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检索条件"任意字段=Conference on Advanced Telescope and Instrumentation Control Software"

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Recent Advances in Stray Light Modeling for Large telescope/Observatory Systems 8

Recent Advances in Stray Light Modeling for Large Telescope/...

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conference on Modeling, Systems Engineering, and Project Management for Astronomy VIII

作者： Pfisterer, Richard N. Pompea, Stephen M. Ellis, Scott Photon Engn LLC 310 S Williams BlvdSuite 222 Tucson AZ 85711 USA Natl Opt Astron Observ 950 N Cherry Ave Tucson AZ 85719 USA

ISBN: (数字)9781510619647

ISBN: (纸本)9781510619647

Stray light analyses have been a serious consideration in the development of optomechanical instrumentation from the time of Galileo. In the late 1960's and 1970's, NASA and the US Air Force realized that software modeling was the key to predictive development and analysis of optical systems and funded the first efforts to automate the analysis process with the development of the GUERAP and APART computer software programs.. The development of multi-wavelength scatterometers in that same era made it possible to more fully characterize the scatter properties of paints and other surface treatments.. These two improvements advanced stray light modeling capabilities and a well-developed modeling approach. In the past twenty years demands for modeling complex structures (e.g., individual screws and small vanes edges) coupled with requirements for ever increasing sensitivity have placed a tremendous computational burden on the stray light analyst. In this paper, we discuss the approaches to modeling today's complex telescope systems that frequently include stray light artifacts traceable to the complete observatory. Scatter modeling and data reduction has become major components of the stray light analysis task and recent work has identified instances where scatter measurements performed by skilled technicians are inaccurate and useless without additional analysis and interpretation. Finally we discuss common metrics for stray light characterization of large systems and how distributed computing, cloud computing, and GPU-enabled software allow the analyst to compute levels and uniformity of stray light in these systems to levels heretofore considered impossible.

关键词： Stray light Sensors software development Systems modeling Stars Large Synoptic Survey telescope Ray tracing Stray light analysis telescopes Observatories

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Leveraging control System Evolution for Plant and Personnel Efficiency

Leveraging Control System Evolution for Plant and Personnel ...

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IEEE Cement Industry Technical conference

作者： Gregory Davis Thomas Jankowski Gregory Kemper Joe Holmes Profi-Vision Automation Allentown PA USA Lehigh Hanson Cement Company LLC Allentown PA USA Siemens Industry Inc Norcross GA USA

With advancing technology, plant-based automated control systems (ACS) eventually reaches the end of its useful life and an upgrade is required. ACS upgrades can be driven by reliability issues, system expansion limitations, or advanced networking security standards to name a few. Within an automated control system platform, there are several layers of automated resources, the enterprise/business level, the manufacturing execution system (MES)/operator control level, the controller level, and the device/instrumentation level. Each of the resource layers have an ideal lifecycle window that is tied to the evolution of the vendor system or hardware that is being utilized for automation. While the device/instrumentation level resources may have a longer life cycle, the enterprise or business level resources have a shorter life cycle due to a more frequent update timeline of vendor software and systems support. Recent patterns for increased connectivity demand on the enterprise level for analytical analysis coupled with demands for advanced networking security standards have accelerated the enterprise/business level's evolution. Inherently, these demands for connectivity have put a strain on the lower MES/operator and controller resource levels of the control system to gather and process this required field information. But these demands are not only limited to the ACS components as the plant must maintain a technical staff outside of a traditional IT department to support the new software and hardware systems. This paper describes the levels within an automated control system and how a management team can leverage the evolution of the control system in the plant to meet the growing demands of the enterprise level while also raising the level of technical aptitude of plant employees required to support the modern system design. It will describe the benefits of giving plant operators access to enhanced process information to increase plant reliability and using web-based

关键词： control systems Process control Maintenance engineering Standards software Tools Protocols

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eROSITA System Functionality and Operation

eROSITA System Functionality and Operation

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conference on Space telescopes and instrumentation - Ultraviolet to Gamma Ray

