Attachment B - Requirements Specification - L1 Series STIS 01-19-24.pdf
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- Space Weather Next L1 Series Suprathermal Ion Sensor (STIS) Federal contract opportunity
- Solicitation number
- 80GSFC23R0036
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This is a solicitation for the Space Weather Next L1 Series Suprathermal Ion Sensor (STIS). The National Aeronautics and Space Administration Goddard Space Flight Center and National Oceanic and Atmospheric Administration plan to issue a Request for Proposal for an ion spectrometer to measure solar ejecta such as coronal mass ejections and interplanetary shocks. The scope of work includes design, analysis, development, fabrication, integration, testing, verification, evaluation, launch support, and ground support equipment supply and maintenance for the instrument. Potential offerors should monitor the website for any amendments and are encouraged to notify the issuing office of their intent to submit a proposal.
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L1 Series STIS SPEC L1SERIES-STIS-REQ-0009, Revision - Effective Date: January 19, 2024 ii Check https://ipdtdms.gsfc.nasa.gov/frontmenu_dsp.cfm to verify that this is the correct version prior to use.
L1 Series Supra Thermal Ion Sensor (STIS) Requirements Specification (SPEC)
Review/Signature/Approval Page
Prepared by:
Originally approved on TDMS by: January 19, 2024 Kevin Kane Date SWO L1 Series NASA GSFC, Code 493
Reviewed by:
Charles “Hudson” DeLee Date SWO L1 Series NASA GSFC, Code 493
Approved by:
Tim Vansant Date L1 Series Project Manager NASA/GSFC, Code 493
Electronic Approval available on-line at: IPD TDMS -Instruments Project Division TDMS (nasa.gov) iii Check https://ipdtdms.gsfc.nasa.gov/frontmenu_dsp.cfm to verify that this is the correct version prior to use.
Preface
This document is under SWO Program configuration control. Once this document is approved, SWO approved changes are handled in accordance with Class I and Class II change control requirements as described in the SWO Configuration Management Procedure, and changes to this document shall be made by complete revision.
In this plan, all mandatory actions (i.e., requirements) are denoted by statements containing the term “shall.” The terms “may” or “can” denote discretionary privilege or permission; “should” denotes a good practice and is recommended but not required; “will” denotes expected outcome;
and “are/is” denotes descriptive material.
Any questions should be addressed to:
SWO Configuration Management Office
NASA/GSFC
Code 493.0 Greenbelt, MD 20771 iv Check https://ipdtdms.gsfc.nasa.gov/frontmenu_dsp.cfm to verify that this is the correct version prior to use.
Change History Log
Revision Effective Date Description of Changes Revision - January 19, 2024 This document was reviewed in CCR L1SERIES-CCR-
0052 to baseline and was approved on January 11, 2024 vii Check https://ipdtdms.gsfc.nasa.gov/frontmenu_dsp.cfm to verify that this is the correct version prior to use.
Table of Contents
1 INTRODUCTION
1.1 General Information
1.2 Scope
2 APPLICABLE DOCUMENTS
3 CONTRACT DESCRIPTION
3.1 STIS Description
3.2 Ground Support Equipment Description
4 FUNCTIONAL/PERFORMANCE REQUIREMENTS
4.1 STIS Performance Requirements
4.1.1 Maximum and Minimum Flux
4.1.2 Flux Measurement Range
4.1.3 Accuracy
4.1.4 Field of View (FOV)
4.1.5 Refresh Rate and Latency
4.1.6 Response Stability
4.2 Resource Allocations
4.2.1 Mass Allocation
4.2.2 Physical Envelope
4.2.3 Operational Power Allocation
4.2.4 Peak Operational Power Allocation
4.2.5 Survival Heater Power Allocation
4.2.6 Telemetry
4.2.7 Transient Magnetic Field
4.2.8 Static Magnetic Field
4.3 STIS Operating Modes
4.3.1 In-Flight Calibration
4.3.2 Mode Transitions
4.3.3 Deterministic Power-on Configuration
4.3.4 Safe Mode
4.3.4.1 Entry into Safe Mode
4.3.5 Fail-safe Recovery Mode
4.3.6 Normal Operational Mode
4.3.7 On-Orbit Operations
4.3.8 Station Keeping
4.3.9 Activation
4.4 Instrument Data Availability
4.5 Power
4.5.1 Voltage Range
4.5.2 Abnormal Voltages
4.5.3 Sudden Removal of Power
4.5.4 Over-Current Protection
4.5.5 Primary Power Return Ground
4.5.6 Turn-on Current Transients
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4.6 Electrical Grounding
4.6.1 Primary Power DC Isolation
4.6.2 Survival Power Isolation
4.6.3 Internally Generated Secondary to Primary DC Isolation
4.6.4 Internally Generated Secondary Return
4.6.5 Mechanical Contact Resistance
4.6.6 Grounding
4.6.7 Connector DC Resistance
4.7 Signal And Data Interfaces
4.7.1 Passive Analog Telemetry
4.7.2 Data Signal Interface
4.7.2.1 Telemetry Source Packet Format
4.7.2.2 Command Source Packet Format
4.7.3 Clock Signal Interface
4.7.4 Command and Housekeeping telemetry
4.7.5 Commands for Autonomous Functions
4.7.6 Limits and Triggers
4.7.7 On-Board Processor Reset
4.7.8 Micro-switches
4.8 Flight Software
4.8.1 Flight Load Non-volatile Memory
4.8.2 Software Updates
4.8.3 Software Table Updates
4.8.4 Flexibility and Ease of Software Modification
