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Flight Operations Segment Status
Swarm 7th Data Quality Workshop Ignacio Clérigo Delft, 27/10/2017
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Business as usual Flight Operation Status No, it was not a boring year Operational highlights since Edinburgh Exciting times ahead of us Future outlook
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4 years in 14 figures (Almost) four years in orbit
More than orbits 204 weekly reports 13 constellation maintenance manoeuvres and 5 collision avoidance telecommands uplinked 7.888 passes since commissioning 24.6 TB of TM parameters stored 189 manual activities since commissioning 294 procedures updated since launch 42 spacecraft database releases 57 spacecraft anomaly reports and 137 ground anomaly reports
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Platform status No changes since Edinburgh: all redundancies available
SW-A SW-B SW-C DMS CTU RU OK AOCS MTQ CGPS CESS FGM TT&C Thermal Power PCDU Battery EoC = V SA All SAR OK
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Payload status No changes since Edinburgh: all instruments working except ASM in Swarm C SW-A SW-B SW-C VFM OK ASM Failed (Nov 2014) EFI TII 3 orbits/day 1 orbit/day LP ACC STR GPSR
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Ground station status No changes since Edinburgh
Ground Station Network Kiruna: ESA station, 2 antennas + SSC commercial station, 3 antennas Svalbard: KSAT commercial station, 2 antennas Troll: KSAT commercial station, 1 antenna Only for contingencies, re-validation done in September 2017
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Ground station status Routine Contingencies
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Routine operations status
No changes since Edinburgh Pass allocation 2 passes per day per satellite, variable pattern Coverage: 10 hours manned by SPACON, SOE on-call for 16 hours Planning: weekly, uploaded on-board not earlier than Thursday Data return > 99.98% Only 1 gap above 5 minutes 18/01/2017, Swarm B: ~1.2 h housekeeping data (mass memory upset) Re-dumped all gaps > 5 minutes when data was available on-board 23 manual re-dumps performed since last DQW Most gaps caused by antenna pattern at 20 degrees elevation
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Routine operations status
From 15th October 2016 – 15th October 2017
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Business as usual Flight Operation Status No, it was not a boring year Operational highlights since Edinburgh Exciting times ahead of us Future outlook
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Flight Control Team Multiple team changes since last DQW Retired
Recovered New Swarm+Cryosat SOM Upgraded EarthCare SOE + Swarm On-call SOE Upgraded New payload SOE deployed New spacons Jonny Denise Cryosat/Earthcare AOCS migrated Shared with Cryosat Other teams supporting: FD, SDO, GS, SWS
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“Train for the worst, hope for the best”
Flight Control Team “Train for the worst, hope for the best” Training is key to deal with turn-over Large improvement of internal training procedures and material Review of safe mode procedures and dedicated trainings Complex and realistic contingency simulations: collision avoidance 2 days full scale exercise Complex scenario with 2 spacecraft threaten at the same time End-to-end simulation from manoeuvre preparation to execution ... and put as in the competition for best performance Oscar
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Manoeuvres 2 constellation manoeuvres since last DQW
3 high risk collision warning events since last DQW All three for Swarm-B 25/01/2017 Last minute NO GO Very large media coverage! Manoeuvre prepared and uplinked Cancelled, probability decreased (> 10e-6) 16/05/2017 CAM Chaser was an old friend: ERS-2 20g fuel, no slew required 24/07/2017 No need for CAM Chaser was a cubesat from Planet Risk quickly decreased Twitter 610k views Facebook 231k views ESA Rocket Science blog 5700 page view
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Anomalies No new genuine anomalies!
