The National Science Foundation’s Daniel K. Inouye Solar Telescope (DKIST) located on the summit of Haleakalā, Maui is the largest solar telescope in the world. Housing a 4-meter off-axis primary mirror and a highly advanced adaptive optics system, DKIST is enabling observations of specific regions of the Sun in higher resolution and greater detail than any preexisting ground-based telescope. The DKIST Enclosure Azimuth Mechanism is responsible for accurate positioning of the Enclosure in azimuth and provides a second degree of freedom to the altitude movement of the Enclosure Shutter which enables an overall position accuracy of 19 arcmin point-to-point at the Enclosure Aperture. The mechanism is primarily comprised of sixteen track rail segments, eight driven bogies, and two idler bogies, and it serves as the interface between the fixed support building Ring Girder structure and the rotating Enclosure structure. Visual observations and control system torque data have shown evidence of a loss of contact at the interface between the individual bogie wheels and the track rail. This loss of contact results in imbalanced loading conditions that impact performance and reliability as loads are varied in proportion to the number of wheels in contact. In addition, visual inspections have shown early indications of rolling contact fatigue at specific azimuth locations of the track rails due to high contact stresses. As a result, a project was initiated to improve load sharing and maintain tracking accuracy by minimizing pointing error deviations that result from rail flatness tolerances variations, unanticipated mechanical deformations from load imbalances, and varying control systems demands. In addition, equalizing the load balance will reduce unintended fatigue loading of the structural and mechanical components as well as reduce contact stresses in the rail sections improving overall mechanism reliability. The investigation, implementation, and evaluation of this process is presented herein.
The US National Science Foundation 4m Daniel K. Inouye Solar Telescope (DKIST) on Haleakala, Maui is the largest solar telescope in the world. DKIST’s superb resolution and polarimetric sensitivity will enable astronomers to explore the origins of solar magnetism, the mechanisms of coronal heating and drivers of flares and coronal mass ejections. DKIST operates as a coronagraph at infrared wavelengths, providing crucial measurements of the magnetic field in the corona. During its Operations Commissioning Phase, DKIST has already conducted a significant number of shared-risk observations for community researchers. The complex raw data are calibrated by the DKIST Data Center located in Boulder and distributed to the science community. We’ll present examples of science results and discuss lessons learned. Ongoing instrument development efforts include, an upgrade of the single-conjugate adaptive optics system to a multi-conjugate AO, the implementation of image slicers for the DL-NIRSP instrument and development of infrared detectors the DL- and CRYO-NIRSP instruments.
The Daniel K. Inouye Solar Telescope (DKIST) will be the largest solar telescope in the world, housing a 4 meter primary mirror that will enable observation of specific regions of the sun in higher resolution and greater detail than any existing telescope. The DKIST Facility Thermal Systems is comprised of various systems and components that contribute to maintaining an appropriate thermal environment for solar observation. One of these systems is the Carousel Cooling System, which contributes to active control of the Enclosure thermal environment. This system is intended to actively maintain the Enclosure exterior at, or just below, ambient temperature through a system of plate heat exchangers. These heat exchangers, termed plate coils, are designed to reject solar radiation from the Enclosure cladding in order to mitigate dome seeing effects caused by turbulent air of dissimilar temperatures. Per DKIST's specifications, OMEGA Thermo Products fabricated 232 type 304 stainless steel plate coils that are categorized into 104 different dimensions. These are in the process of being installed on the following sections of the Enclosure: Aperture Stop, Shutter, Arches and Vent Gates. This has further complicated installation as each section yields different requirements for lifting, integrating, mounting, and piping the various plate coils. Presented here is a review of the installation progress and future planning for the Carousel Cooling System.
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