4.8.5 Version Identifiers
4.8.6 Warm Restart
4.8.7 Memory Tests
4.8.8 Memory Dump
4.8.9 Fault Detection and Correction Control
4.8.10 Health and Safety Monitoring
5 PHYSICAL REQUIREMENTS
5.1 Interface and Design Units and Exclusions
5.2 Mass Properties Accuracy
5.2.1 Instrument Mass Accuracy
5.2.2 Center of Mass Location
5.2.3 Center of Mass Accuracy
5.2.4 Determination of Moments and Products of Inertia
5.3 Mounting
5.3.1 Surface Flatness
5.3.2 Method
5.4 Coordinate System and Alignment
6 ENVIRONMENTAL REQUIREMENTS
6.1 Mechanical Factors of Safety
6.2 Quasi-Static Acceleration
6.3 Frequency Requirement
6.3.1 Fundamental Launch Frequencies
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6.4 Vibration
6.4.1 Sinusoidal Vibration
6.4.2 Random Vibration
6.5 Shock
6.6 Acoustics
6.7 Transportation
6.7.1 Transportation Cleanliness
6.8 Pressure
6.8.1 Operating Pressure Range
6.8.2 Maximum Depressurization Rate
6.8.3 Launch Vehicle (LV) Environmental Control System (ECS) Impingement
6.9 On-Orbit Dynamic Environment
6.9.1 Dynamic Linear Acceleration
6.9.2 Dynamic Angular Acceleration
6.10 Thermal Requirements
6.10.1 Flight Interface Design Temperature Limits
6.11 Charged Particle Radiation Requirements
6.11.1 Definitions
6.11.2 Radiation Hardness Assurance
6.11.2.1 Single-Event Effect Rate Calculations
6.11.3 Charging Environment
6.11.4 Total Ionizing Dose
6.11.5 Displacement Damage Dose Levels
6.11.6 Single Event Effects
6.11.7 Solar Cycle Performance
6.11.8 Solar Particle Event Operations
6.11.9 Solar Flare Survival
7 CONTAMINATION CONTROL
7.1 Surface Cleanliness Requirements
7.2 Contamination Generation
7.2.1 Particulate Generation
7.2.2 Molecular Contamination Generation
7.2.2.1 Molecular Material Restrictions
7.3 Vacuum Bakeouts
7.4 Contamination Analyses
7.5 Venting Requirements
7.6 Instrument Purging
7.7 Cleanability and Protection
7.8 Electrostatic Cleanliness
7.8.1 Conductive Surface Ground Path
7.8.2 Conductive Surface Resistivity
7.8.3 Closeout of Gaps and Apertures
7.8.4 Exposed Harness Specific Requirements
7.8.5 Thermal Blankets
8 DESIGN AND CONSTRUCTION REQUIREMENTS
8.1 Electrical
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8.1.1 Test Sensors
8.1.2 MGSE Grounding
8.1.3 Connector Specifications
8.1.3.1 Contact Derating
8.1.3.2 Redundant Contact Derating
8.1.3.3 Signal Segregation
8.1.3.4 Test and Flight Signal Isolation
8.1.4 Test Interfaces
8.1.4.1 Facility-Induced Noise
8.1.4.2 Facility-Induced ESD GSE Malfunction
8.1.4.3 Facility-Induced GSE Malfunction
8.1.5 Mitigation of Internal Charging
8.1.5.1 Mitigation Strategies for Internal Charging
8.1.5.2 Floating Conductors
8.1.5.3 Dielectric Structures
8.2 Safety
8.3 Electromagnetic Compatibility
8.3.1 Conducted Emissions
8.3.1.1 Applicability of Conducted Emissions
8.3.1.2 CE101 – Differential Mode Conducted Emissions Limits
8.3.1.3 CE03 – Differential Mode Conducted Emissions Limits
8.3.1.4 CMBCE – Common Mode Bulk Conducted Emissions Limits
8.3.2 Conducted Susceptibility
8.3.2.1 Applicability of Conducted Susceptibility
8.3.2.2 CS101 – Conducted Susceptibility Limit
8.3.2.3 CS114 – Conducted Susceptibility Differential Mode Limit
8.3.2.4 CS114 – Conducted Susceptibility, Common Mode, Power Cables
8.3.2.5 CS06 – Conducted Susceptibility, Transients Limits
8.3.2.6 CS115 - Conducted Susceptibility, Bulk Cable Injection, Impulse Excitation ... 67
8.3.3 Radiated Emissions
8.3.3.1 RE102 - Electric Field Emissions Limits
8.3.4 Radiated Susceptibility
8.3.4.1 RS103 - Radiated Susceptibility, Electric Field, Launch Limit
8.3.4.2 RS103 - Radiated Susceptibility, Electric Field, On-Orbit Limit
8.4 Identification and Marking
8.5 Workmanship
8.5.1 Connectors
8.6 Reliability and Mission Lifetime
8.6.1 Mission Life
8.6.2 Operating Time
8.6.3 Trouble-Free Time
8.7 Ground Handling
8.7.1 Ground Support Equipment (GSE) Design
8.7.2 Lifting Hardware
8.7.3 Manual Lifting Hardware
8.7.4 GSE Cleanliness
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8.7.5 GSE Bakeout
8.7.6 Test Harness
8.8 Interface Documentation
8.8.1 Mechanical Interface
8.8.2 Electrical Interface
8.8.3 Data Interface
9 MECHANICAL DESIGN REQUIREMENTS
9.1 Structural Requirements
9.1.1 Component Fatigue
9.1.2 Fracture Control Requirements
9.2 Fastening Systems
9.2.1 Factors of Safety
9.2.2 Supplemental Factor
9.2.3 Ultimate Design Loads
9.2.4 Yield Design Loads
9.2.5 Design Separation Load
9.2.6 Fastener Locking and Retention
9.2.6.1 Thread Engagement
9.2.6.2 Locking Feature Verification
9.2.6.3 Locking Feature Installation
9.2.6.4 Snap Ring and Cotter Pin Use Limitation
9.2.6.5 Snap Ring and Cotter Pin Use
9.2.6.6 Liquid Locking Compounds
9.2.6.6.1 Verification
9.2.6.7 Locking Features
9.2.6.7.1 Specification
9.2.6.7.2 Validation
9.2.7 Installation Torque Specification and Control
9.2.7.1 Installation Torque Range
9.2.7.2 Running Torque Identification
9.2.8 Fastened Joints Criteria
9.2.8.1 Minimum and Maximum Preload
9.2.8.2 Analysis Addressing Potential Rupture
9.2.8.3 Ultimate Strength Analysis
9.2.8.3.1 Applied Shear Loading
9.2.8.3.2 Shear Loading
9.2.8.4 Simultaneous Applied Tensile and Shear Loads