Only sporadic recurrence of already investigated anomalies 3 upsets of the on-board mass memory unit causing lost of data (~1h HK data) 2 autonomous STR reboots 35 ACC power-cycles 2 VFM upsets Frequent GPSR data lost events (seasonal, a few times per week) Result in TM packets wrongly time-stamped for 1s 1s gaps in science Cause of these events understood, work-around under discussion
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Anomalies 2 VFM upsets since last DQW
Single event upsets corrupt part of the VFM packets (same cause, different signatures) Both cases solved by power cycling the unit 29/04/2017, Swarm-A Science packets between 29th April 11:22 and 1st May 08:05 were lost Average field in HK TM used by PDGS to recover the gap 11/09/2017, Swarm-B Wrong time in science packets generated between 11/09 03:54 and 13/09 Actions taken to react faster to VFM upsets Agreement to power-cycle VFM as soon as problem is detected Procedures and on-call engineers training being improved …but FOS can react only if anomaly is detected (no hints in HK TM in few cases)
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Changes New TM packets to provide thermal parameter for STR thermal correction Preparations and validation of STR 2Hz operations EFI “extended commissioning” Covered in “EFI Operations” presentation EFI heating test by facing the Sun Swarm-B 7 days flying with non-nominal attitude Dawn/dusk orbit (LTAN~6am) Spring Equinox optimum conditions 16° yaw angle bias Achieved to increase EFI TII sensor temperature Average temperature ~15 °C …but far from ideal target (~50 °C) …and large fuel penalty (~400g in total)
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Mission planning New delivery of MPS software deployed in January 2017
Better interface with ESOC infrastructure for ground station planning Bug fixing and better consistency checks Partial simplification of planning rules and planning inputs More and more complex planning rules deployed Mainly linked to EFI operations (OPF interface with UoC) Automatic planning of EFI TII daily inner dome scrubbing activities Swarm-C test to set both EFI LP probes in high gain while EFI TII is in ready state Dynamic EFI HK TM packets rate to monitor voltage spikes during ramp-up Covered in “EFI Operations” presentation
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Business as usual Flight Operation Status No, it was not a boring year Operational highlights since Edinburgh Exciting times ahead of us Future outlook
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Spacecraft ageing analysis
Systematic analysis of all units and payloads in preparation for the mission extension Inputs from industry and payloads No technical constraint that could prevent the satellites from lasting one full solar cycle (and more!) could be identified Life limited items are not a concern Battery very small battery capacity fading until now (~5% since launch) Solar panel power consumption at lower end, large margin available Some risks beyond 2024 identified Availability of certain GPS signals
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Mission extension Impact of mission extension on FOS preliminary analysis completed Flight Dynamics: no problems foreseen Data Systems: major updates to address HW & SW obsolescence + additional storage Flight Control Team: no problems foreseen Ground stations: no problems foreseen ESOC infrastructure (computers, communications, ESTRACK…): no problems foreseen FOS is ready to support the mission extension and to cover at least one full solar cycle, as recommended by the Swarm science community
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Mission extension Mission Control System would require major updates to support operations in the future Hardware (both servers and clients) obsolescence Replacement of MySQL based archives Upgrade of the operating system Update of the Mission Control System Application Software (SCOS-2000) Deployment of new mission planning tool (if upgrade of existing one is not feasible) Additional data storage for telemetry-parameter and telemetry-packet archives required Long term performance of all data systems shall be taken into account Preparatory activities to identify most efficient approach have started
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Flight Dynamics acrobatics
Orbit evolution extensive work done by Flight Dynamics Covered in “Constellation Status of the Swarm Mission” presentation Flight Control Team is ready for manoeuvring campaigns Review of orbit manoeuvre procedures completed Team cross-training to support long demanding campaigns Additional resources only required for special cases Very close approach of the lower pair Very low altitude operations
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Flight Dynamics acrobatics
Several alternatives for close approach between A & C Very close approach (same plane) increases collision risk Special considerations in case of safe mode and CAM FOS response time reduced Additional monitoring passes Extended on-call support from FCT and FD More frequent manoeuvres to keep formation As close as possible weekly manoeuvres Requires low solar activity better now than later
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Conclusion FOS is ready for the extension! Thank you! Questions?
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