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Critical Science Plan for the Daniel K. Inouye Solar Telescope (DKIST)

Mark Rast, +89 more
- 19 Apr 2021 - 
- Vol. 296, Iss: 4, pp 1-88
TLDR
The National Science Foundation's Daniel K. Inouye Solar Telescope (DKIST) will revolutionize our ability to measure, understand, and model the basic physical processes that control the structure and dynamics of the Sun and its atmosphere as discussed by the authors.
Abstract
The National Science Foundation’s Daniel K. Inouye Solar Telescope (DKIST) will revolutionize our ability to measure, understand, and model the basic physical processes that control the structure and dynamics of the Sun and its atmosphere. The first-light DKIST images, released publicly on 29 January 2020, only hint at the extraordinary capabilities that will accompany full commissioning of the five facility instruments. With this Critical Science Plan (CSP) we attempt to anticipate some of what those capabilities will enable, providing a snapshot of some of the scientific pursuits that the DKIST hopes to engage as start-of-operations nears. The work builds on the combined contributions of the DKIST Science Working Group (SWG) and CSP Community members, who generously shared their experiences, plans, knowledge, and dreams. Discussion is primarily focused on those issues to which DKIST will uniquely contribute.

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Citations
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The Atmospheric Response to High Nonthermal Electron-beam Fluxes in Solar Flares. II. Hydrogen-broadening Predictions for Solar Flare Observations with the Daniel K. Inouye Solar Telescope

TL;DR: In this paper , the authors incorporate nonideal, nonadiabatic line-broadening profiles of hydrogen into the RADYN code to accurately interpret the upcoming spectral data of solar flares with the DKIST.
Journal ArticleDOI

The Visible Spectro-Polarimeter of the Daniel K. Inouye Solar Telescope

TL;DR: The Visible Spectro-Polarimeter (ViSP) as mentioned in this paper is a spectrograph with the ability to observe solar regions up to a $120\times 78~\mbox{arcsec}^{2}$ .
Journal ArticleDOI

Irradiance Variations of the Sun and Sun-Like Stars – Overview of Topical Collection

TL;DR: In this article, a topical collection summarizes recent advances in observing and modeling irradiance variations of the Sun and Sun-like stars, emphasizing the links between surface magnetic fields and the resulting solar and stellar variability.
References
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Relaxation of toroidal plasma and generation of reverse magnetic fields

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Journal ArticleDOI

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TL;DR: In this article, a magnetic breakout model for the initiation of a solar coronal mass ejection (CME) was proposed, where reconnection between a sheared arcade and neighboring flux systems triggers the eruption.
Journal ArticleDOI

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Critical Science Plan for the Daniel K. Inouye Solar Telescope (DKIST)