作者： Coutinho, D. Bornemann, W. Budau, B. Burwitz, V. Fuermetz, M. Gaida, R. Hartner, G. Kink, W. Meidinger, N. Mueller, S. Predehl, P. Max Planck Inst Extraterr Phys Garching Germany

ISBN: (数字)9781510619524

ISBN: (纸本)9781510619524

eROSITA (extended ROentgen Survey with an Imaging telescope Array) is the primary scientific payload on board the SRG (Spektrum Rontgen Gamma) mission, scheduled for launch in March 2019. Its destination is the Lagrangian point L2, and its mission is to make a full survey of the X-ray sky. eROSITA is a complex instrument composed of seven identical co-aligned X-ray telescopes with a focal length of 1600mm and an aperture of 7x350mm. Each telescope is equipped with an independent CCD camera. The cold redundant ITC manages all seven cameras as well as the thermal control of the telescope and the interface to the spacecraft. The complexity of this system resides in the fact that the hardware and software interfaces to the spacecraft are minimal. In this respect the ITC has a key role in the management of the instrument, as well as in the science data management. This proved to be an optimal solution in terms of instrument flexibility, but also presented some challenges. The paper presents an overview on the eROSITA system functionality, its interfaces and operational modes together with an outline of the main challenges, which were faced during integration and verification of the complete system. The function of the instrument was verified in the frame of an extensive end-to-end test in vacuum under representative thermal control conditions to verify that the instrument functions under worst case conditions. Currently tests are performed in combination with the spacecraft to verify communication between eROSITA and the spacecraft and the data transfer through the Russian radio complex (TM/TC system). This includes all operational and survival modes. The paper summarizes the main results of the functional tests on instrument level and on spacecraft level.

关键词： eROSITA SRG Spectrum-Roentgen-Gamma X-ray telescope space telescope all-sky survey astrophysics

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High-Contrast Imager for Complex Aperture telescopes(HiCAT): 5. First Results With Segmented-Aperture Coronagraph and Wavefront control

High-Contrast Imager for Complex Aperture Telescopes(HiCAT):...

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conference on Space telescopes and instrumentation - Optical, Infrared, and Millimeter Wave

作者： Soummer, Remi Brady, Gregory R. Brooks, Keira Comeau, Thomas Choquet, Elodie Dillon, Tom Egron, Sylvain Gontrum, Rob Hagopian, John Laginja, Iva Leboulleux, Lucie Perrin, Marshall D. Petrone, Peter Pueyo, Laurent Mazoyer, Johan N'Diaye, Mamadou Riggs, A. J. Eldorado Shiri, Ron Sivaramakrishnan, Anand St Laurent, Kathryn Valenzuela, Ana-Maria Zimmerman, Neil T. Space Telescope Sci Inst 3700 San Martin Dr Baltimore MD 21218 USA Lab Astrophys Marseille UMR 7326 F-13388 Marseille France Off Natl Etud & Rech Aerosp BP 72 F-92320 Chatillon France Observ Nice Cote Azur Lab Lagrange F-06304 Nice France CALTECH MC 249-17 Pasadena CA 91125 USA Jet Prop Lab 4800 Oak Grove Dr Pasadena CA 91109 USA Iridescence SARL 149 Ave Maine F-75014 Paris France Adv Nanophoton Inc 4437 Windsor Farm Rd Harwood MD USA Iridescence SARL 149 Ave Maine F-75014 Paris France NASA Goddard Space Ctr 8800 Greenbelt Rd Greenbelt MD 20771 USA Johns Hopkins Univ 3400 North Charles St Baltimore MD 21218 USA Sigma Space Corp 4600 Forbes Blvd Lanham MD 20706 USA Univ Delaware Newark DE 19716 USA

