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 National Science Foundation’s (NSF) Daniel K. Inouye Solar Telescope (DKIST) is a four-meter off-axis telescope on the island of Maui, Hawai'i. DKIST took its first light images in 2019, making it the most powerful solar telescope in the world. From the inception of DKIST, safety was a fundamental consideration. To ensure that hazard reduction was considered throughout a Hazard Analysis Team (HAT) was formed from members of the staff. This team conducted regular meetings during the design phases to analyze design choices, assess inter-system hazards, and to ensure compliance with safety standards. In addition to the core team members, subject matter experts were brought into the meetings when specific expertise was needed. A key understanding was that hazard analysis (HA) was not a single event or deliverable, but a continuous, managed process to ensure that hazards were properly identified, analyzed, and mitigated. As the design matured, the HAT continued meetings, retiring some hazards, while identifying new hazards. New hazards would appear not only because of changes in the design but also from a better understanding of the interaction between observatory systems. The DKIST is now beyond the construction phase and moving into operations yet we find that the HAT continues to be used to refine how hazards are handled and implement mitigations appropriately. Changes to the hazard analysis process itself were also implemented as we learned how to better handle our hazard analysis procedures. During the early design and construction phases, hazard analyses were a required contract deliverable, with the HAs conducted by individual sub-system vendors. As the project shifted from design into construction and eventually integration, the various hazard analyses had to be combined. New tools for tracking hazards and methods for on-line collaboration were added to aid continuing management of hazards as the project shifted from design to construction to operations.
The National Science Foundation’s 4m Daniel K. Inouye Solar Telescope (DKIST) on Haleakala, Maui is now the largest solar telescope in the world. DKIST’s superb resolution and polarimetric sensitivity will enable astronomers to unravel many of the mysteries the Sun presents, including the origin of solar magnetism, the mechanisms of coronal heating and drivers of flares and coronal mass ejections. Five instruments, four of which provide highly sensitive measurements of solar magnetic fields, including the illusive magnetic field of the faint solar corona. DKIST operates as a coronagraph at infrared wavelengths where the sky background is low and bright coronal emission lines are available. The high-order, single-conjugate adaptive optics system (AO) provides diffraction limited imaging and the ability to resolve features approximately 20 km on the Sun. A multi-conjugate AO upgrade is in progress. With these unique capabilities DKIST will address basic research aspects of Space Weather and help improve predictive capabilities. DKIST has completed construction and is now in the early phases of operations. Community proposal-based shared-risk observations are conducted by the DKIST operations team.
Construction of the Daniel K. Inouye Solar Telescope (DKIST) is well underway on the Haleakalā summit on the Hawaiian island of Maui. Featuring a 4-m aperture and an off-axis Gregorian configuration, the DKIST will be the world’s largest solar telescope. It is designed to make high-precision measurements of fundamental astrophysical processes and produce large amounts of spectropolarimetric and imaging data. These data will support research on solar magnetism and its influence on solar wind, flares, coronal mass ejections, and solar irradiance variability. Because of its large aperture, the DKIST will be able to sense the corona’s magnetic field—a goal that has previously eluded scientists—enabling observations that will provide answers about the heating of stellar coronae and the origins of space weather and exo-weather. The telescope will cover a broad wavelength range (0.35 to 28 microns) and operate as a coronagraph at infrared (IR) wavelengths. Achieving the diffraction limit of the 4-m aperture, even at visible wavelengths, is paramount to these science goals. The DKIST’s state-of-the-art adaptive optics systems will provide diffraction-limited imaging, resolving features that are approximately 20 km in size on the Sun.
At the start of operations, five instruments will be deployed: a visible broadband imager (VTF), a visible spectropolarimeter (ViSP), a visible tunable filter (VTF), a diffraction-limited near-IR spectropolarimeter (DLNIRSP), and a cryogenic near-IR spectropolarimeter (cryo-NIRSP). At the end of 2017, the project finished its fifth year of construction and eighth year overall. Major milestones included delivery of the commissioning blank, the completed primary mirror (M1), and its cell. Commissioning and testing of the coudé rotator is complete and the installation of the coudé cleanroom is underway; likewise, commissioning of the telescope mount assembly (TMA) has also begun. Various other systems and equipment are also being installed and tested. Finally, the observatory integration, testing, and commissioning (IT&C) activities have begun, including the first coating of the M1 commissioning blank and its integration within its cell assembly. Science mirror coating and initial on-sky activities are both anticipated in 2018.
