feasibility of nano-satellites constellations for ais...
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Feasibility of Nano-Satellites Constellations for AIS
Decoding and Fire detection J. Castelvi, E. Lancheros, A. Camps, and H. Park.
Departament de Teoria del Senyal i Comunicacions,
Universitat Politècnica de Catalunya-BarcelonaTech, Barcelona, Spain.
{jordi.castellvi, estefany, camps, park.hyuck}@tsc.upc.edu
Outline 1. Gap requirements for Fire detection
• Global look on State of the art. • Requirements.
2. Why Automatic Identification System (AIS) decoding? • Advantages and disadvantages. • Operational and future AIS decoding on CubeSat • Requirements.
3. 3CAT-3 initiative • Threshold Performance Requirements for fire detection
and AIS • Technical data • Sample analysis • Data Budget Simulation
4. Constellation configuration • Coverage and revisit time
5. Conclusions
Feasibility of Nano-Satellites Constellations for AIS Decoding and Fire detection 2
1. Gap for Fire Detection
LEO-MISSIONS • Moderate-resolution: 300 – 1000 m Global coverage: twice/day – 2 days • High-resolution 8 – 60 m Global coverage: 5 – 90 days
GEO-MISSIONS • Moderate-resolution: 1000 m Full disk each 10 -15 min
User requirements by OSCAR: Nowcasting: at 1 km of spatial resolution; revisit time of 15 min, and global land coverage each 15 min Agricultural meteorology: at 10 m spatial resolution; revisit time of 60 min, and global land of 6 hours.
Main missions time-line that can be used for fire detection
Feasibility of Nano-Satellites Constellations for AIS Decoding and Fire detection
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Why AIS Decoding?
Feasibility of Nano-Satellites Constellations for AIS Decoding and Fire detection
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Source: Review of Maritime Transport 2015. United Nations Conference on Trade and Development (UNCTAD)
Adoption of international AIS as global
regulation for maritime traffic control.
Growth of global demand for container
shipping reached 6 %.
Global container demand boosted in the Far
East–Europe and the trans-Pacific.
Monitoring on continental remote navigation
(coastal areas are covered by the AIS
terrestrial stations)
To improve the security and surveillance
services.
More than 70,000 ships worldwide have
installed AIS system.
Why AIS Decoding?
Several universities are developing AIS
receivers (e.g. UPC AIS uses a SDR for
upcoming nanosat mission).
Advantages Disadvantages
• Accurate information
(position, course, speed).
• Is a normative (IMO) - Required on
board all passenger ships regardless
of size.
• Global Coverage.
• Possible implementation on nano-
satellites. (Low cost, low size, low
power, low weight).
• Huge number of AIS messages
simultaneously received from satellite
antenna footprint, easily exceeds
maximum TDMA time-slots.
• Required on board of ships with gross
tonnage of 300 or more.
Security services: revisit time of 1 hr.
Management services for commercial user: revisit time of 3 hr.
User requirements over remote areas of the ocean :
Feasibility of Nano-Satellites Constellations for AIS Decoding and Fire detection
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Operational and future AIS decoding on Cubesats
Feasibility of Nano-Satellites Constellations for AIS Decoding and Fire detection
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3CAT-3 ZACube-2
AAUSAT-4 AISSat 2 AISAT
AAUSAT-3 AISSat 1 CanX-6 (NTS)
Operator or
contractor
Universidad
Politécnica
de Cataluña
Cape
Peninsula
University of
Technology
Aalborg
University
Cubesat
UTIAS DLR Aalborg
University
Cubesat
UTIAS
UTIAS
Satellite Mass (kg)
9 4 0,88 6 14 0,8 6 6.5
Size 6U 3U 1U -
1 U 1 U - 2 U
Power Consumption
- - 1.15 W 0.97 W 15 W 1.15 W 0.97 W 5.6 W
Launch date - 2017 2016 2014 2014 2013 2010 2008
Payload AIS + high resolution VIS and VNIR camera
AIS + Low resolution NIR imager
AIS AIS AIS AIS AIS AIS
Item Description
CMOS optical sensor Spatial Resolution 10 - 30 m. VIS and VNIR ; Swath: 18 km; bands: 475, 555, 650,710, 870 nm-
AIS system:
162 MHz ± 25 KHz, Power consumption: < 800 mW. Mass: 55 g, volume: 94.7x89.0x6.7 mm
Alternate: SDR-based UPC instrument (under development)
2 Electrical Power System (EPS)
Mass: 200 g; volume: 96x90x16 mm. Batteries providing up to 6-8 W (2 sets)
Batteries Mass: 240 g; volume: 94x88x23 mm Battery heater; heater power: 3.5 to 7 W
Solar Panels 1U 14 solar panels (1U), GaAs, 0.1 A/m2
28.3 % efficiency
On Board Computer (OBC) 400 MHz, 32 MB RAM Mass: 94 g; volumen: 96x90x12.4 mm Power consumption: 400 mW.