ISBN: (数字)9781510619500

ISBN: (纸本)9781510619500

Segmented telescopes are a possible approach to enable large-aperture space telescopes for the direct imaging and spectroscopy of habitable worlds. However, the increased complexity of their aperture geometry, due to the central obstruction, support structures and segment gaps, makes high-contrast imaging very challenging. The High-contrast Imager for Complex Aperture telescopes (HiCAT) testbed was designed to study and develop solutions for such telescope pupils using wavefront control and coronagraphic starlight suppression. The testbed design has the flexibility to enable studies with increasing complexity for telescope aperture geometries starting with off-axis telescopes, then on-axis telescopes with central obstruction and support structures - e.g. the Wide Field Infrared Survey telescope (WFIRST) - up to on-axis segmented telescopes, including various concepts for a Large UV, Optical, IR telescope (LUVOIR). In the past year, HiCAT has made significant hardware and software updates in order to accelerate the development of the project. In addition to completely overhauling the software that runs the testbed, we have completed several hardware upgrades, including the second and third deformable mirror, and the first custom Apodized Pupil Lyot Coronagraph (APLC) optimized for the HiCAT aperture, which is similar to one of the possible geometries considered for LUVOIR. The testbed also includes several external metrology features for rapid replacement of parts, and in particular the ability to test multiple apodizers readily, an active tip-tilt control system to compensate for local vibration and air turbulence in the enclosure. On the software and operations side, the software infrastructure enables 24/7 automated experiments that include routine calibration tasks and high-contrast experiments. In this communication we present an overview and status update of the project, both on the hardware and software side, and describe the results obtained with APLC wavefro

关键词： Segmented telescopes coronagraphy exoplanet high-contrast imaging coronagraphy testbed Apodized Pupil Lyot Coronagraph APLC

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SALT and SAAO strategy, focusing on the time-domain: process, plans, and challenges 7

SALT and SAAO strategy, focusing on the time-domain: process...

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conference on Observatory Operations - Strategies, Processes, and Systems VII

作者： Vaisanen, Petri Crause, Lisa Gilbank, David Buckley, David A. H. Coetzee, Chris Crawford, Steven M. Potter, Stephen Pretorius, Retha Colmenero, Encarni Romero Sefako, Ramotholo Shara, Michael Sickafoose, Amanda Willames, Theodore B. South African Astron Observ POB 9 ZA-7935 Cape Town South Africa South African Large Telescope POB 9 ZA-7935 Cape Town South Africa Univ Cape Town Dept Astron ZA-7701 Cape Town South Africa Amer Museum Nat Hist Dept Astrophys Cent Pk West 79th St New York NY 10024 USA MIT 77 Massachusetts Ave Cambridge MA 02139 USA

ISBN: (数字)9781510619623

ISBN: (纸本)9781510619623

The South African astronomical community together with the international SALT community recently completed a process to detail a science strategy for SALT, the 10m international telescope that SAAO operates. After six years of science operations, the telescope is a very cost-effective large telescope science producer. The strategy was adopted by the SALT Board, and has already resulted in funding choices for the next stage of instrumentation. The SALT strategy intertwines with that of the SAAO and South African optical astronomy in general. This paper outlines the process followed, the main motivations and plans for the next stage, including risks and challenges. This paper in particular concentrates on the plans to making SAAO/SALT a major player in time domain astrophysics, one of three adopted strategic science focus areas. Plans include a novel design for a high-efficiency spectrograph serving transient follow-up, for which South Africa is well positioned;advanced software aiming to make the whole mountain-top operate as a single transient machine;feasibility studies into revolutionizing SALT observations by utilizing the primary mirror's hundreds of square degree size uncorrected field-of-view. Other SPIE papers in this meeting describe these and other developments at SALT and SAAO in more detail.

关键词： SALT Southern African Large telescope SAAO South African Astronomical Observatory Transients Time domain Strategy Intelligent software

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Development of the Arizona Robotic telescope Network 7

Development of the Arizona Robotic Telescope Network

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conference on Observatory Operations - Strategies, Processes, and Systems VII

作者： Weiner, Benjamin J. Sand, David Gabor, Paul Johnson, Chris Swindell, Scott Kubanek, Petr Gasho, Victor Golota, Taras Jannuzi, Buell Milne, Peter Smith, Nathan Zaritsky, Dennis Steward Observ MMT 933 N Cherry St Tucson AZ 85721 USA Steward Observ 933 N Cherry St Tucson AZ 85721 USA Vatican Observ 933 N Cherry St Tucson AZ 85721 USA Large Binocular Telescope Observ 933 N Cherry St Tucson AZ 85721 USA