We provide an update on the construction status of the Daniel K. Inouye Solar Telescope. This 4-m diameter facility is designed to enable detection and spatial/temporal resolution of the predicted, fundamental astrophysical processes driving solar magnetism at their intrinsic scales throughout the solar atmosphere. These data will drive key research on solar magnetism and its influence on solar winds, flares, coronal mass ejections and solar irradiance variability. The facility is developed to support a broad wavelength range (0.35 to 28 microns) and will employ state-of-the-art adaptive optics systems to provide diffraction limited imaging, resolving features approximately 20 km on the Sun. At the start of operations, there will be five instruments initially deployed: Visible Broadband Imager (VBI; National Solar Observatory), Visible SpectroPolarimeter (ViSP; NCAR High Altitude Observatory), Visible Tunable Filter (VTF (a Fabry-Perot tunable spectropolarimeter); Kiepenheuer Institute for Solarphysics), Diffraction Limited NIR Spectropolarimeter (DL-NIRSP; University of Hawaii, Institute for Astronomy) and the Cryogenic NIR Spectropolarimeter (Cryo-NIRSP; University of Hawaii, Institute for Astronomy).
As of mid-2016, the project construction is in its 4th year of site construction and 7th year overall. Major milestones in the off-site development include the conclusion of the polishing of the M1 mirror by University of Arizona, College of Optical Sciences, the delivery of the Top End Optical Assembly (L3), the acceptance of the Deformable Mirror System (Xinetics); all optical systems have been contracted and are either accepted or in fabrication. The Enclosure and Telescope Mount Assembly passed through their factory acceptance in 2014 and 2015, respectively. The enclosure site construction is currently concluding while the Telescope Mount Assembly site erection is underway. The facility buildings (Utility and Support and Operations) have been completed with ongoing work on the thermal systems to support the challenging imaging requirements needed for the solar research.
Finally, we present the construction phase performance (schedule, budget) with projections for the start of early operations.
KEYWORDS: Solar telescopes, Systems engineering, Telescopes, Visualization, Astronomy, Geographic information systems, Coating, Optical alignment, Wavefronts, Systems modeling
The Daniel K. Inouye Solar Telescope (DKIST) has been in its construction phase since 2010, anticipating the onset of the integration, test, and commissioning (IT&C) phase in early 2017, and the commencement of science verification in 2019. The works on Haleakala are progressing at a phenomenal rate and many of the various subsystems are either through or about to enter their Factory (or Laboratory) acceptance. The delays in obtaining site planning permissions, while a serious issue for Project Management, has allowed the sub-systems to develop well ahead of their required delivery to site. We have benefited from the knowledge that many sub-systems will be on site and ready for integration well before affecting the critical path. Opportunities have been presented for additional laboratory/factory testing which, while not free, significantly reduce the risks of potential delays and rework on site. From the perspective of IT&C this has provided an opportunity to develop the IT&C plans and schedules free from the pressures of imminent deployment.
In this paper we describe the ongoing planning of the Integration, Testing and Commissioning (IT&C) phase of the project in particular the detailed planning phase that we are currently developing.
KEYWORDS: Solar telescopes, Systems engineering, Observatories, Content addressable memory, Chromium, Control systems, Neodymium, Databases, Phase modulation, Process control
We provide a brief update on the construction status of the Daniel K. Inouye Solar Telescope, a $344M, 10-year construction project to design and build the world's largest solar physics observatory. We review the science drivers along with the challenges in meeting the evolving scientific needs over the course of the construction period without jeopardizing the systems engineering and management realization. We review the tools, processes and performance measures in use in guiding the development as well as the risks and challenges as the project transitions through various developmental phases. We elaborate on environmental and cultural compliance obligations in building in Hawai'i. We discuss the broad "lessons learned". Finally, we discuss the project in the context of the evolving management oversight within the US (in particular under the NSF).
