Difference between pages "Radiometer" and "Hayabusa"

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=== Requirements ===
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Instructions for instruments operated during the Hayabusa-2 observation campaign.
  
* Sensitive to fireballs (mag -4) with a SNR of at least
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= Infrasound =
* Will provide calibrated brightness in apparent magnitude without observations from other sensors or absolute magnitude with trajectory data
 
* Bandwidth from DC to at least 1kHz, but ideally capable of more
 
* Low power (able to add to a DFNEXT observatory without changing power system)
 
* Less than $1000 per station
 
* Able to be used by a wide variety of users as standalone instruments and add-ons for fireball cameras
 
* Absolute timing precision that makes sense relative to the sample rate and no worse than the DFN observatories
 
  
=== Resulting Capabilities ===
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== [[RPi infrasound logger|Raspberry Pi (bare) logger]] ==
<Stuart please fill in>
 
  
=== Paper Plan ===
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== [[Blackbox infrasound logger|Blackbox logger]] ==
Authors: Robert, Stuart, Hadrien or Stuart, Robert, Hadrien
 
  
* Abstract
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== [[RS&BOOM|Raspberry Boom]] ==
* Introduction
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** Background
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** Objective
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** Motivation
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= Seismic =
** Approach
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* Prior Solutions
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== [[RS&BOOM|Raspberry Shake]] ==
** MORP
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** Prairie
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** Czech
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** Low cost
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= Optical (imaging) =
* Radiometer
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** Requirements
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** Concept Design
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** Design Evolution
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= Optical (spectroscopy) =
** Problems
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* Results
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** Sensitivity
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= EM =
** SNR
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** Spectrum
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* [[log-periodic antenna|log-periodic antenna]]
** Bandwidth
 
** Cost
 
** '''DATA'''
 
** Availability/open source?
 
* Conclusions
 
** Future Work
 
*** Multispectral
 
*** Cubesat
 

Revision as of 09:44, 3 November 2020

Instructions for instruments operated during the Hayabusa-2 observation campaign.

Infrasound

Raspberry Pi (bare) logger

Blackbox logger

Raspberry Boom

Seismic

Raspberry Shake

Optical (imaging)

Optical (spectroscopy)

EM