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

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Applying Hardware in the Loop to Designing, Integrating, Verifying and Validating the control System of New Aircraft Engines

Applying Hardware in the Loop to Designing, Integrating, Ver...

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EVI-GTI conference on Gas Turbine instrumentation

作者： G. Giliberti A. De Grassi D. Marchei C. Lai A. Ragnoni Avio Aero Loccioni Group Angeli di Rosora

ISBN: (纸本)9781785617546;9781785617539

A new experimental rig is presented, developed to design, integrate, verify and validate the control system of the all-new advanced turboprop engine, produced by GE Aviation and chosen by Textron Aviation to power its new Cessna Denali airplane. The ATP Wet Rig has been conceived to demonstrate the successful integration of engine components, to perform a functional verification at software and system level and to allow an early validation of the final engine system in a controlled and safe environment, preliminary to flight test activities. A dedicated Engine Simulator has been developed to run the ATP Engine model within a Hard Real Time framework. It provides aircraft's interfaces emulation, controls the load actuators and the electrical motors' speeds, replicates consistent loads on the components in compliance with the engine simulated status, intercepts all the EECU electrical I/O lines through appropriate "break out boxes" and physical test points, required for integration purposes. Finally, a dedicated Rig control System has been developed to communicate and to control all the equipment present in the Wet Rig. It is a distributed system responsible for supervision, test point management, data acquisition, sub-systems control, safety and equipment management, communication with the Engine Simulator.

关键词： Hardware in the Loop ATP Program Wet Rig Engine Simulation Validation

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The software Architecture to control the Cherenkov telescope Array 4

The Software Architecture to Control the Cherenkov Telescope...

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conference on software and Cyberinfrastructure for Astronomy IV

作者： Oya, I. Fuessling, M. Antonino, P. Oliveira Conforti, V. Hagge, L. Melkumyan, D. Morgenstern, A. Tosti, G. Schwanke, U. Schwarz, J. Wegner, P. Colome, J. Lyard, E. DESY Zeuthen Germany Fraunhofer IESE Kaiserslautern Germany IASF Bologna Bologna Italy DESY Hamburg Germany Univ Perugia I-06100 Perugia Italy Humboldt Univ Berlin Germany INAF Osservatorio Astron Brera Milan Italy IEEC CSIC Barcelona Spain Univ Geneva Dept Astron CH-1211 Geneva 4 Switzerland

ISBN: (纸本)9781510602052;9781510602069

The Cherenkov telescope Array (CTA) project is an initiative to build two large arrays of Cherenkov gamma ray telescopes. CTA will be deployed as two installations, one in the northern and the other in the southern hemisphere, containing dozens of telescopes of different sizes. CTA is a big step forward in the field of ground based gamma-ray astronomy, not only because of the expected scientific return, but also due to the order-of-magnitude larger scale of the instrument to be controlled. The performance requirements associated with such a large and distributed astronomical installation require a thoughtful analysis to determine the best software solutions. The array control and data acquisition (ACTL) work-package within the CTA initiative will deliver the software to control and acquire the data from the CTA instrumentation. In this contribution we present the current status of the formal ACTL system decomposition into software building blocks and the relationships among them. The system is modelled via the Systems Modelling Language (SysML) formalism. To cope with the complexity of the system, this architecture model is sub-divided into different perspectives. The relationships with the stakeholders and external systems are used to create the first perspective, the context of the ACTL software system. Use cases are employed to describe the interaction of those external elements with the ACTL system and are traced to a hierarchy of functionalities (abstract system functions) describing the internal structure of the ACTL system. These functions are then traced to fully specified logical elements (software components), the deployment of which as technical elements, is also described. This modelling approach allows us to decompose the ACTL software in elements to be created and the flow of information within the system, providing us with a clear way to identify sub-system interdependencies. This architectural approach allows us to build the ACTL system model and tra

关键词： Cherenkov telescope Array (CTA) software Architecture telescope control software Alma Common software (ACS) SysML UML

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Status report of the SRT radiotelescope control software: the DISCOS project 4

Status report of the SRT radiotelescope control software: th...