9.2.8.5 Allowable Yield Tensile Load
9.2.8.6 Separation Analysis
9.2.8.7 Seal Analysis
10 LOGISTICS
10.1 I&T Deliverables
10.2 Ground Support Equipment
10.2.1 Electrical System Test Equipment
10.2.2 Instrument Emulator
10.3 Transportation Equipment
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10.3.1 Shipping Container
11 VERIFICATION REQUIREMENTS
11.1 Verification Methods
11.1.1 Inspection
11.1.2 Analysis
11.1.3 Test
11.1.4 Demonstration
11.2 Inspection Requirements
11.2.1 Visual Inspection
11.2.2 Physical Measurement
11.2.3 Documentation Search
11.3 Analysis Requirements
11.4 Test Requirements
11.4.1 Definitions
11.4.2 Test Factors
11.4.3 Test Tolerances
11.4.4 Test Restrictions
11.4.4.1 Failure During Tests
11.4.4.2 Modification of Hardware
11.4.4.3 External Adjustment
11.4.4.4 Re-Test Requirements
11.4.4.5 Configuration
11.5 Required Tests
11.5.1 Performance Tests
11.5.1.1 Comprehensive Performance Test
11.5.1.2 Limited Performance Test
11.5.1.3 Abbreviated Functional Test
11.5.2 Mass Properties Measurement
11.5.3 Static Loads/Strength Test
11.5.3.1 Sine Burst
11.5.3.2 Static Pull
11.5.4 Sine Sweep Survey
11.5.5 Sine Vibration
11.5.6 Random Vibration
11.5.7 Acoustic Test
11.5.8 Shock
11.5.9 Thermal Vacuum Bake-out
11.5.10 Thermal Vacuum Test
11.5.10.1 Thermal Vacuum Test Parameters
11.5.10.2 Thermal Vacuum Test Profile
11.5.11 Magnetics Test
11.5.12 Harness Tests
11.5.13 EMI/EMC Tests
APPENDIX A ABBREVIATIONS AND ACRONYMS
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List of Figures
Figure 1 Telemetry Source Packet Definition Figure 2 Time Code Format Figure 3 Command Source Packet Figure 4 Spacecraft Time Message Packet Figure 5 Spacecraft Reference System Figure 6 Sine Vibration Environment Figure 7 Random Vibration Environment Figure 8 Candidate LV Shock Environment Figure 9 L1 Series Acoustic Design Envelope (TBR) Figure 10 Allowable Analytical, Flight Operation, Flight Acceptance Test, and Qualification
(ProtoFlight or Prototype) Test Temperature Ranges Figure 11 Total Ionizing Dose-Depth Curve Figure 12 Displacement Damage Dose in Silicon vs. Shielding Thickness Dose-Depth Curve 37 Figure 13 Displacement Damage Dose in Gallium Arsenide Dose-Depth Curve Figure 14 LET Spectrum of GCR Background Figure 15 Solar LET Spectrum Background Figure 16 Solar Proton Background Spectra Figure 17 Peak Solar Particle Event Flux Figure 18 Peak Solar Proton Flux Figure 19 CE101/CE03 Differential Mode Conducted Emissions Limits Figure 20 Common Mode Bulk Conducted Emissions Limit Figure 21 Power Lead Conducted Susceptibility (CS101) Voltage Limit Figure 22 Conducted Susceptibility Power Limit (30 Hz to 150 kHz) Figure 23 Conducted Susceptibility, Power Leads, 150 kHz to 50 MHz Limit Figure 24 Conducted Susceptibility, Power Leads, 150 kHz to 50 MHz Current Limits Figure 25 Common Mode Conducted Susceptibility Calibration Limit Figure 26 Conducted Susceptibility Transient Waveform Figure 27 CS115 Impulse Waveform Figure 28 Unit Level RE102 Radiated Electric Field Emission Limits Figure 29 Thermal Vacuum Profile
List of Tables
Table 1 Applicable Documents (TBR) Table 2 Factors of Safety1,2 Table 3 Design Limit Loads Table 4 Candidate LV Shock Environment Table 5 L1 Series Acoustic Design Envelope (TBR) Table 6 Transportation Loads (TBR) Table 7 Orbit Thermal Parameters Table 8 Total Ionizing Dose vs. Shielding Thickness Table 9 Displacement Damage Dose in Silicon vs. Shielding Thickness Table 10 Displacement Damage Dose in Gallium Arsenide vs. Shielding Thickness xiv Check https://ipdtdms.gsfc.nasa.gov/frontmenu_dsp.cfm to verify that this is the correct version prior to use.
Table 11 LET Spectrum of GCR Background Table 12 Solar Background LET Spectrum Table 13 Solar Proton Background Flux Table 14 Peak Solar Particle Event Flux Table 15 Peak Solar Proton Flux Table 16 Lifetime Contamination Requirements Table 17 Thermal Blanket Area vs. Grounding Tabs Table 18 Emission and Susceptibility Requirements Table 19 RS103 Radiated Susceptibility Levels Table 20 Test Factors and Durations Table 21 Thermal Vacuum Test Parameters
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1 INTRODUCTION
1.1 General Information
1.2 Scope
This specification describes the performance and electrical, mechanical, environmental, and verification testing requirements for a space-qualified Suprathermal Ion Sensor (STIS) for the Space Weather Next L1 Series Mission.
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2 APPLICABLE DOCUMENTS
The following documents and drawings in effect on the day this specification was signed shall apply to the fabrication and to the electrical, mechanical, and environmental requirements of the STIS to the extent specified herein. In the event of conflict between this specification and any referenced document, this specification will govern, with the exception of the L1 Series STIS Statement of Work (L1SERIES-STIS-SOW-0004), in which case the Statement of Work takes precedence.
The following is a list of the applicable specifications and publications.
