Small Satellites: The Execution and Launch of a GPS Radio Occultation Instrument in a 6U Nanosatellite

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Small Satellites: The Execution and Launch of a GPS Radio Occultation Instrument in a 6U Nanosatellite Dave Williamson Director, Strategic Programs Tyvak

Tyvak: Satellite Solutions for Multiple Organizations Wide Variety of Customers Commercial Civil Defense Facts and Figures Tyvak Nanosatellite Systems founded in 2011 Holding company Terran Orbital Corp. founded in 2014 Tyvak International founded in 2015 Fully independent European establishment 3 locations, > 60 employees Irvine, CA San Luis Obispo, CA Torino, Italy 2

Complexity & Size Nanosatellite evolution Nanosatellites have evolved to powerful instruments for advanced operational capabilities and high mission utility Operational : fulfil critical official government or commercial missions Substantial mission life (> 3years) High utility: high level of performance, reliability and confidence in mission success Precise attitude control, formation flying, station keeping Proximity operations, orbit boost/control, disposal manoeuvres Multiple Applications GPS Radio Occultation Advanced Optics Demonstrations Atmospheric Science RF Signal processing Technology Demonstrations 2013 2014 2015 2016 2017 2018 Time (and company growth) 3

Background Tyvak is developing the GeoOptics, Inc. CICERO constellation of satellites. Completed first three satellites in the constellation Intended to gather vital data on the Earth s weather, climate and environment. Program utilizes Tyvak s Endeavour small satellite platform 6U CubeSat, high-speed communications, 3-axis high performance attitude control The CICERO Constellation will test and demonstrate the newly developed instrument and the integrated satellites Data gathered will provide: Weather monitoring and forecasting information to the National Oceanic and Atmospheric Administration (NOAA) Science and Weather Data to Other government and commercial customers. In the past, larger satellites have executed these missions. Small satellite missions can collect more distributed data with faster revisit times around Earth. The GPS Radio Occultation instrument development emphasized building an instrument of equal quality to previous instruments. 4

CICERO Radio Occultation Constellation Mission Demonstration and operational constellation of radio occultation observation satellites for a Commercial Customer Data Products to be delivered to Customer as part of commercial data buy for near real-time weather data Phased 2 x 3 patch array for GPS L1 and L2 Launch First 4 units to be launched May and June 2017 3 more spacecraft to be launched in Q4 2017 Technologies Developed and Demonstrated Scientific RO instrumentation made in collaboration with JPL Very low EMI spacecraft, extensive RF shielding Program Challenges & Experiences Low EMI requirement GPS Antenna and RO Payload Development 5

Design Goals Achieved and General Capabilities Near 100% duty Cycle: Fixed deployable solar arrays to allow nearly 100% duty cycle operation of the CION instrument Data capacity 2Mbps X-Band transmitter can Download all RO data collected in 1 Orbit along with associated back-orbit telemetry Compatibility with KSAT Network for fast data delivery Algorithms to target RO Opportunities Calculated on the ground and then event scripts for vehicle slews for optimal RO opportunities are executed Will be automated on the vehicle using the onboard propagator in future batches GPS RO Instrument Improvements Updated software to support GLONASS Software upload and re-flash capabilities Parameter Size Mass Power ADCS Battery Average Solar Array ~21 W Cion 6U CubeSat ~10kg 21 W Orbit avg. Full 3 axis stabilized, 2 Star Trackers, 3 reaction wheels 120 W-hrs Comms X-band down (Payload) UHF up/down (S/C housekeeping) 6

Cion - CICERO Instrument for GPS-RO Key Challenges & Experiences Miniaturize the instrument from a power and mass perspective but ensure end data product quality and support essential JPL heritage software compatibility. The quality and effectiveness of collaboration is far superior when the collaborators are within driving distance. JPL has been on-sight for system test verifications, and design reviews. Cion Instrument Features: RF Inputs: 3 antenna inputs with 4 down converters each Processor: 1.2 GHz Dual Core Arm processor RAM: 1GB Flash: up to 256GB DSP: Programmable FPGA for Digital Signal Processing Sub-channels: 16 GPS (8 dual freq satellites) External Clock: High performance Osc (10MHz, ~5X10-12) Ext PPS output and Ext event input Accommodations: Volume: 3U available 30cm X 10cm X 6cm utilized by final payload configuration Mass: 1.2kg Power: ~8 watts at 12 VDC Comm Interfaces Available : Two RS 422, USB and Ethernet 7