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conference on software and Cyberinfrastructure for Astronomy IV

作者： Orlati, A. Bartolini, M. Buttu, M. Fara, A. Migoni, C. Poppi, S. Righini, S. INAF Ist Radio Astron Bologna Italy INAF Osservatorio Cagliari Cagliari Italy

ISBN: (纸本)9781510602052;9781510602069

The Sardinia Radio telescope (SRT) is a 64-m fully-steerable radio telescope. It is provided with an active surface to correct for gravitational deformations, allowing observations from 300 MHz to 100 GHz. At present, three receivers are available: a coaxial LP-band receiver (305-410 MHz and 1.5-1.8 GHz), a C-band receiver (5.7-7.7 GHz) and a 7-feed K-band receiver (18-26.5 GHz). Several back-ends are also available in order to perform the different data acquisition and analysis procedures requested by scientific projects. The design and development of the SRT control software started in 2004, and now belongs to a wider project called DISCOS (Development of the Italian Single-dish control System), which provides a common infrastructure to the three Italian radio telescopes (Medicina, Noto and SRT dishes). DISCOS is based on the Alma Common software (ACS) framework, and currently consists of more than 500k lines of code. It is organized in a common core and three specific product lines, one for each telescope. Recent developments, carried out after the conclusion of the technical commissioning of the instrument (October 2013), consisted in the addition of several new features in many parts of the observing pipeline, spanning from the motion control to the digital back-ends for data acquisition and data formatting;we briefly describe such improvements. More importantly, in the last two years we have supported the astronomical validation of the SRT radio telescope, leading to the opening of the first public call for proposals in late 2015. During this period, while assisting both the engineering and the scientific staff, we massively employed the control software and were able to test all of its features: in this process we received our first feedback from the users and we could verify how the system performed in a real-life scenario, drawing the first conclusions about the overall system stability and performance. We examine how the system behaves in terms of network

关键词： SRT ACS control software Astronomical instrumentation Radiotelescope

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TCS and peripheral robotization and upgrade on the ESO 1-meter telescope at La Silla Observatory 2

TCS and peripheral robotization and upgrade on the ESO 1-met...

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

作者： Ropert, S. Suc, V. Jordan, A. Tala, M. Liedtke, P. Royo, S. Obstech SpA Ave Nueva Providencia 18811620 Santiago Chile Pontificia Univ Catolica Chile Astroengn Ctr Av Vicuna Mackenna 4860 Santiago 7820436 Chile Heidelberg Univ Zentrum Astron Max Planck Landessternwarte Konigstuhl 12 D-69117 Heidelberg Germany Pontificia Univ Catolica Chile Dept Elect Engn Av Vicuna Mackenna 4860 Santiago Chile Univ Politecn Cataluna Rambla St Nebridi 10 Barcelona 08222 Spain

ISBN: (数字)9781510602045

ISBN: (纸本)9781510602038;9781510602045

In this work we describe the robotization and upgrade of the ESO 1m telescope located at La Silla Observatory. The ESO 1m telescope was the first telescope installed in La Silla, in 1966. It now hosts as a main instrument the FIber Dual EchellE Optical Spectrograph (FIDEOS), a high resolution spectrograph designed for precise Radial Velocity (RV) measurements on bright stars. In order to meet this project's requirements, the telescope control System (TCS) and some of its mechanical peripherals needed to be upgraded. The TCS was also upgraded into a modern and robust software running on a group of single board computers interacting together as a network with the CoolObs TCS developed by ObsTech. One of the particularities of the CoolObs TCS is that it allows to fuse the input signals of 2 encoders per axis in order to achieve high precision and resolution of the tracking with moderate cost encoders. One encoder is installed on axis at the telescope and the other on axis at the motor. The TCS was also integrated with the FIDEOS instrument system so that all the system can be controlled through the same remote user interface. Our modern TCS unit allows the user to run observations remotely through a secured internet web interface, minimizing the need of an on-site observer and opening a new age in robotic astronomy for the ESO 1m telescope.

关键词： TCS telescope control telescope Robotization Remote Robotic Operation telescope Upgrade Mechanical Upgrades telescope Peripherals telescope Mechanical Backlash Correction

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Status of the array control and data acquisition system for the Cherenkov telescope Array 4

Status of the array control and data acquisition system for ...

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conference on software and Cyberinfrastructure for Astronomy IV

作者： Fuessling, Matthias Oya, Igor Balzer, Arnim Berge, David Borkowski, Jerzy Conforti, Vito Colome, Josep Lindemann, Rico Lyard, Etienne Melkumyan, David Punch, Michael Schwanke, Ullrich Schwarz, Joseph Tanci, Claudio Tosti, Gino Wegner, Peter Wischnewski, Ralf Weinstein, Amanda DESY Zeuthen Germany GRAPPA Anton Pannekoek Inst Astron Amsterdam Netherlands N Copernicus Astron Ctr Warsaw Poland IASF Bologna Bologna Italy IEEC CSIC Barcelona Spain Univ Geneva Dept Astron CH-1211 Geneva 4 Switzerland APC Paris France Humboldt Univ Berlin Germany INAF Osservatorio Astron Brera Milan Italy Univ Perugia I-06100 Perugia Italy Iowa State Univ Ames IA USA