Table 1 Applicable Documents (TBR)
Document Number Title
L1SERIES-STIS-SOW-
L1 Series Suprathermal Ion Sensor (STIS) Statement of Work
(SOW)
L1SERIES-STIS-REQ-
L1 Series Suprathermal Ion Sensor (STIS) Contract Deliverables Requirements List (CDRL)
ANSI/TIA/EIA-422
Revision -B
Electrical Characteristics of Balanced Voltage Digital Interface Circuits
ANSI/TIA/EIA-644
Revision -A-2001
Electrical Characteristics of Low Voltage Differential Signaling (LVDS) Interface Circuits
NFPA 70 National Fire Protection Association National Electric Code NASA-STD-5001B Structural Design and Test Factors of Safety for Spaceflight
Hardware NASA-STD-8719.24 NASA Expendable Launch Vehicle Payload Safety Requirements NASA-STD-6016C Standard Materials and Processes Requirements for Spacecraft NASA-HDBK-7005 Dynamic Environment Criteria NASA-STD-7001 Payload Vibroacoustic Test Criteria IEST-STD-CC-1246E Product Cleanliness Levels and Contamination Control Program ASTM E-595-07 Standard Test Method for Total Mass Loss and Collected Volatile
Condensable Materials from Outgassing in a Vacuum Environment
MIL-DTL-5541 Chemical Conversion Coatings on Aluminum and Aluminum Alloys
MIL-A-8625F Anodic Coatings for Aluminum and Aluminum Alloys EEE-INST-002 Instructions for EEE Parts Selection, Screening, Qualification, and Derating MIL-STD-461G Military Standard, Electromagnetic Emission and Susceptibility
Requirements for the Control of Electromagnetic Interference
(EMI)
GSFC-STD-7000B General Environmental Verification Standard (GEVS) NASA-STD-5019A Fracture Control Requirements for Spaceflight Hardware NASA-STD-5020B Requirements for Threaded Fastening Systems in Spaceflight
Hardware NASA-STD-5017B Design and Development Requirements for Mechanisms
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NASA-HDBK-4002B Mitigating In-Space Charging Effects—A Guideline FAA AC 20-71 Federal Aviation Administration Advisory Circular (AC) 20-71, “Dual Locking Devices on Fasteners".
NASM 33540 Safety Wiring, Safety Cabling, Cotter Pinning, General Practices for SAE AS567 Safety Cable, Safety Wire, Key Washers, and Cotter Pins for
Propulsion Systems, General Practices for Use of MSFC-STD-3029A Guidelines for the Selection of Metallic Materials for Stress
Corrosion Cracking Resistance in Sodium Chloride Environments MIL-STD-462, Notice 4 Electromagnetic Interference Characteristics, Measurement of, 1
May 1970 ISO 14644-1:2015 Part 1: Classification of air cleanliness by particle concentration ISO 14644-3: 2005 Cleanrooms and associated controlled environments -- Part 3:
Test methods CCSDS 133.0-B-2 Space Packet Protocol, Blue Book, Issue 2, June 2020 CCSDS 301.0-B-4 Time Code Formats. Blue Book. November 2010
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3 CONTRACT DESCRIPTION
3.1 STIS Description
The Suprathermal Ion Sensor (STIS) is an ion spectrometer device that measures ions across a broad range of energies to characterize solar ejecta including Coronal Mass Ejections (CMEs), co-rotating interaction regions (CIRs) and interplanetary shocks. In particular, STIS is a low energy charged particle detector that is capable of measuring the ion flux population as a function of energy. This ion population with energies higher than that of the bulk plasma are produced by local solar acceleration as well as acceleration from a CME shock front. Analysis of these spectra can aid in estimating the arrival time and strength of CME shocks.
The STIS contract includes the delivery of two (2) Flight Models (FM) instrument and one (1) Engineering Development Unit (EDU), flight harnesses between instrument boxes, if applicable, and enough spares and built-up sub-assemblies for one additional FM, an electronics unit, and harnesses.
3.2 Ground Support Equipment Description
The STIS contract includes the delivery of two (2) sets of the Electrical System Test Equipment (ESTE), four (4) STIS Emulators (STISEs), one (1) Flight Software Development Environments (FSDEs), and one (1) Ground Processing Development System (GPDS). Additionally, Mechanical Ground Support Equipment (MGSE) such as lifting fixtures/handles, shipping containers, purge carts, drill templates, test fixtures, non-flight protective covers, etc. are included in the delivery. Electrical Ground Support Equipment includes, but is not limited to, test cables and break-out boxes as required.
Ground Support Equipment is necessary to operate the instrument during spacecraft testing.
Supplying this equipment is considered part of the delivery for the instrument. More information is provided in the Contract Deliverable Requirement List (CDRL).
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4 FUNCTIONAL/PERFORMANCE REQUIREMENTS
This section defines the functional and performances requirements for the L1 Series STIS.
The requirements in this Specification pertain to the STIS "system", which may include all instrument hardware, software, and ground processing algorithms. The STIS contractor is not responsible for the operational ground system, but certain specifications will require ground processing after collection but before data distribution for which the contractor is responsible for defining.
4.1 STIS Performance Requirements
4.1.1 Maximum and Minimum Flux
STISPEC-22: The STIS shall provide in situ solar wind suprathermal ion flux observation with flux observations in the following range (particles/[cm^2 sec sr keV]):
Minimum Flux: 2.48x10^2 * E(keV)^-1.6
Maximum Flux: 1.01x10^7 * E(keV)^-1.6
4.1.2 Flux Measurement Range
STISPEC-27: The STIS shall provide in situ solar wind suprathermal ion flux observation with observational energy range of 50 to 2,000 keV.
STISPEC-28: The STIS shall determine the differential ion fluxes in sufficient evenly spaced logarithmic energy bands to meet the accuracy requirement defined in section 4.1.3.
4.1.3 Accuracy
STISPEC-30: The STIS shall provide heliospheric suprathermal ion flux, jion, observations with flux accuracy over the required energy range as follows:
a) ±100% of flux at the minimum flux, jion, min, specified in STISPEC-22, and ±20% at an intermediate flux, jion, mid = 50,048 * E(keV)^-1.6 #/cm2/s/sr/keV;
b) linearly interpolated accuracy for fluxes in the low range, jion, min < jion < jion, mid;
c) ±20% for fluxes in the high range, jion > jion, mid.
STISPEC-928: The STIS instrument shall provide >3 bands in a logarithmic bin per energy decade.
4.1.4 Field of View (FOV)
STISPEC-32: The spacecraft shall provide the STIS a FOV that is 80 degrees in the ecliptic by 60 degrees centered 50 degrees in the ecliptic off of the sun-earth line in the “ahead” direction
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(the ahead direction is the direction the earth travels in the ecliptic). The unit vector for the centroid of the FOV of the instrument should be (cos 50 degrees, 0, sin 50 degrees) or (0.643, 0, 0.766).
