| Information from Subsystem | Subsystem | Information to Subsystem |
| Power requirements (actuators). | Structure | Mass. Maximum launch loads. PV array position req. |
| Power requirements by mission phase. | Thermal Control | Energy dissipation. Thermal limits. PV array position. |
| Power requirements by mission phase | Navigation, Guidance and Control | PV array pointing requirements |
| Power requirements by mission phase | Propulsion | |
| Power requirements by mission phase. Load scheduling | Command and Data Handling (Computers) | Load scheduling. Subsystem status |
| Power requirements by mission phase. Ground-control direct commands | Communication | |
| Power requirements | Oxygen Plant | |
| Power requirements by mission phase | Science Sensors | |
| Step | Reference (Wertz and Larson) | Examples |
| 1. Determine requirements and constraints for power subsystem solar array design. a. Avg. power required during daylight & eclipse b. Orbit altitude and eclipse duration c. Design lifetime. (Oversize the beginning of life (BOL) power to compensate for end of life (EOL) degradation; solar is poor for missions over 10 years.) | 10.1, 10.2 (Input parameter) Input parameter Input | 500 W during daylight & eclipse 800 km; 35.1 min. 10 years |
| 2. Calculate amount of power that must be produced by the solar arrays, Psa | Psa=((PeTe/Xe)+(PdTd/Xd))/Td Pe and Pd are the power requirements during eclipse and daylight. Xe and Xd are the efficiency of the paths from the arrays to the batteries and the loads (typically Xe = 0.6 and Xd = 0.8). Te and Td are the times in eclipse and daylight. | Pe = Pd = 500 W Te = 35.1 min Td = 65.9 min Xe = 0.6, Xd = 0.8 Psa = 1069 W |
| 3. Select type of solar cell and estimate power output with sun normal to surface of cells | Si: Po = 0.14*1358 W/m^2 = 190 W/m^2 GaAs: Po = 0.18*1358 = 244 (0.14 and 0.18 are the efficiencies for the cells; 1358 is the solar flux at Earth distance) | If we choose Si, Po = 190 If we choose GaAs, Po = 244 |
| 4. Find BOL and EOL power, per unit of array. If we configure the s/c well, its appendages will shadow few cells and shadowing losses will be slight. (Shadowing causes temp. variations and degrades the cells.) For Si cells, the ref temp is about 28C. Efficiency falls about 0.5% per degree above 28C. | Table 11-35 Eq. 5-6 PBOL = PoIdcos q | Id = degradation=0.77 q = sun incidence angle = 23.5 degrees PBOL = 134 |
| 5. Determine EOL power for the array. Radiation can cause a great amount of damage. Si cells protected by coverslides lose 15% of their voltage and current when exposed to 10^15 MeV for 4 to 5 years. | Degradation for Si = 3.75% per year, GaAs = 2.75% per year. Life degradation is given by Ld = (1-degrad/yr)^sat life PEOL = PBOLLd | For Si, Ld = 0.68 over 10 yr mission. For GaAs, Ld = 0.76 PEOL = 91.4 for Si PEOL = 102 for GaAs |
| 6. Estimate solar array size | Asa = Psa/PEOL | For Si, Asa = 11.7 m^2; for GaAs Asa = 10.5 m^2 |
| 7. Estimate mass | Mass = 0.04*Psa | Mass= 42.8 kg |
| 8. Iterate? | ||
| Mission phase | No. of cycles | Cycle Duration (min.) | Load (W) | DOD (%) |
| LEO | 144 | 36 | 146 | 21 |
| Transfer | 3 | 123 | 121 | 60 |
| Lunar | 370 | 75 | 226 | 65 |
The basic element is a 4x4 cm gallium-arsenide on germanium (GaAs/Ge) cell that is 5.5 mil thick, with a 3.5-mil coverglass. The cells were mounted on a graphite epoxy/aluminum honeycomb core substrate.
Array characteristics:
The arrays were steered so that they faced the Sun. The array Sun sensor was a pair of angled solar cells whose voltage was monitored.
Last Modified:
CSR/TSGC Team Web