Daniel K. Inouye Solar Telescope: High-resolution observing of the dynamic Sun

被引：78

作者：

Tritschler, A. ^{[1
]}

Rimmele, T. R. ^{[1
]}

Berukoff, S. ^{[1
]}

Casini, R. ^{[2
]}

Kuhn, J. R. ^{[4
]}

Lin, H. ^{[4
]}

Rast, M. P. ^{[5
]}

McMullin, J. P. ^{[3
]}

Schmidt, W. ^{[6
]}

Woger, F. ^{[1
]}

机构：

[1] Natl Solar Observ, 3665 Discovery Dr, Boulder, CO 80303 USA

[2] Natl Ctr Atmospher Res, High Altitude Observ, POB 3000, Boulder, CO 80307 USA

[3] Natl Solar Observ, 950 N Cherry Ave, Tucson, AZ 85719 USA

[4] Univ Hawaii, Inst Astron, 34 Ohia Ku St, Pukalani, HI 96768 USA

[5] Univ Colorado, Dept Astrophys & Planetary Sci, Lab Atmospher & Space Phys, Boulder, CO 80309 USA

[6] Kiepenheuer Inst Sonnenphys, Schoneckstr 6, D-79104 Freiburg, Germany

来源：

ASTRONOMISCHE NACHRICHTEN | 2016年 / 337卷 / 10期

关键词：

instrumentation: adaptive optics; instrumentation: high angular resolution; instrumentation: polarimeters; instrumentation: spectrographs; telescopes;

D O I：

10.1002/asna.201612434

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The 4-m aperture Daniel K. Inouye Solar Telescope (DKIST) formerly known as the Advanced Technology Solar Telescope (ATST) is currently under construction on Haleakala (Maui, Hawai'i) projected to start operations in 2019. At the time of completion, DKIST will be the largest ground-based solar telescope providing unprecedented resolution and photon collecting power. The DKIST will be equipped with a set of first-light facility-class instruments offering unique imaging, spectroscopic and spectropolarimetric observing opportunities covering the visible to infrared wavelength range. This first-light instrumentation suite will include: a Visible Broadband Imager (VBI) for high-spatial and-temporal resolution imaging of the solar atmosphere; a Visible Spectro-Polarimeter (ViSP) for sensitive and accurate multi-line spectropolarimetry; a Fabry-Perot based Visible Tunable Filter (VTF) for high-spatial resolution spectropolarimetry; a fiber-fed Diffraction-Limited Near Infra-Red Spectro-Polarimeter (DL-NIRSP) for two-dimensional high-spatial resolution spectropolarimetry (simultaneous spatial and spectral information); and a Cryogenic Near Infra-Red Spectro-Polarimeter (Cryo-NIRSP) for coronal magnetic field measurements and on-disk observations of, e. g., the CO lines at 4.7 mu m. We will provide an overview of the DKISTs unique capabilities with strong focus on the first-light instrumentation suite, highlight some of the additional properties supporting observations of transient and dynamic solar phenomena, and touch on some operational strategies and the DKIST critical science plan. (C) 2016 WILEY-VCH Verlag GmbH& Co. KGaA, Weinheim

引用

页码：1064 / 1069

页数：6

共 28 条

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