIRSP) is a combination slit-based spectrograph and context-imaging instrument designed and built for...
Abstract The Cryogenic Near-Infrared Spectro-Polarimeter ( Cryo -NIRSP) is a combination slit-based spectrograph and context-imaging instrument designed and...
The Cryogenic Near-Infrared Spectro-Polarimeter (Cryo-NIRSP) is a combination slit-based spectrograph and context-imaging instrument designed and built for the...
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StartPage 5
SubjectTerms Astronomy
Astrophysics and Astroparticles
Atmospheric Sciences
Corona
Design
Fabrication
Infrared spectra
Magnetic fields
Near infrared radiation
Observatories
Optics
Physics
Physics and Astronomy
Polarimeters
Polarimetry
Sensors
Solar corona
Solar physics
Space Exploration and Astronautics
Space Sciences (including Extraterrestrial Physics
Spectrum analysis
Telescopes
The Daniel K. Inouye Solar Telescope (DKIST)
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Title The Daniel K. Inouye Solar Telescope (DKIST) Cryogenic Near-Infrared Spectro-Polarimeter
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