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| − | === Requirements ===
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| − | * Sensitive to fireballs (mag -4) with a SNR of at least 10dB
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| − | * Will provide calibrated brightness in apparent magnitude without observations from other sensors or absolute magnitude with trajectory data
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| − | * Bandwidth from DC to at least 1kHz, but ideally capable of more
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| − | * Low power (able to add to a DFNEXT observatory without changing power system)
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| − | * Less than $1000 per station
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| − | * Able to be used by a wide variety of users as standalone instruments and add-ons for fireball cameras
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| − | * Absolute timing precision that makes sense relative to the sample rate and no worse than the DFN observatories
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| − | === Resulting Capabilities ===
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| − | <Stuart please fill in>
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| − | === Paper Plan ===
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| − | Authors: Robert, Stuart, Hadrien or Stuart, Robert, Hadrien
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| − | | |
| − | * Abstract
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| − | * Introduction
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| − | ** Background
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| − | ** Objective
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| − | ** Motivation
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| − | ** Approach
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| − | * Prior Solutions
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| − | ** MORP
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| − | ** Prairie
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| − | ** Czech
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| − | ** Low cost
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| − | * Radiometer
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| − | ** Requirements
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| − | ** Concept Design
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| − | ** Design Evolution
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| − | ** Problems
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| − | * Results
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| − | ** Sensitivity
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| − | ** SNR
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| − | ** Spectrum
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| − | ** Bandwidth
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| − | ** Cost
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| − | ** '''DATA'''
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| − | ** Availability/open source?
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| − | * Conclusions
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| − | ** Future Work
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| − | *** Multispectral
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| − | *** Cubesat
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