Integrating Lithium Polymer Charging and Peak Power Tracking on a CubeSat Class Satellite
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1 Integrating Lithium Polymer Charging and Peak Power Tracking on a CubeSat Class Satellite Dan Kaste, Dan Brinks, Jim Moore, Hugh White Zach Palmer and Will Holmes
2 Presentation Overview Students Involved Mission Summary Design for Assembly Mesh Network Science Instruments Power System Design Principles Summary / Conclusion
3 Dan Kaste Hugh White Dan Brinks Jared Sutter Jim Moore Zach Palmer Students Involved
4 Mission Objectives Demonstrate a functional wireless mesh network in orbit Take concurrent multipoint measurements of space plasma density Detect Very Low Frequency (VLF) Whistler Waves with spatial and temporal resolution. Langmuir Plasma probe and VLF must be able to interface into Boston University s BUSAT Satellite must Demonstrate a high level of modularity, allowing subsystems to be reused on future missions and on BUSAT
5 Satellite System
6 Mission Objectives Demonstrate a functional wireless mesh network in orbit Take concurrent multipoint measurements of space plasma density Detect Very Low Frequency (VLF) Whistler Waves with spatial and temporal resolution. Langmuir Plasma probe and VLF must be able to interface into Boston University s BUSAT Satellite must Demonstrate a high level of modularity, allowing subsystems to be reused on future missions and on BUSAT
7 Demonstrate a Mesh Network (Zigbee or ) Parent Node Node A Node B Node C Node D Node E
8 Demonstrate a Mesh Network (Zigbee or ) Parent Node Node A Node B Node C Node D Node E
9 Demonstrate a Mesh Network (Zigbee or ) Parent Node Node A Node C Node B Node E Ground Station Node Node D
10 Demonstrate a Mesh Network (Zigbee or ) Parent Node Node A Node C Node B Node E Ground Station Node Node D
11 Mission Objectives Demonstrate a functional wireless mesh network in orbit Take concurrent multipoint measurements of space plasma density Detect Very Low Frequency (VLF) Whistler Waves with spatial and temporal resolution. Langmuir Plasma probe and VLF must be able to interface into Boston University s BUSAT Satellite must Demonstrate a high level of modularity, allowing subsystems to be reused on future missions and on BUSAT
12 Mission Objectives Demonstrate a functional wireless mesh network in orbit Take concurrent multipoint measurements of space plasma density Detect Very Low Frequency (VLF) Whistler Waves with spatial and temporal resolution. Langmuir Plasma probe and VLF must be able to interface into Boston University s BUSAT Satellite must Demonstrate a high level of modularity, allowing subsystems to be reused on future missions and on BUSAT
13 Langmuir Plasma Probe Purpose: Measure low energy, thermal electrons (0 to 6 ev) (L1-2) Returns both Density and Energy (Temperature)
14 Detect Whistler Waves. VLF Receiver Image from Stanford website
15 Presentation Overview Students Involved Mission Summary Design for Assembly Mesh Network Science Instruments Power System Design Principles Summary / Conclusion
16 Power System Requirements Maintain Downlink Capability Available power always above 2 watt hours Charge batteries correctly Maximize Power Flow into Satellite Figure from Panasonic
17 Power System Requirements Maintain Downlink Capability Available power always above 2 watt hours Charge batteries correctly Maximize Power Flow into Satellite Distribute Power to Satellite Have an efficiency greater than 80%
18 Power System Microcontroller (MSP430) Solar Cells Digital Potentiometer Linear Regulator Battery
19 Power System
20 Status Implementation of Peek Power Tracking / Li Battery Charging not Complete First Iteration of Circuit Board Complete Software awaiting Hardware Look for Testing Results at Booth at Next Year s Conference Satellite Subsystems Developed VLF, Plasma, Communications (Mesh Network), System
21 Lessons Learned / Summary Pay Attention to Assembly and Systems Engineering from the beginning of a Project. Make sure that Complexity does not increase. While satellite not delivered, six students were trained.
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