Space ory! echnology! Evolution of a Payload Cion End Result! TriG!Vs!Cion! TriG! Cion! Significant reduction in Size, Weight, and Power Parameter TriG Cion Size 11 x 19 x 22 cm 30 x 10 x 6 cm Mass ~6 kg 1.2 kg Power ~65 Watts 8 Watts Antenna incorporates combiner into the phased array Eliminated need for external RF Combiner Eliminates need for complex coax harnessing and associated mass EMI/EMC Bus design has a RF gasket enclosure to prevent EMI Payload resides in its own separate volume within the 6U CubeSat External Inputs Temperature controlled highly stable Crystal Oscillator for precise data clocking and timing External GPS for Position, Orbit Determination Collection Rate 1kHz, 100Hz, or 50Hz native data collection rate from all channels 8

t sep+0 minutes Ppod sep +0 minutes Ppod sep +1 minutes Ppod sep +30 minutes tppod sep +First Contact Ppod sep +1-2 days] Launch and Early Operations (LEOPS) Remotes Tracking Station Injection Orbit (e.g., 600 km) 2.1 Power on Deploy Panels UHF Antennas Initial SOH 4a Verify Comm Launch Rideshare using 6U dispenser Power on Initialize Only core avionics will turn on Deployables released ADCS turn on and auto transition to sun pointing Initial SOH 2.0 GPS seeded Propagator used to initiate SOH over UHF stations SOH on demand if GPS not available Verify Comm t 0+ Checkout uplink/downlink using UHF, downlink using X-Band 9

Summary of CICERO Mission Phases Initial SOH Checkout 4 Energy Collection and RO Target Selection 5a RO Target slew and RO collection 5b Slew to X Band GS and downlink Science Data 5c Modify RO configuration to repeat PHASE 5 Release from 6U dispenser 3 CMD/TLM CMD/TLM TLM CMD/TLM CMD/TLM 6 TLM Disposal 7 2 Launch Ground Network Main CICERO Mission Phases Mission-Planning / Pre-Launch 1 Mission Operations Center 10

Mission Operations Overview LEGEND GPS/GNSS CICERO LEO ORBIT ATMOSPHERE GPS SIGNAL 1 2 3 1. Nominal RO Collection CICERO- OP1 collects RO while slewing for Sun-Pointing 2. X-Band Data Downlink Every orbit CICERO has at least 1 pass with X- Band station for downlink 3. Target RO Collection CICERO- OP1 slews to target RO collection 4. UHF Uplink Uplink any specific RO targets or modify collection angle Collection Flexibility Spacecraft will slew for optimal RO coverage and also to track certain events prioritized by operators 4 High Degree of Automation Each spacecraft has the ability to operate more than a weeks worth of automated collection and data downlink events 11

Mission Operations Mission Operation Center (Tyvak, Irvine) Main UHF system on-site Additional UHF station is available K-SAT site in Tromso UHF only All data from all sites comes directly to Tyvak once downlinked Kongsberg Satellite Services (K-Sat) Additional Downlink Stations available for X-Band Irvine Internal Network GeoOptics/Customer Data Delivery VPN Tyvak UHF Ground Segment Tyvak Irvine Mission Operations Server Vehicle Operator Vehicle Operator Nominal Operations are mostly autonomous for the routine RO collection and Data Downlink. Fault Flag notify operators of any off nominal cases and put the spacecraft into Safe Mode. Vehicle Director Tyvak Mission Operations Center (MOC) Commercial Ground Station Partners KSAT 12

Timeline Final Testing Q1 2017 Launch Q2 2017 Operations Q3 2017 and beyond 1 on PSLV (500km SSO) 2 on Soyouz (600km SSO) Sustained data delivery to customers First 3 Satellites Second Batch of 3 Additional satellites for the constellation planned Launch Q4 2017 Operations Q4 2017 and beyond 1 on PSLV (500km SSO) 2 on Soyouz (600km SSO) Batches can be built rapidly in order to be available for opening launch opportunities 13

Final Configuration Phased 2 x 3 patch array for GPS L1 and L2 UHF Antenna POD GPS Antenna Umbilical and Test ports Mag and Sun Sensor Module Star Trackers 14

Thank You! Questions? Come see us at our Booth! Special Thanks to our partners GeoOptics Dave Williamson Director, Strategic Programs dave.williamson@tyvak.com 15