ISBN: (数字)9781510619623

ISBN: (纸本)9781510619623

The Arizona Robotic telescope Network (ARTN) project is a long term effort to develop a system of telescopes to carry out a flexible program of PI observing, survey projects, and time domain astrophysics including monitoring, rapid response, and transient/target-of-opportunity followup. Steward Observatory operates and shares in several 1-3m class telescopes with quality sites and instrumentation, largely operated in classical modes. Science programs suited to these telescopes are limited by scheduling flexibility and people-power of available observers. Our goal is to adapt these facilities for multiple co-existing queued programs, interrupt capability, remote/robotic operation, and delivery of reduced data. In the long term, planning for the LSST era, we envision an automated system coordinating across multiple telescopes and sites, where alerts can trigger followup, classification, and triggering of further observations if required, such as followup imaging that can trigger spectroscopy. We are updating telescope control systems and software to implement this system in stages, beginning with the Kuiper 61" and Vatican Observatory 1.8-m telescopes. The Kuiper 61" and its Mont4K camera can now be controlled and queue-scheduled by the RTS2 observatory control software, and operated from a remote room at Steward. We discuss science and technical requirements for ARTN, and some of the challenges in adapting heterogenous legacy facilities, scheduling, data pipelines, and maintaining capabilities for a diverse user base.

关键词： remote observing robotic telescopes queue scheduling time-domain astronomy

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Fast Linearized Coronagraph Optimizer (FALCO) I: A software toolbox for rapid coronagraphic design and wavefront correction

Fast Linearized Coronagraph Optimizer (FALCO) I: A software ...

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conference on Space telescopes and instrumentation - Optical, Infrared, and Millimeter Wave

作者： Riggs, A. J. Eldorado Ruane, Garreth Sidick, Erkin Coker, Carl Kern, Brian D. Shaklan, Stuart B. CALTECH Jet Prop Lab Pasadena CA 91109 USA CALTECH Pasadena CA 91125 USA

ISBN: (数字)9781510619500

ISBN: (纸本)9781510619500

The Fast Linearized Coronagraph Optimizer (FALCO) is an open-source toolbox of routines for coronagraphic focal plane wavefront correction. The goal of FALCO is to provide a free, modular framework for the simulation or testbed operation of several common types of coronagraphs. FALCO includes routines for pair-wise probing estimation of the complex electric field and Electric Field Conjugation (EFC) control, and we ask the community to contribute other wavefront correction algorithms. FALCO utilizes and builds upon PROPER, an established optical propagation library. The key innovation in FALCO is the rapid computation of the linearized response matrix for each deformable mirror (DM), which facilitates re-linearization after each control step for faster DM-integrated coronagraph design and wavefront correction experiments. FALCO is freely available as source code in MATLAB at ***/ajeldorado/falco-matlab and will be available later this year in Python 3 at ***/ajeldorado/falco-python.

关键词： wavefront control wavefront estimation coronagraph high-contrast imaging PROPER modeling

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AvTA Based Assessment of Dependability Considering Recovery After Failures and Attacks on Vulnerabilities

AvTA Based Assessment of Dependability Considering Recovery ...

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IEEE International conference on Intelligent Data Acquisition and advanced Computing Systems

作者： Vyacheslav Kharchenko Yuriy Ponochovniy Al-Sudani Mustafa Qahtan Abdulmunem Iryna Shulga National Aerospace University KhAI Poltava State Agrarian Academy

ISBN: (纸本)9781728140704

The paper describes modification of the ATA (Attack Tree Analysis) technique for assessment of instrumentation and control systems (ICS) dependability (reliability, availability and cyber security) called AvTA (Availability Tree Analysis). The techniques FMEA, FMECA and IMECA applied to carry out preliminary semi-formal and criticality oriented analysis before AvTA based assessment are described. AvTA models combine reliability and cyber security subtrees considering probabilities of ICS recovery in case of hardware (physical) and software (design) failures and attacks on components casing failures. Successful recovery events (SREs) avoid corresponding failures in tree using OR gates if probabilities of SRE for assumed time are more than required. Case for dependability AvTA based assessment (model, availability function and technology of decision-making for choice of component and system parameters) for smart building ICS (Building Automation Systems, BAS) is discussed.