The Daniel K. Inouye Solar Telescope (DKIST) was envisioned from an early stage to incorporate a functional safety system to ensure the safety of personnel and equipment within the facility. Early hazard analysis showed the need for a functional safety system. The design used a distributed approach in which each major subsystem contains a PLC-based safety controller. This PLC-based system complies with the latest international standards for functional safety. The use of a programmable controller also allows for flexibility to incorporate changes in the design of subsystems without adversely impacting safety. Various subsystems were built by different contractors and project partners but had to function as a piece of the overall control system. Using distributed controllers allows project contractors and partners to build components as standalone subsystems that then need to be integrated into the overall functional safety system. Recently factory testing was concluded on the major subsystems of the facility. Final integration of these subsystems is currently underway on the site. Building on lessons learned in early factory tests, changes to the interface between subsystems were made to improve the speed and ease of integration of the entire system. Because of the distributed design each subsystem can be brought online as it is delivered and assembled rather than waiting until the entire facility is finished. This enhances safety during the risky period of integration and testing. The DKIST has implemented a functional safety system that has allowed construction of subsystems in geographically diverse locations but that function cohesively once they are integrated into the facility currently under construction.
The Daniel K. Inouye Solar Telescope (DKIST), formerly the Advanced Technology Solar Telescope (ATST), has
been in its construction phase since 2010, anticipating the onset of the integration, test, and commissioning (IT&C)
phase late in 2016, and the commencement of science verification in early 2019. In this paper we describe the
planning of the Integration, Testing and Commissioning (IT&C) phase of the project.
KEYWORDS: Safety, Hazard analysis, Injuries, Standards development, Systems engineering, Telescopes, Solar telescopes, Geographic information systems, Robots, Control systems
System safety for the Daniel K. Inouye Solar Telescope (DKIST) is the joint responsibility of a Maui-based safety team
and the Tucson-based systems engineering group. The DKIST project is committed to the philosophy of “Safety by
Design”. To that end the project has implemented an aggressive hazard analysis, risk assessment, and mitigation system.
It was initially based on MIL-STD-882D, but has since been augmented in a way that lends itself to direct application to
the design of our Global Interlock System (GIS). This was accomplished by adopting the American National Standard
for Industrial Robots and Robot Systems (ANSI/RIA R15.06) for all identified hazards that involve potential injury to
personnel.
In this paper we describe the details of our augmented hazard analysis system and its use by the project. Since most of
the major hardware for the DKIST (e.g., the enclosure, and telescope mount assembly) has been designed and is being
constructed by external contractors, the DKIST project has required our contractors to perform a uniform hazard analysis
of their designs using our methods. This paper also describes the review and follow-up process implemented by the
project that is applied to both internal and external subsystem designs. Our own weekly hazard analysis team meetings
have now largely turned to system-level hazards and hazards related to specific tasks that will be encountered during
integration, test, and commissioning and maintenance operations. Finally we discuss a few lessons learned, describing
things we might do differently if we were starting over today.
Since inception, the Advanced Technology Solar Telescope (ATST) has planned to implement a facility-wide functional
safety system to protect personnel from harm and prevent damage to the facility or environment. The ATST will deploy
an integrated safety-related control system (SRCS) to achieve functional safety throughout the facility rather than relying
on individual facility subsystems to provide safety functions on an ad hoc basis.
The Global Interlock System (GIS) is an independent, distributed, facility-wide, safety-related control system, comprised
of commercial off-the-shelf (COTS) programmable controllers that monitor, evaluate, and control hazardous energy and
conditions throughout the facility that arise during operation and maintenance.
The GIS has been designed to utilize recent advances in technology for functional safety plus revised national and
international standards that allow for a distributed architecture using programmable controllers over a local area network
instead of traditional hard-wired safety functions, while providing an equivalent or even greater level of safety.
Programmable controllers provide an ideal platform for controlling the often complex interrelationships between
subsystems in a modern astronomical facility, such as the ATST. A large, complex hard-wired relay control system is no
longer needed. This type of system also offers greater flexibility during development and integration in addition to
providing for expanded capability into the future. The GIS features fault detection, self-diagnostics, and redundant
communications that will lead to decreased maintenance time and increased availability of the facility.
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