The spacecraft will provide an unobstructed field of view.
4.1.5 Refresh Rate and Latency
STISPEC-35: The STIS shall provide in situ solar wind suprathermal ion flux observation at a refresh rate of 300 sec.
STISPEC-36: The STIS shall provide in situ solar wind suprathermal ion flux observation that meet an overall latency requirement of 5 minutes.
STISPEC-37: The STIS ground processing algorithms contribution to data latency of the STIS Level 1b algorithm output shall be ≤ 236 seconds.
4.1.6 Response Stability
STISPEC-39: The STIS instrument shall provide monotonically increasing fluxes up to three times the maximum flux for a given energy range.
4.2 Resource Allocations
4.2.1 Mass Allocation
STISPEC-42: The STIS, including the sensor unit, electronics, box, and sensor standoff bracket (if required), and the intra-instrument harness, shall have a combined mass of less than or equal to 5.2 kg.
STISPEC-2024: The STIS instrument mass margin shall comply with GSFC-STD-1000H Rule 1.06.
4.2.2 Physical Envelope
STISPEC-44: The STIS volume (length*width*height), including the sensor unit, electronics box, mounts, sensor standoff bracket (if required), intra-instrument harness, thermal blankets, and connectors, for both stowed and operational configurations shall have dimensions that do not exceed a total volume of 27,000 cm3. These dimensions pertain to both static and dynamic envelopes of the instrument.
STISPEC-45: The STIS maximum dimension shall be less than 30 cm.
4.2.3 Operational Power Allocation
STISPEC-47: The STIS shall have a nominal operational power of ≤4W.
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4.2.4 Peak Operational Power Allocation
STISPEC-49: The STIS shall have a peak (instantaneous) operational power of ≤ 8 W for a duration of 20 msec at 30 V.
4.2.5 Survival Heater Power Allocation
STISPEC-51: The STIS shall have a survival heater power consumption of ≤ 4W (TBR).
4.2.6 Telemetry
STISPEC-53: The STIS instrument science and engineering data rate, including all overhead associated with Consultative Committee for Space Data Systems (CCSDS) packetization by the instrument at the spacecraft interface, shall not exceed 1.0 kilobits per second (kbps) averaged over any 4.5 second period.
4.2.7 Transient Magnetic Field
STISPEC-55: The STIS instrument shall limit varying magnetic field less than 5 Hz to less than 4 nT zero-to-peak in any axis 1 meter from any face of the unit for any operating mode and changing configurations.
4.2.8 Static Magnetic Field
STISPEC-57: The STIS units shall limit the static magnetic field to less than 1 nT in any axis
3.5 meters from any face of the unit for any operating mode.
4.3 STIS Operating Modes
STISPEC-59: The STIS current operating mode shall be identified by a flag in its telemetry stream.
4.3.1 In-Flight Calibration
STISPEC-61: The STIS shall provide an in-flight calibration mode that provides a test input to support calibration and testing both on the ground and in space.
STISPEC-63: The STIS in-flight calibration shall be both self-terminating and able to be terminated by a ground command.
4.3.2 Mode Transitions
STISPEC-65: The instrument shall transition from the current mode to any other mode without causing damage to itself.
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4.3.3 Deterministic Power-on Configuration
STISPEC-67: The instrument shall initialize upon power-up into a predetermined configuration.
STISPEC-929: The STIS initialization configuration shall not enable any high voltage power supplies.
STISPEC-930: High voltage power supplies shall be enabled by ground command only.
4.3.4 Safe Mode
STISPEC-69: The instrument shall provide a Safe Mode. Safe mode is an operating mode of the instrument during which all non-essential subsystems are shut down and only essential functions are active. Safe mode represents a configuration in which the instrument is thermally, mechanically, and optically “safe” without receiving commands from the Spacecraft.
STISPEC-70: In safe mode any STIS high-voltage power supplies shall be disabled.
STISPEC-2025: High voltage power supplies shall be re-enabled by ground command only.
STISPEC-71: The instrument shall be capable of remaining in a safe configuration for at least 168 hours without ground intervention.
4.3.4.1 Entry into Safe Mode
STISPEC-73: The instrument shall enter Safe Mode upon detection of internal faults that are capable of causing damage to the instrument.
The L1 Series spacecraft will monitor up to three (TBR) analog instrument health and safety parameters defined by the STIS contractor and command the STIS into safe mode when any of those key values have been exceeded.
The L1 Series spacecraft will monitor up to 12 (TBR) digital telemetry points that are part of the normal instrument generated data stream for instrument health and safety parameters defined by the STIS contractor and command the STIS into safe mode when any of those key values have been exceeded.
4.3.5 Fail-safe Recovery Mode
STISPEC-2027: The instrument shall provide a failsafe recovery mode dependent on a minimal hardware configuration capable of accepting and processing a minimal command subset sufficient to load and dump memory.
4.3.6 Normal Operational Mode
STISPEC-79: In normal operational mode, the STIS shall be in a fully functional configuration in which designed measurements are made in accordance with the performance requirements listed in section 4.1 of this document and are available to be sent to the spacecraft for downlink.
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4.3.7 On-Orbit Operations
STISPEC-81: The STIS shall operate normally, within specification, while flying aboard a 3-axis stabilized spacecraft with orbital limit constraints as stated in this specification.
4.3.8 Station Keeping
STISPEC-83: The STIS shall continuously operate during all spacecraft maneuvers.
4.3.9 Activation
STISPEC-86: The instrument shall require no active commanding prior to fourteen (14) days after launch.
4.4 Instrument Data Availability
STISPEC-2029: The STIS shall limit on-orbit calibrations to no more than four (4) calibrations per year with each calibration lasting no more than 30 minutes.
STISPEC-2030: The instrument shall be capable of maintaining nominal observation mode without ground interaction for a minimum of 4 days.
4.5 Power
The spacecraft will supply one operational power bus for normal instrument operation.
The spacecraft will supply one survival power bus for the instrument survival heaters.
4.5.1 Voltage Range
STISPEC-89: The instrument shall operate over the operational bus voltage range of +26 to +34 VDC at the primary power inputs for all expected load conditions (except when turned off).