关键词： Availability tree analysis instrumentation and control system Dependability assessment Building automation system Building automation systems Network security Probability failures Series Relay Vulnerability Integrated circuits Criticality system parameter Trees

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VIRUS: the instrument infrastructure to support the deployment and upkeep of 156 spectrographs at the Hobby-Eberly telescope 3

VIRUS: the instrument infrastructure to support the deployme...

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conference on Advances in Optical and Mechanical Technologies for telescopes and instrumentation III

作者： Spencer, R. Balderrama, E. Damm, G. Fowler, J. Good, J. Hill, G. J. Kriel, H. MacQueen, P. Mrozinski, E. Perry, D. Peterson, T. Shetrone, M. Savage, R. Smith, G. Cook, E. DePoy, D. Marshall, J. Prochaska, T. Sauseda, M. Univ Texas Ft Davis McDonald Observ Hobby Eberly Telescope 32 Mt Fowlkes Rd Ft Davis TX 79734 USA Univ Texas Austin McDonald Observ 2515 SpeedwayC1402 Austin TX 78712 USA Texas A&M Univ Dept Phys & Astron TAMU 4242 College Stn TX 77843 USA

ISBN: (数字)9781510619661

ISBN: (纸本)9781510619661

The Visible Integral-field Replicable Unit Spectrograph (VIRUS) consists of 156 identical spectrographs fed by 35,000 fibers from the upgraded 10-meter Hobby-Eberly telescope (HET). VIRUS is in a phased deployment. At the submission of this paper, over half of the units are installed and the full support infrastructure is operational. This paper will describe the VIRUS infrastructure which includes the physical support system, the air cooling, the cryogenic cooling, and the temperature control of VIRUS. The paper will also discuss the various installation, maintenance, and operational procedures based on growing experience with the VIRUS array.

关键词： VIRUS spectrograph cryogenics nitrogen maintenance Hobby Eberly telescope vacuum fiber optics

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LSST telescope and Site Status 7

LSST Telescope and Site Status

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conference on Ground-based and Airborne telescopes VII

作者： Gressler, William J. Coleman, Grissel Delgado, Francisco Neill, Douglas R. Sebag, Jacques Serio, Andrew Thomas, Sandrine Large Synopt Survey Telescope 950 N Cherry Ave Tucson AZ 85719 USA

ISBN: (数字)9781510619548

ISBN: (纸本)9781510619548

The Large Synoptic Survey telescope (LSST) Project(1) received its construction authorization from the National Science Foundation in August 2014. The LSST telescope and Site (T&S) group has achieved significant progress in the development and delivery of an integrated telescope system solution to meet the LSST science mission requirements. The summit facility construction has been completed on Cerro Pachon in Chile, construction of the base facility and data center continues in La Serena, and many major vendor subsystem integration and verification efforts are currently in progress. This paper summarizes the status of the T&S group, which is responsible to provide the summit and base facilities and infrastructure necessary to support the wide, fast, deep LSST survey mission. The major elements of the telescope system are well into factory assembly and testing, in anticipation of shipping, integration and final acceptance testing and verification on the summit. Progress continues on the dome system assembly atop the lower enclosure of the summit facility. The M1M3 primary/tertiary and M2 secondary mirror assembly systems are undergoing integrated system testing prior to shipment to Chile. Factory testing has been achieved on the telescope mount assembly, hexapod and rotator systems, coating plant, and the auxiliary calibration telescope. Other in-house efforts including software for observatory supervisory functions, scheduling of the survey, and active optics control has also advanced. The summary status of these subsystems and future integration and verification plans are presented.

关键词： LSST telescope

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