ISBN: (纸本)9781510602052;9781510602069

The Cherenkov telescope Array (CTA) will be the next-generation ground-based observatory using the atmospheric Cherenkov technique. The CTA instrument will allow researchers to explore the gamma-ray sky in the energy range from 20 GeV to 300 TeV. CTA will comprise two arrays of telescopes, one with about 100 telescopes in the Southern hemisphere and another smaller array of telescopes in the North. CTA poses novel challenges in the field of ground-based Cherenkov astronomy, due to the demands of operating an observatory composed of a large and distributed system with the needed robustness and reliability that characterize an observatory. The array control and data acquisition system of CTA (ACTL) provides the means to control, readout and monitor the telescopes and equipment of the CTA arrays. The ACTL system must be flexible and reliable enough to permit the simultaneous and automatic control of multiple sub-arrays of telescopes with a minimum effort of the personnel on-site. In addition, the system must be able to react to external factors such as changing weather conditions and loss of telescopes and, on short timescales, to incoming scientific alerts from time-critical transient phenomena. The ACTL system provides the means to time-stamp, readout, filter and store the scientific data at aggregated rates of a few GB/s. Monitoring information from tens of thousands of hardware elements need to be channeled to high performance database systems and will be used to identify potential problems in the instrumentation. This contribution provides an overview of the ACTL system and a status report of the ACTL project within CTA.

关键词： Cherenkov telescope Array CTA Central Array control software Data Acquisition software telescope control software gamma-Ray Astronomy Cherenkov telescopes Alma Common software (ACS) OPC UA

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FalconSAT-7: A membrane space solar telescope

FalconSAT-7: A membrane space solar telescope

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

作者： Andersen, Geoff Asmolova, Olha McHarg, Matthew G. Quiller, Trey Maldonado, Carlos USAF Acad HQ USAFA DFP 2354 Fairchild DrSte 2A31 Colorado Springs CO 80840 USA

ISBN: (数字)9781510601888

ISBN: (纸本)9781510601871;9781510601888

The US Air Force Academy of Physics has built FalconSAT-7, a membrane solar telescope to be deployed from a 3U CubeSat in LEO. The primary optic is a 0.2m photon sieve - a diffractive element consisting of billions of tiny circular dimples etched into a Kapton sheet. The membrane its support structure, secondary optics, two imaging cameras and associated control, recording electronics are packaged within half the CubeSat volume. Once in space the supporting pantograph structure is deployed, extending out and pulling the membrane flat under tension. The telescope will then be directed at the Sun to gather images at H-alpha for transmission to the ground. We will present details of the optical configuration, operation and performance of the flight telescope which has been made ready for launch in early 2017.

关键词： Membrane optics space telescope diffractive optics satellite imaging

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The software system for the control and Data Acquisition for the Cherenkov telescope Array 17

The software system for the Control and Data Acquisition for...

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17th International Workshop on advanced Computing and Analysis Techniques in Physics Research (ACAT)

作者： Wegner, P. Fuessling, M. Oya, M., I Hagge, L. Schwanke, U. Schwarz, J. Tosti, G. Conforti, V Lyard, E. Walter, R. Antonino, P. Oliveira Morgenstern, A. DESY Zeuthen Germany DESY Hamburg Germany Humboldt Univ Berlin Germany INAF Osservatorio Astron Brera Milan Italy Univ Perugia Perugia Italy INAF IASF Bologna Bologna Italy Univ Geneva ISDC Geneva Switzerland Fraunhofer IESE Kaiserslautern Germany

The Cherenkov telescope Array (CTA), as the next generation ground-based very high-energy gamma-ray observatory, is defining new areas beyond those related to physics. It is also creating new demands on the control and data acquisition system. CTA will consist of two installations, one in each hemisphere, containing tens of telescopes of different sizes. The ACTL (array control and data acquisition) system will consist of the hardware and software that is necessary to control and monitor the CTA array, as well as to time-stamp, read-out, filter and store the scientific data at aggregated rates of a few GB/s. The ACTL system must implement a flexible software architecture to permit the simultaneous automatic operation of multiple sub-arrays of telescopes with a minimum personnel effort on site. In addition ACTL must be able to modify the observation schedule on timescales of a few tens of seconds, to account for changing environmental conditions or to prioritize incoming scientific alerts from time-critical transient phenomena such as gamma-ray bursts. This contribution summarizes the status of the development of the software architecture and the main design choices and plans.

关键词： software architecture

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Alignment of the James Webb Space telescope Optical telescope Element

Alignment of the James Webb Space Telescope Optical Telescop...