STISPEC-965: The instrument survival heaters shall operate over the voltage range of +24 to +34 VDC at the power inputs for all expected load conditions.
4.5.2 Abnormal Voltages
STISPEC-91: The instrument shall survive without performance degradation after indefinite exposure to an anomalous voltage range of 0 to +40 VDC.
4.5.3 Sudden Removal of Power
STISPEC-95: The instrument shall meet its performance requirements without degradation after exposure to an abrupt, unannounced removal of power.
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4.5.4 Over-Current Protection
STISPEC-97: The instrument shall not use non-resetting over-current protection (i.e., fuses) internal to the unit.
4.5.5 Primary Power Return Ground
STISPEC-99: The instrument shall provide a dedicated Primary Power return in the same connector as the primary power.
4.5.6 Turn-on Current Transients
STISPEC-101: The instrument shall meet its performance requirements without degradation after exposure to a turn-on input voltage (0 – 34 VDC) with a rise time of 500µs.
Note: The spacecraft bus will not drop below 26 V during instrument turn on.
4.6 Electrical Grounding
4.6.1 Primary Power DC Isolation
STISPEC-111: The instrument primary power interfaces, primary power and primary power returns, shall be isolated from the unit chassis by a DC resistance of greater than or equal to 10 Megaohms.
4.6.2 Survival Power Isolation
STISPEC-113: The instrument survival heater power interfaces shall be isolated from the unit chassis by a DC resistance of greater than or equal to 10 Megaohms.
4.6.3 Internally Generated Secondary to Primary DC Isolation
STISPEC-115: Secondary power inputs shall be isolated from primary power by a DC resistance of greater than 10 Megaohms.
4.6.4 Internally Generated Secondary Return
STISPEC-117: The instrument shall reference its secondary returns (power and signal grounds) to the unit chassis ground by connecting them at one or more places.
4.6.5 Mechanical Contact Resistance
STISPEC-119: The DC resistance of the mechanical contact between two conductive mating surfaces (internal to the unit) shall be less than or equal to 2.5 milliohms DC resistance.
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4.6.6 Grounding
STISPEC-2033: The DC resistance between the STIS chassis and the observatory chassis shall be ≤ 2.5 milliohms.
STISPEC-122: The STIS shall provide a ground lug for a grounding strap to be attached from the STIS chassis for connection to the spacecraft conductive structure.
STISPEC-123: The grounding lug location on the STIS instrument chassis or the tie points in contact with the ground strap shall be defined in the Mechanical Interface Control Drawing (MICD). The ground lug contact area must remain free of any material finish that may affect the reliability of the ground connection and will be shown in the MICD.
4.6.7 Connector DC Resistance
STISPEC-125: STIS connector backshells shall be electrically connected to Electronic Unit chassis with a DC resistance ≤ 2.5 milliohms.
4.7 Signal And Data Interfaces
4.7.1 Passive Analog Telemetry
STISPEC-128: The STIS shall utilize no more than six (TBR) analog signals to monitor critical temperature points when the instrument is powered off.
4.7.2 Data Signal Interface
The spacecraft will provide two data signal interface feeds to the instrument for command and telemetry. The spacecraft will also provide an interface line for a Pulse Per Second (PPS) time pulse.
STISPEC-130: The instrument data transfer interface to or from the spacecraft shall either use a serial Universal Asynchronous Receiver Transmitter (UART) using ANSI/TIA/EIA-422-B Electrical Characteristics of Balanced Voltage Differential Interface Circuits, or ANSI/TIA/EIA- 644-A-2001 Electrical Characteristics of Low Voltage Differential Signaling (LVDS) Interface Circuits.
4.7.2.1 Telemetry Source Packet Format
STISPEC-132: The instrument shall transfer all data to the spacecraft using the CCSDS 133.0- B-2 Section 4.1 Protocol Data Unit definition shown in the Telemetry Source Packet Definition Figure 1.
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Figure 1 Telemetry Source Packet Definition
STISPEC-134: The instrument telemetry Source packets shall be variable length with a maximum data zone of 8192 octets including Secondary Header.
STISPEC-135: The instrument shall set the telemetry source packet Secondary Header Flag to the value 1.
STISPEC-136: The instrument shall set the Telemetry Source Packet Sequence Flags to the value of 11.
Note: Segmentation services are not permitted.
STISPEC-138: The instrument shall set the Telemetry Source Packet Time Code per CCSDS 301.0-B-4 Time Code Formats, Day Segmented format in the Time Code Format Figure 2.
Figure 2 Time Code Format
Note: The P-Field is implied and not included in the actual time message.
The spacecraft on-board reference time will be Coordinated Universal Time (UTC).
4.7.2.2 Command Source Packet Format
STISPEC-143: The instrument shall receive all data from the spacecraft formatted per CCSDS 133.0-B-2 Section 4.1 Protocol Data Unit definition shown in the Command Source Packet Definition Figure 3.
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Figure 3 Command Source Packet
STISPEC-145: The instrument Command Source Packets shall be variable length with a maximum data zone of 1013 octets.
STISPEC-146: The instrument shall receive Command Source Packet with Secondary Header Flag set to the value 0.
STISPEC-147: The instrument shall receive Command Source Packet with the Sequence Flags set to the value of 11.
Note: Segmentation services are not permitted.
4.7.3 Clock Signal Interface
STISPEC-150: The instrument shall receive a Pulse Per Second (PPS) time pulse from spacecraft clock line by the interface defined in section 4.7.2 of this document.
The Spacecraft will maintain Spacecraft time correlation to within +/- 0.95 sec of UTC and will provide the instrument a 1 PPS with a time code message.
STISPEC-152: The instrument shall receive from the spacecraft a time code message on the data line as defined in Spacecraft Time Message Packet Figure 4. The time code message is the time applicable to receipt of the 1 PPS.
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Figure 4 Spacecraft Time Message Packet
4.7.4 Command and Housekeeping telemetry
STISPEC-155: The instrument shall provide command and housekeeping telemetry functions in all powered modes.
4.7.5 Commands for Autonomous Functions
STISPEC-157: The instrument shall execute commands to individually enable and disable each autonomous function.
4.7.6 Limits and Triggers
STISPEC-159: The instrument autonomous limits and triggers shall be changeable by command.
