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Lecture 7: Power Systems and Thermal Management

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1 Lecture 7: Power Systems and Thermal Management

2 Power System Structure and Requirements
Electrical Power Subsystem Energy Storage Power Source Power Distribution Regulation & Control Typical Requirements Supply continuous electrical power to s/c loads during mission Control and distribute electrical power Handle average and peak electrical load Provide ac, dc power converters Protect against failures in the EPS Suppress transient voltages and protect against faults

3 Power System Design Process
Step Info. Required Derived Requirements 1. Identify requirements Top-level requirements, s/c configuration, mission life, payload definition Design requirements, average and peak power 2. Select power source S/c configuration, average load requirements EOL power required, type of solar cell, mass and area of solar array, solar array configuration 3. Select energy storage Orbital parameters, average and peak load Battery capacity required, battery mass, volume and type 4 Identify power regulation and control Power source selection, mission life, regulation and thermal control requirements Peak power tracker or direct energy-transfer system, thermal control requirements, bus-voltage quality, power control algorithms

4 Power Sources Power sources
Photovoltaic Static Dynamic Planar Concentrators Thermionics Thermoelectrics Brayton Stirling Rankine Photovoltaic solar cells convert incident solar radiation directly to electrical energy Static power sources uses a heat source, typically plutonium or uranium-235 for direct thermal-to-electrical conversion Dynamic sources also use a heat source – concentrated solar, plutonium-238, or enriched uranium – to produce power via Brayton, Stirling or Rankine cycles

5 Comparison of Power Sources
Design Parameters Solar Photovoltaic Solar Thermal Dynamic Radio- isotope Nuclear Reactor Power range (kW) Specific power (W/kg) 9 - 15 8 - 10 Specific cost ($/W) 16K – 18K Hardness to natural radiation Medium High Very high Stability and maneuverability Low Degradation over life Storage required for eclipse? Yes No Sun angle sensitivity None Sensitivity to shadowing Low (with bypass diodes) Fuel availability Unlimited Very low

6 Solar Array Design Process
Determine requirements and constraints Av. Power needed during daylight and eclipse Eclipse durations Design lifetime Calculate power that must be produced, Psa

7 Solar Array Design Process
3. Select type of solar cell and estimate power output, P0 , with the sun normal to the surface of the cells 4. Determine BOL power production per unit area, taking account of inherent degradation: And the cosine loss and life degradation: Elements of inherent degradation Nominal Range Design and assembly 0.85 Temperature of array Shadowing of cells 1.00 Inherent degradation, Id 0.77

8 Secondary Battery Couple Specific Energy Density
Energy Storage Primary batteries have higher specific energy densities but cannot be recharged. Thus, they typically apply to short missions. Characteristics of some secondary batteries: Secondary Battery Couple Specific Energy Density (W-Hr/Kg) Status Nickel-Cadmium 25-30 Space-qualified, extensive database Nickel-Hydrogen (individual pressure vessel) 35-43 Space-qualified. Good database (common pressure vessel) 40-56 Space qualified for GEO and planetary (single pressure vessel) 43-57 Space-qualified Lithium-Ion 70-110 Sodium-Sulfur Under development

9 Energy Storage

10 Black Body Radiation Model
A sea of photons is surrounded on all sides by high temperature atoms. These particles randomly absorb or emit photons, permitting all possible energy transitions compatible with conservation of overall energy

11 Black Body Radiation Model

12 Black Body Radiation Model
UV & Vis Infrared Microwave Wien’s law

13 COBE (Cosmic Background Explorer) satellite data precisely verifies Planck’s radiation law

14 Black Body Radiation Model

15 Thermal Equilibrium of an Isolated Body in Space
Electronics

16 Spherical Spacecraft Equations

17 Spherical Spacecraft Equations

18 Putting the Equations to Work: The Preliminary Design Process
Step Notes 1. Determine requirements and constraints Identify temperature limits – see Table 11 43, L&W Estimate electrical power dissipation 2. Find the diameter of a sphere with the same surface area as the spacecraft Make first-order estimates assuming an isothermal, spherical spacecraft (using the above equations). 3. Select radiation surface property values Initially assume white paint with S=0.6 and IR=0.8 4. Compute worst-case hot and cold temp.s for the spacecraft Upper limit: Use high-side values of all power input terms Lower limit: Include only the IR emissions. 5. Compare worst-case hot and cold temp.s with temp. limits found in step 1. If worst-case hot temperature is > required upper limit, use a deployed radiator with a pumped-looped system. Otherwise, use body-mounted radiators 6. Estimate required area for body-mounted radiator. Use upper temp. limit for radiator temp., assume no heat inputs and max. heat dissipation – see equation 11.23, L&W 7. Estimate radiator temp. for worst-case cold conditions Use the area from step 6 and min. heat dissipation

19 The Preliminary Design Process - Continued
Step Notes 8. If temp. in step 7 is less than the lower limit, determine heater power required to maintain radiator at lower temp. limit Assume radiator temp. is at the lower limit 9. Determine if there are special thermal control problems Identify components with narrow temp. ranges, high power dissipation or low temp. requirements. See thermal control options in section , L&W. 10. Estimate subsystem weight, cost and power. I f no special problems, use 4.5% of spacecraft dry weight, 4% of the total spacecraft cost, and heater power from step 8.

20 Thermal Control Devices and Strategies - If special thermal control problems are encountered in step 9 Materials and Coatings Optical Solar reflectors Silver-Coated Teflon MultiLayer Insulation Electrical Heaters Thermostats Space radiators Cold-Plates Doublers Phase Change Devices Heat Pipes Louvers Temp. Sensors Adhesive Tapes Fillers Thermal isolators Thermoelectric Coolers Cryogenic Systems Active Refrigeration Systems Expendable Cooling Systems

21 Thermal Control Devices and Strategies
Materials and Coatings: paints, silverized plastics, special coatings – all with special absorptivity & emissivity values– See Table 11-44 Optical Solar Reflectors (OSRs): Highly reflective surface mounted on a substrate and overlaid with a transparent coating. Reflects most incoming radiation back to space, IR emissivity = 0.8, solar absorptivity = 0.15 Expensive and fragile. Silver-Coated Teflon - Cheaper alternative to OSRs. MultiLayer Insulation (MLI): The primary spacecraft insulation device. Alternate layers of aluminized Mylar or Kapton, separated by net material, e.g. nylon, Dacron or Nomex See Fig for the effective emmitance of MLI Electrical Heaters Used in cold-biased systems to bring selected components up to proper temp. Thin electrical resister between two Kapton sheets Typical power densities  1 W/cm2 Thermostats Switches to turn heaters on/off Typical operating range: -50 to 1600C

22 Thermal Control Devices and Strategies
Space radiators Heat exchanger on the outer surface of the spacecraft that radiates waste heat Can be structural panels or flate plates mounted on the spacecraft Cold-Plates Heat dissipated by electrical equipment is conducted across the interface to the cold plate. Fluid circulating through the cold plate Carries the heat to a space radiator. Heat Pipes Lightweight devices used to transfer heat from one location to another, e.g. from an electrical component to a space radiator Temp. Sensors Thermisters: Semiconductor materials that vary their resistance with temperature. They operate around -50 to C. Resistance Thermisters: Uses a pure platinum conductor. Very accurate and expensive Heat in - evaporation Wicking material Gas Heat out - condensation Liquid flow via wick


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