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

作者： Glassman, Tiffany Levi, Joshua Liepmann, Till Hahn, Walter Bisson, Gary Porpora, Dan Hadjimichael, Theo Northrop Grumman Aerosp Syst 1 Space Pk Dr Redondo Beach CA 90278 USA Harris Space & Intelligence Syst 400 Initiat DrPOB 60488 Rochester NY 14606 USA Sigmadyne Inc 803 West AveSuite 311 Rochester NY 14611 USA Ball Aerosp & Technol Corp 1600 Commerce St Boulder CO 80301 USA Goddard Space Flight Ctr 8800 Greenbelt Rd Greenbelt MD 20771 USA

ISBN: (数字)9781510601888

ISBN: (纸本)9781510601871;9781510601888

The optical telescope element (OTE) of the James Webb Space telescope has now been integrated and aligned. The OTE comprises the flight mirrors and the structure that supports them - 18 primary mirror segments, the secondary mirror, and the tertiary and fine steering mirrors (both housed in the aft optics subsystem). The primary mirror segments and the secondary mirror have actuators to actively control their positions during operations. This allows the requirements for aligning the OTE subsystems to be in the range of microns rather than nanometers. During OTE integration, the alignment of the major subsystems of the OTE structure and optics were controlled to ensure that, when the telescope is on orbit and at cryogenic temperatures, the active mirrors will be within the adjustment range of the actuators. Though the alignment of this flagship mission was complex and intricate, the key to a successful integration process turned out to be very basic: a clear, concise series of steps employing advanced planning, backup measurements, and cross checks that this multi-organizational team executed with a careful and methodical approach. This approach was not only critical to our own success but has implications for future space observatories.

关键词： James Web Space telescope Optical Integration Alignment Space telescope Infrared

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STELLA: 10 years of robotic observations on Tenerife 6

STELLA: 10 years of robotic observations on Tenerife

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

作者： Weber, Michael Granzer, Thomas Strassmeier, Klaus G. Leibniz Inst Astrophys Potsdam AIP Sternwarte 16 D-14482 Potsdam Germany

ISBN: (数字)9781510602007

ISBN: (纸本)9781510601994;9781510602007

STELLA is a robotic observatory on Tenerife housing two 1.2m robotic telescopes. One telescope is fibre-feeding a high-resolution (R=55,000) echelle spectrograph (SES), while the other telescope is equipped with a visible wide field (FOV-22' x 22') imaging instrument (WiFSIP). Robotic observations started mid 2006, and the primary scientific driver is monitoring of stellar-activity related phenomena. The STELLA control System (SCS) software package was originally tailored to the STELLA roll-off style building and high-resolution spectroscopy, but was extended over the years to support the wide-field imager, an off-axis guider for the imager, separate acquisition telescopes, classical domes, and targets-of-opportunity. The SCS allows for unattended, off-line operation of the observatory, targets can be uploaded at any time and are selected based on merit-functions in real-time (dispatch scheduling). We report on the current status of the observatory and the current capabilities of the SCS.

关键词： instrumentation: photometers instrumentation: spectrographs observatory: robotic

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The QUIJOTE TGI control system 8

The QUIJOTE TGI control system

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conference on Millimeter, Submillimeter, and Far-Infrared Detectors and instrumentation for Astronomy VIII

作者： Gomez Renasco, M. F. Martin, Y. Aguiar-Gonzalez, M. Cozar, J. Gonzalez-Cobos, N. Hoyland, R. Nunez Cagigal, M. Perez-de-Taoro, M. R. Sanchez-de la Rosa, V. Vega-Moreno, A. Viera-Curbelo, T. IAC C Via Lactea S-N E-38205 San Cristobal la Laguna Tenerife Spain

ISBN: (纸本)9781510602076;9781510602083

The QUIJOTE-CMB experiment (Q-U-I JOint TEnerife CMB experiment) has been described in previous publications. In particular, the architecture of the MFI instrument control system, the first of the three QUIJOTE instruments, was presented in [1]. In this paper we describe the control system architecture, hardware, and software, of the second QUIJOTE instrument, the TGI (Thirty GHz Instrument), which has been in the process of commissioning for a few weeks now. It is a 30 pixel 26--36 GHz polarimeter array mounted at the focus of the second QUIJOTE telescope. The polarimeter design is based on the QUIET polarimeter scheme, implementing phase switches of 90 degrees and 180 degrees to generate four states of polarisation. The TGI control system acquires the scientific signal of the four channels for each of the 30 polarimeters, sampled at 160 kHz;it controls the commutation of the 30 x 4 phase switches at 16 kHz or 8 kHz;it performs the acquisition and monitoring of the health of the complete instrument, acquiring housekeeping from the various subsystems and also controls the different operational modes of the telescope. It finally, implements a queue system that permits automation of the observations by allowing the programming of several days of observations with the minimum of human intervention. The acquisition system is based on a PXI-RT host from NI, the commutations of the phase switches are performed by a PXI-FPGA subsystem and the telescope control is based on an EtherCAT bus from Beckhoff.

关键词： CMBr polarimeter B-modes LabVIEW TwinCAT EtherCAT Real Time FPGA

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