4.7.7 On-Board Processor Reset
STISPEC-161: The instrument On-Board Processor shall be reset by command.
STISPEC-162: An autonomous power-on reset occurrence shall be unambiguously identifiable via telemetry.
Note: This does not imply real-time telemetry as the reset is occurring.
4.7.8 Micro-switches
STISPEC-164: Micro-switches shall be used for information only and not used to initiate on-board autonomous activity or as an on-board interlock.
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4.8 Flight Software
4.8.1 Flight Load Non-volatile Memory
STISPEC-167: The instrument flight software image shall be contained in its entirety in non-volatile memory at launch.
4.8.2 Software Updates
STISPEC-169: The flight software modules shall be reprogrammable.
4.8.3 Software Table Updates
STISPEC-172: Instrument configuration data (e.g., Table Loads or Configuration Parameters) shall be reprogrammable during integration and test phases and on-orbit without computer restart.
STISPEC-173: Modified instrument configuration data (e.g., Table Loads or Configuration Parameters) shall be committed to operational use by ground command.
4.8.4 Flexibility and Ease of Software Modification
STISPEC-175: The instrument flight software shall be deterministic in terms of scheduling and prioritization of critical processing tasks to ensure their timely completion.
STISPEC-176: Instrument configuration data (e.g., Table Loads or Configuration Parameters) shall be referenced such that data can be loaded and dumped by the ground without reference to memory address.
STISPEC-177: The definition of instrument commands within the ground database (excluding memory diagnostic/load commands) shall not be dependent on physical memory addresses within the flight software.
4.8.5 Version Identifiers
STISPEC-179: The instrument software and firmware versions shall each have an internal identifier (embedded in the executive program) that can be included in the instrument engineering data.
STISPEC-180: This software identifier shall be configuration management controlled.
4.8.6 Warm Restart
STISPEC-182: The instrument flight software shall provide a restart by command with preservation of instrument configuration data and memory tables.
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4.8.7 Memory Tests
STISPEC-184: The instrument flight software shall provide a mechanism to verify the contents of all memory areas.
4.8.8 Memory Dump
STISPEC-186: The instrument flight software, and associated on-board computer hardware, shall provide the capability to dump any memory location.
STISPEC-187: The flight software memory dump capability shall not disturb normal operations and instrument data processing.
4.8.9 Fault Detection and Correction Control
STISPEC-189: If applicable, the instrument shall provide the capability to enable and disable any internal Fault Detection and Correction (FDC) features.
4.8.10 Health and Safety Monitoring
STISPEC-191: The instrument flight software shall provide health and safety monitoring, including memory checksum and watchdog timer.
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5 PHYSICAL REQUIREMENTS
5.1 Interface and Design Units and Exclusions
STISPEC-194: The contractor shall use metric units to design the instrument and for developing interfaces with the spacecraft including any drawings, documents, models, except for the following cases:
• Heritage Component or unit: Components or units that has been previously qualified, or of similar design heritage, may be specified in English units where use of metric equivalents would lead to additional cost to the program.
• Fasteners: Although bolt patterns will be defined using metric dimensioning, use of English fasteners (with hole dimensioning and tolerancing) is permitted.
• Angular Measurement: Angular measurement may be expressed in degree of arc or in an appropriate subdivision of degree of arc such as second of arc (arc-sec) when advantageous to application.
5.2 Mass Properties Accuracy
5.2.1 Instrument Mass Accuracy
STISPEC-200: The mass of the instrument shall be measured to within ±0.1 kg.
5.2.2 Center of Mass Location
STISPEC-202: The contractor shall define the instrument center of mass in the MICD.
5.2.3 Center of Mass Accuracy
STISPEC-204: The instrument center of mass shall be determined to within ±5 mm relative to a reference that will be defined in the MICD.
5.2.4 Determination of Moments and Products of Inertia
STISPEC-206: The Contractor shall determine by analysis the launch and on-orbit moments and products of inertia to an accuracy of ±5.0 percent of the maximum principal moment of inertia, referenced to the coordinate axes with an origin at the center of gravity.
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5.3 Mounting
5.3.1 Surface Flatness
STISPEC-209: Mounting interface flatness, and co-planarity requirements for the instrument side of the interface (including brackets, if any, and shims) shall be as defined in the MICD.
5.3.2 Method
The method by which the instrument is mounted to the spacecraft will be defined in the Spacecraft to Instrument Interface Control Document (ICD).
5.4 Coordinate System and Alignment
STISPEC-213: The instrument shall use the spacecraft on-orbit coordinate system which uses a right-hand orthogonal, body-fixed XYZ coordinate system, Spacecraft Reference Frame (SRF), as follows: the +X-axis is aligned with the nominal direction of the spacecraft to Sun vector pointing towards the Sun, the +Y-axis nominal to normal of the ecliptic plane and pointing to celestial North, and the Z-axis is obtained from the right-hand rule. The roll, pitch and yaw rotations are defined about the X, Z, and Y axes, respectively. The origin of the coordinate system is at the center of the Launch Vehicle separation ring attachment plane. See Figure 5 Spacecraft Reference System.
Figure 5 Spacecraft Reference System
The Spacecraft will align the STIS to within 0.5 deg in each axis.
STISPEC-215: The instrument shall have clear fiducial marks to enable alignment during integration with spacecraft.
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The instrument unit mounting frame is an orthogonal reference frame defined by the locations of the spacecraft side of the instrument unit mounting points. A rigorous definition of this frame will be documented in the ICD.
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6 ENVIRONMENTAL REQUIREMENTS
Environmental design requirements for the instrument are specified in this section.
STISPEC-219: The instrument shall meet its performance requirements in section 4.0 after exposure to the environments specified in this section.
