southwest research institute nsf conference on small satellites plasma instrument miniaturization...
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Plasma InstrumentMiniaturization and Integration:
Approaches and Limitations
C.J. Pollock, R. Torbert, and D.T. Young
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Plasma Instrument Miniaturization and Integration: Approaches and Limitations
- Functional Guidelines- Measurement Focus- Sensor vs Electronics- System Integration
-Examples of Low Resource Flight or Prototype Instruments- PEPE
- IES- TECHS- MOSS
-Limitations and Pitfalls:- It takes an aperture- It often takes high voltage
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Functional Guidelines
Measurement Focus• Disciplined approach that focuses narrowly on priority science• Sensor technologies for disparate plasma regimes:
• Langmuir Probe – Temperature and density of thermal plasma• Segmented Faraday Cup/RPA: High Mach # flowing plasma• Curved Plate ESA: Low mach number, structured plasma distributions
Sensor vs Electronics• In some cases there are limitations to sensor size reduction (aperture size dictates signal)
( X ~ A1A2/L2)
• Other times, the electronics may be irreducible (high voltage circuits)
System Integration vs Modularity(?)• A high degree of functional integration is helpful to minimize resource consumption and unintended functional redundancy;• Still, developmental modularity allows parallel development, often critical for small budget/short time scale flight development
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Particle Experiment for Planetary Exploration (PEPE) on Deep Space-I
• Developed as outgrowth of Dave Young’s Internal Research project at SwRI, entitled: Miniaturized, Optimized Smart Spectrometer (MOSS)
• Designed as a low resource, high performance electron and ion composition spectrometer
• Design principals include:• Innovative use of materials to reduce mass (ESAs are plated plastic)• Tight integration of electronics and sensor• Ions and electrons share entrance aperture
• ~5 kg, 5W dual spectrometer with LEF TOF measurement included
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Miniature -15kV Power Supply
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Flight Model – Ready for Cal
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Thermal Electron Capped Hemisphere Spectrometer(TECHS)
• Developed to target thermal electron fluxes in Earth’s ionosphere;
• Extreme miniaturization of tophat ESA necessary to measure low energy electrons in Earth’s ~0.4G field;
• Prime target electron energy from 0.1 to 100 eV
• Radius of curvature of ESA plates ~5mm.
• ESA Analyzer gap < 1 mm
• With analyzer ratio of ~7, application of 1kV ESA voltage would allow viewing of 7 keV electrons;
• Sensor the size of 35 mm film can;
• pre-amp boom and electronics box presently occupies more macroscopic scale.
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A Very Small & Very Black Inner Tophat Electrode
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TECHS Sensor Elements
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E-box and Boom Not So Small (room for improvement)
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Ion an Electron Sensor (IES) on Rosetta
• This was an exercise in extreme resourse conservation, patterned on the PEPE development.
• Dual, shared aperture ion and electron tophats with FOV deflection
• No time of flight (read: no ion composition)
• Tightly integrated but no modularity (difficult to troubleshoot and repair)
• Good performance obtained;
• Flight resource requirements: 1.25 kg; 1.8 Watts
• Severe compromises sometimes required. In IES, for example, to save power, the 1st HV step on the z-style MCP stack is 2.5 kV (for both electron and ion stacks), and the stacks are enabled and commanded in common;
• This is scary (perhaps less so for those with rocket background); It has worked well on orbit.
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IES Sensor Design
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Rosetta Ion and Electron Sensor Parameters.Parameter ValueEnergy
Range 1 eV/e to 30 keV/eResolution (DE/E) 0.04Scan Mode-dependent
AngleRange (FOV) 90 x 360º (2.8p sr)Resolution (e-) 5 x 22.5º (16 azimuthal x 16 polar)Resolution (ions) 5 x 45º (16 azimuthal x 7 polar)
Temporal resolution 3D distribution 3 sGeometric factor
Total (ions) 5 x 10-4 cm2-sr-eV/eV count/ionPer 45º sector (ions) 6 x 10-5 cm2 sr eV/eV count/ion
Total (e-) 5 x 10-4 cm2 sr eV/eV count/electronPer 22.5º sector (e-) 3 x 10-5 cm2 sr eV/eV count/electron
Mass 1040 gVolume 1297 cm3
DimensionsSensor: 73 mm dia x 101 mmElectronics box: 139 x 121 x 64 mm
Power 1850 mWDownlink data rate 5 - 250 bit s-1
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A MagCon System Concept
• Magnetometer, e and i+ plasma spectrometer, energetic particles
• A 3-instrument suite, integrated with a single central c&dh
• Instruments are sensors with bare bones co-located support circuitry;
• C&DH system that holds all possible command functions;
• C&DH system holds all possible signal processing functions;
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Micro-Satellite Architectural Diagram
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Final Draco Bench-Top Configuration
CDPU
Mag Sensor
Mag Electronics
IES Elec.
EPSElectronics
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Conclusions
• Significant miniaturization in capable plasma instrumentation is possible;
• Limitations exist, however:
• Aperture size sets limits on sensor miniaturization
• HV requirements set limits on certain electronics miniaturization
• Minimum resource plasma instruments and instrument suites can be focused on limited science goals
• Minimum resource/limited capability instrument suites can also be fielded for constellation-class payloads
• Continual investment in instrument & advanced technology development is a must!