S-band transceiver Data rate: 2Mbps Mass: 95 g; volumen: 96x90.2x17 mm. Power consumption < 6 W
UHF-transceiver card for T&T
Data rate: 115 Kbps Mass: 24.5 g; volumen: 65x40x6.5 mm. Power consumption: 0.2 W (receptor mode)
Attitude Determination and Control System (ADCS)
Mass: 865 g; volumen: 100x100x79 mm. Power Consumption: 1.5 W to 4.5 W Pointing accuracy 1°
3Cat-3 mission (6U): technical data
Feasibility of Nano-Satellites Constellations for AIS Decoding and Fire detection
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P/L: MS optical imager, reconfig. SDR RF
receiver (AIS + GNSS-R)
Main application: vegetation/agriculture
Secondary application: fire monitoring
and AIS
6U nano-satellite cost-effective
demonstrator
Threshold Performance Requirements for fire detection and AIS.
Feasibility of Nano-Satellites Constellations for AIS Decoding and Fire detection
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Minimum Acceptable Desired
Spatial resolution for fire detection
1000 m 300 m 10 m
Revisit time for fire detection
6 hours 3 hours 1 hour
Revisit time for AIS decoding
3 hours 2 hours 1 hour
Coverage for fire detection
Contiental EU each 18 hr
EU and Amazon each 12 hr
Gobal land each 6 hrs
Coverage for AIS decoding
Remote areas of Atlantic North ocean
Remote areas of Atlantic North ocean and Pacific North ocean
All remote areas of the oceans
Satellite mass 20 – 30 kg 10 – 20 kg > 10 kg
Feasibility of Nano-Satellites Constellations for AIS Decoding and Fire detection
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Target areas for fire detection Target area for AIS event Ground station
Sample Analysis: Ground Stations and Target Areas
Data Budget for a 24 hours simulation:
Feasibility of Nano-Satellites Constellations for AIS Decoding and Fire detection
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Inclined orbit : 55°
Altitude: 600 km
Orbit: circular
2 ground stations. S‐band transmitter ON if visibility with ground station and power budget permitting 2GB SD memory card. AIS active over target areas, imager active over target areas.
Image compression FAPEC
Constellation
Feasibility of Nano-Satellites Constellations for AIS Decoding and Fire detection
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Scenario 1 Scenario 2 Scenario 3
Inclined orbit : 98° 55° 55°
Altitude: 600 km 600 km 600 km
Orbit: Circular Circular Circular
# of satellites: 24 24 50
Orbital planes: 4 4 5
Swath: 18 km Spatial resolution: 10 m
Swath: 50 km Spatial resolution: 30 m
OPTICAL SENSOR
Constellation: Coverage and revisit time
MS Optical Instrument
Feasibility of Nano-Satellites Constellations for AIS Decoding and Fire detection
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Scenario 1
• Inclined orbit : 98°
• # of satellites: 24
• Orbital planes: 4
Swath: 18 km Swath: 50 km
Constellation: Coverage and revisit time
MS Optical Instrument:
Feasibility of Nano-Satellites Constellations for AIS Decoding and Fire detection
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Scenario 2
• Inclined orbit : 55°
• # of satellites: 24
• Orbital planes: 4
Swath: 18 km Swath: 50 km
Constellation: Coverage and revisit time
MS Optical Instrument
Feasibility of Nano-Satellites Constellations for AIS Decoding and Fire detection
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Scenario 3
• Inclined orbit : 55°
• # of satellites: 50
• Orbital planes: 5
Swath: 18 km Swath: 50 km
Constellation: Coverage AIS Decoding
Scenario 1
• Inclined orbit : 98°
• Altitude: 600 km
• Orbit: circular
• # of satellites: 24
• Orbital planes: 4
Feasibility of Nano-Satellites Constellations for AIS Decoding and Fire detection
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Scenario 2
• Inclined orbit : 55°
• Altitude: 600 km
• Orbit: circular
• # of satellites: 24
• Orbital planes: 4
Scenario 3
• Inclined orbit : 55°
• Altitude: 600 km
• Orbit: circular
• # of satellites: 50
• Orbital planes: 5
Conclusion
• A constellation /federation of nanosats can be an excellent candidate low-cost mission to improve the spatial and temporal resolution for fire and AIS measurements to complement the Copernicus system in the mid term.
• Next step: orbit optimization
Detailed power, memory, data Links budgets and thermal analysis
Feasibility of Nano-Satellites Constellations for AIS Decoding and Fire detection
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