6.1 Mechanical Factors of Safety
STISPEC-221: The instrument flight hardware shall demonstrate positive Margins of Safety under limit loads for all yield and ultimate failures using the Factors of Safety (FS) defined in Table 2. Margin of Safety (MS) is defined as follows:
MS = (Allowable Stress (or Load) / (Applied Limit Stress (or Load) x FS)) -1
Table 2 Factors of Safety1,2
Type Static Sine Random/Acoustic 4,5 Metallic Yield 1.253 1.25 1.6 Metallic Ultimate 1.43 1.4 1.8 Stability Ultimate 1.4 1.4 1.8 Beryllium Yield 1.4 1.4 1.8 Beryllium Ultimate 1.6 1.6 2.0 Composite Ultimate 1.5 1.5 1.9 Bonded Inserts/Joints Ultimate 1.5 1.5 1.9
1 Factors of safety for pressurized systems to be compliant with AFSPCMAN 91-710 (Range Safety).
2 Factors of safety for glass and structural glass bonds specified in NASA-STD-5001 3 If qualified by analysis only, positive margin must be shown for factors of safety of
2.0 on yield and 2.6 on ultimate. See section 2.4.1.1.1 GSFC-STD-7000B 4 Factors shown should be applied to statistically derived peak response based on RMS level. As a minimum, the peak response shall be calculated as a 3-sigma value.
5 Factors shown assume that qualification/protoflight testing is performed at acceptance level plus 3dB. If difference between acceptance and qualification levels is less than 3dB, then above factors may be applied to qualification level minus 3dB instead of analyzing to acceptance level.
STISPEC-225: Primary and secondary structure comprised of composite materials, Beryllium, bonded joints and/or bonded inserts shall be proof tested to 1.25 x Limit Load; qualification by analysis only is not acceptable. Actual flight hardware testing is preferred, but testing of representative sets of hardware with a similar qualification argument can be used if approved by the NASA/GSFC COR.
6.2 Quasi-Static Acceleration
Quasi-static acceleration represents the combination of steady-state accelerations and the low frequency mechanically transmitted dynamic accelerations that occur during launch.
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STISPEC-228: The instrument shall be designed to withstand the quasi-static design limit loads defined in the mass-acceleration curve (MAC) shown in Table 3 without damage or degradation of performance and are to be applied one axis at a time. The design loads shown below will be updated based on the results of coupled loads analysis.
Linear interpolation should be used between breakpoints to determine the appropriate limit load as a function of instrument weight. Note that these design limit loads are intended to cover only the low frequency launch environment and must be used in conjunction with the random vibration environments to assess structural margins.
Table 3 Design Limit Loads
Mass (kg) Accel (g) 1 or less 51.3
5 42.4 10 36.6 20 30.3 40 24.2 60 20.9 80 18.7
100 or greater 18.1
6.3 Frequency Requirement
6.3.1 Fundamental Launch Frequencies
STISPEC-237: The instrument shall have a fundamental frequency greater than 100 Hz when hard mounted at its spacecraft interface. Any unit which fails to meet the specified fundamental frequency must supply a finite element model, correlated to modal survey test results or measured responses from vibration testing, so that it accurately represents the frequency and response amplitudes from the test. Requirements for the submitted finite element model are shown in the CDRL.
6.4 Vibration
6.4.1 Sinusoidal Vibration
STISPEC-240: The instrument shall undergo qualification, protoflight or acceptance (level depends on qualification status or qualification approach for the unit) sine vibration testing in all three axes at the levels shown in Figure 6. Instruments with a first mode greater than 150 Hz can be exempted from sine vibration testing upon approval by the NASA/GSFC COR. See Section
11.4.2 for definitions of Protoflight, Qualification, and Acceptance.
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Figure 6 Sine Vibration Environment
Levels may be notched to not exceed 1.25 times the design limit load outlined in section 6.2.
Peak levels at the low end of the frequency range (5 – 20 Hz typically) may be ramped up as needed to accommodate shaker table displacement limitations.
6.4.2 Random Vibration
STISPEC-245: The instrument shall demonstrate its ability to meet its performance requirements after being subjected to the random vibration environment in Figure 7 for units weighing 22.7 kg (50 lb.) or less, applied at the Spacecraft to instrument interface.
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Figure 7 Random Vibration Environment
The random environment will be updated by NASA once more information is available at the mission level. Note for lightweight STIS, the highest design loads may be from this random vibration environment.
STISPEC-249: The contractor shall provide random vibration analysis along with static loads analysis. Please see NASA-HDBK-7005 and NASA-STD-7001 for more information.
STISPEC-251: Notching shall be limited to -12 dB of the original input and to a bandwidth of less than 100 Hz to limit the random vibration responses to 3 dB above design limit levels.
Notching beyond these limits will require NASA/GSFC COR approval.
6.5 Shock
STISPEC-253: The instrument shall be designed to meet its performance requirements after being subjected to the shock environment shown in Table 4 and Figure 8, applied at the instrument interface to the L1 Series spacecraft structure. The shock environment envelopes all
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the Observatory shock events including separation from the launch vehicle and other actuations and will not exceed those shown in Table 4 and Figure 8.
Note: Figure 8 is the acceptance shock input at the L1 Series S/C to Launch Vehicle interface, not at the instrument to S/C interface. Further reduction between that interface and the instrument interfaces is expected due to joint and distance reductions.
The spacecraft will develop an attenuated shock environment for the instrument to spacecraft interface and document that environment in the spacecraft to instrument ICD.
STISPEC-255: A shock susceptibility and attenuation assessment (analysis) shall be performed for the instrument. If the flight shock environment as shown on a Shock Response Spectra (SRS) plot (Q=10) is enveloped by the curve shown in Figure 8, then the shock environment can be considered benign and there is low risk in deferring the shock test to the Observatory level.
STISPEC-897: Analysis supporting this conclusion (i.e., deferral of shock testing) shall be provided to the NASA/GSFC COR for review and deferral approval.
Any component within the instrument considered susceptible to the shock environment should have shock testing performed at the component level (preferably on a qualification unit).
STISPEC-2039: Instrument self-induced shock testing shall be accomplished by two actuations at the instrument level for each self-induced shock source (in order to account for the scatter associated with the actuation of the device) for the first flight unit, and a single actuation on subsequent units.
Table 4 Candidate LV Shock Environment
Candidate LV Separation Shock Design Envelope (P95/50 MPE)
Frequency [Hz] SRS [G-peak] 100 70 500 431.9
1000 1554 1550 2000
10000 2000
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Figure 8 Candidate LV Shock Environment
6.6 Acoustics
STISPEC-261: The instrument shall be designed to withstand, without any damage or degradation of performance, the protoflight acoustic noise…
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