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This document details the software requirements for the Swift X-Ray Telescope Control Processor, addressing system context, operational concepts, software components, and data handling for the mission
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How to fill out software requirements specification for
How to fill out Software Requirements Specification for the X-Ray Telescope Control Processor for the Swift Gamma Ray Burst Explorer
01
Title Page: Include the project title, version number, and date.
02
Introduction: Provide an overview of the X-Ray Telescope Control Processor and its significance to the Swift Gamma Ray Burst Explorer.
03
Scope: Define the boundaries of the software and its operational environment.
04
Definitions and Acronyms: List and explain any terms or acronyms used within the document.
05
Overall Description: Describe the general factors that affect the product and its requirements including user needs.
06
Specific Requirements: Document detailed functional and non-functional requirements, including performance, security, and usability.
07
Use Cases: Create use case diagrams to illustrate interactions between users and the system.
08
Acceptance Criteria: Define criteria for determining whether the requirements are met.
09
Dependencies: Outline any external systems or components that the software will rely on.
10
Revision History: Keep track of changes made to the document for future reference.
Who needs Software Requirements Specification for the X-Ray Telescope Control Processor for the Swift Gamma Ray Burst Explorer?
01
Software developers and engineers working on the control processor.
02
Project managers overseeing the development process.
03
Quality assurance teams responsible for testing and validation.
04
Stakeholders who require transparency about software capabilities.
05
Regulatory bodies ensuring compliance with standards and guidelines.
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People Also Ask about
What is the energy band of Swift XRT?
The XRT is a focusing X-ray telescope with a 110 cm2 effective area, 23.6 x 23.6 arcmin FOV, 18 arcsec resolution (half-power diameter), and 0.2-10 keV energy range.
How long is the Swift gamma ray observatory supposed to last?
Explorer program The burst detection rate is 100 per year, with a sensitivity ~3 times fainter than the BATSE detector aboard the Compton Gamma Ray Observatory. The Swift mission was launched with a nominal on-orbit lifetime of two years. Swift is a NASA MIDEX (medium-class Explorer) mission.
What is Swift system used for?
SWIFT works as a financial messaging system by assigning unique BIC codes for international money transfers by its member financial institutions that may be cross-border transactions. The SWIFT network is also used for securities transactions and some other purposes.
What type of telescope is the Swift Gamma Ray Burst Explorer?
The Neil Gehrels Swift Observatory Swift, launched at 17:16 GMT on 20th November 2004, is a flexible, rapid-response satellite with a wide-field of view Gamma-Ray Burst detector and narrow field X-ray and optical telescopes.
What instruments are used in the Swift telescope?
Swift is a multiwavelegth observatory carrying three instruments: the Burst Alert Telescope (BAT; Gamma Ray), the X-ray Telescope (XRT) and the Ultraviolet/Optical Telescope (UVOT). The Swift key characteristics are the rapid response to newly detected GRB and rapid data dissemination.
What is the flux limit of Swift XRT?
upper limit of 7 × 10−3 /s, or a flux limit of ≈ 2 × 10−13 erg/s/cm2. At 1LHAASO J0523+3533, we obtained 2733s of Swift-XRT observations (obs ID 00016789001 and 00016789002).
What is Swift XRT?
Overview of the Swift X-ray Telescope. The XRT is a sensitive, flexible, autonomous X-ray CCD imaging spectrometer designed to measure the position, spectrum, and brightness of gamma-ray bursts (GRBs) and afterglows over a wide dynamic range covering more than 7 orders of magnitude in flux.
What is the flux limit of Swift XRT?
upper limit of 7 × 10−3 /s, or a flux limit of ≈ 2 × 10−13 erg/s/cm2. At 1LHAASO J0523+3533, we obtained 2733s of Swift-XRT observations (obs ID 00016789001 and 00016789002).
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What is Software Requirements Specification for the X-Ray Telescope Control Processor for the Swift Gamma Ray Burst Explorer?
The Software Requirements Specification (SRS) for the X-Ray Telescope Control Processor for the Swift Gamma Ray Burst Explorer is a comprehensive document that outlines the functional and non-functional requirements, design constraints, and operational conditions for the software used to control the X-Ray Telescope within the Swift Gamma Ray Burst Explorer mission.
Who is required to file Software Requirements Specification for the X-Ray Telescope Control Processor for the Swift Gamma Ray Burst Explorer?
Typically, the development team working on the software for the X-Ray Telescope, including software engineers, project managers, and system architects, is required to file the Software Requirements Specification as part of the project documentation.
How to fill out Software Requirements Specification for the X-Ray Telescope Control Processor for the Swift Gamma Ray Burst Explorer?
To fill out the Software Requirements Specification, one should collect stakeholder requirements, define detailed functional and non-functional specifications, document use cases, and outline any interfaces with other systems. It is also important to ensure clarity and completeness to facilitate understanding among all stakeholders.
What is the purpose of Software Requirements Specification for the X-Ray Telescope Control Processor for the Swift Gamma Ray Burst Explorer?
The purpose of the Software Requirements Specification is to provide a clear and detailed description of the software functions and constraints required for the X-Ray Telescope Control Processor. It serves as a guideline for developers, ensures stakeholder alignment, and supports project management.
What information must be reported on Software Requirements Specification for the X-Ray Telescope Control Processor for the Swift Gamma Ray Burst Explorer?
The information that must be reported includes the software's functional requirements, performance metrics, design constraints, system interfaces, user interactions, compliance requirements, and any assumption or dependency details related to the software operation.
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