fusion: bringing star power to earth farrokh najmabadi prof. of electrical engineering director of...
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Fusion: Bringing star power to earth
Farrokh NajmabadiProf. of Electrical EngineeringDirector of Center for Energy ResearchUC San Diego
NES Grand Challenges SummitRaleigh, North CarolinaMarch 4-5, 2010
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World uses (& needs) a lot of energy!
World Primary Energy consumption is 14 TW (2004) Equivalent to ~0.5 EJ or 11.2 Billion Ton of Oil Equivalent pa World energy [electricity] market ~ $4.5 trillion [$1.5 trillion] pa
World energy use is expected to grow 50% by 2030. Growth is necessary in developing countries to lift billions of
people out of poverty
80% of world energy is from burning fossil fuels
World Primary Energy consumption is 14 TW (2004) Equivalent to ~0.5 EJ or 11.2 Billion Ton of Oil Equivalent pa World energy [electricity] market ~ $4.5 trillion [$1.5 trillion] pa
World energy use is expected to grow 50% by 2030. Growth is necessary in developing countries to lift billions of
people out of poverty
80% of world energy is from burning fossil fuels
Conditions for Sustainability: Large supply of the energy resource (TW scale) Acceptable land/resource usage Minimal by-product stream Economically feasible technology
Conditions for Sustainability: Large supply of the energy resource (TW scale) Acceptable land/resource usage Minimal by-product stream Economically feasible technology
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Fusion Energy Requirements:
Confining the plasma so that alpha particles sustain fusion burn Lawson Criteria: nE ~ 1021 s/m3
Heating the plasma for fusion reactions to occur to 100 Million oC (routinely done in present experiments)
Optimizing plasma confinement device to minimize the cost Smaller devices Cheaper systems, e.g., lower-field magnets (MFE) or lower-
power lasers (IFE)
Extracting the fusion power and breeding tritium Developing power extraction technology that can operate in
fusion environment Co-existence of a hot plasma with material interface
Confining the plasma so that alpha particles sustain fusion burn Lawson Criteria: nE ~ 1021 s/m3
Heating the plasma for fusion reactions to occur to 100 Million oC (routinely done in present experiments)
Optimizing plasma confinement device to minimize the cost Smaller devices Cheaper systems, e.g., lower-field magnets (MFE) or lower-
power lasers (IFE)
Extracting the fusion power and breeding tritium Developing power extraction technology that can operate in
fusion environment Co-existence of a hot plasma with material interface
![Page 4: Fusion: Bringing star power to earth Farrokh Najmabadi Prof. of Electrical Engineering Director of Center for Energy Research UC San Diego NES Grand Challenges](https://reader035.vdocuments.site/reader035/viewer/2022062423/56649e7f5503460f94b8389e/html5/thumbnails/4.jpg)
Fusion Energy Requirements:
Confining the plasma so that alpha particles sustain fusion burn Lawson Criteria: nE ~ 1021 s/m3
Heating the plasma for fusion reactions to occur to 100 Million oC (routinely done in present experiments)
Optimizing plasma confinement device to minimize the cost Smaller devices Cheaper systems, e.g., lower-field magnets (MFE) or lower-
power lasers (IFE)
Extracting the fusion power and breeding tritium Developing power extraction technology that can operate in fusion
environment Co-existence of a hot plasma with material interface
Confining the plasma so that alpha particles sustain fusion burn Lawson Criteria: nE ~ 1021 s/m3
Heating the plasma for fusion reactions to occur to 100 Million oC (routinely done in present experiments)
Optimizing plasma confinement device to minimize the cost Smaller devices Cheaper systems, e.g., lower-field magnets (MFE) or lower-
power lasers (IFE)
Extracting the fusion power and breeding tritium Developing power extraction technology that can operate in fusion
environment Co-existence of a hot plasma with material interface
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We have made tremendous progress in optimizing fusion plasmas
Substantial improvement in plasma performance though optimization of plasma shape, profiles, and feedback.
Achieving plasma stability at high plasma pressure.
Achieving improved plasma confinement through suppression of plasma turbulence, the “transport barrier.”
Progress toward steady-state operation through minimization of power needed to maintain plasma current through profile control.
Controlling the boundary layer between plasma and vessel wall to avoid localized particle and heat loads.
Substantial improvement in plasma performance though optimization of plasma shape, profiles, and feedback.
Achieving plasma stability at high plasma pressure.
Achieving improved plasma confinement through suppression of plasma turbulence, the “transport barrier.”
Progress toward steady-state operation through minimization of power needed to maintain plasma current through profile control.
Controlling the boundary layer between plasma and vessel wall to avoid localized particle and heat loads.
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Fusion Energy Requirements:
Confining the plasma so that alpha particles sustain fusion burn Lawson Criteria: nE ~ 1021 s/m3
Heating the plasma for fusion reactions to occur to 100 Million oC (routinely done in present experiments)
Optimizing plasma confinement device to minimize the cost Smaller devices Cheaper systems, e.g., lower-field magnets (MFE) or lower-power
lasers (IFE)
Extracting the fusion power and breeding tritium Developing power extraction technology that can operate in
fusion environment Co-existence of a hot plasma with material interface
Confining the plasma so that alpha particles sustain fusion burn Lawson Criteria: nE ~ 1021 s/m3
Heating the plasma for fusion reactions to occur to 100 Million oC (routinely done in present experiments)
Optimizing plasma confinement device to minimize the cost Smaller devices Cheaper systems, e.g., lower-field magnets (MFE) or lower-power
lasers (IFE)
Extracting the fusion power and breeding tritium Developing power extraction technology that can operate in
fusion environment Co-existence of a hot plasma with material interface
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First wall and blanket System is subject to a harsh environment
Environment:
Surface heat flux (due to X-ray and ions)
First wall erosion by ions.
Radiation damage by neutrons (e.g. structural material)
Volumetric heating by neutrons in the blanket.
MHD effects
Functions:
Tritium breeding management
Maximize power recovery and coolant outlet temperature for maximum thermal efficiency
Constraints:
Simple manufacturing technique
Safety (low afterheat and activity)
Environment:
Surface heat flux (due to X-ray and ions)
First wall erosion by ions.
Radiation damage by neutrons (e.g. structural material)
Volumetric heating by neutrons in the blanket.
MHD effects
Functions:
Tritium breeding management
Maximize power recovery and coolant outlet temperature for maximum thermal efficiency
Constraints:
Simple manufacturing technique
Safety (low afterheat and activity)
Outboard blanket & first wall
x rayNeutronsions
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New structural material should be developed for fusion application
Fe-9Cr steels: builds upon 9Cr-1Mo industrial experience and materials database (9-12 Cr ODS steels are a higher temperature future option) SiC/SiC: High risk, high performance option (early in its development path) W alloys: High performance option for PFCs (early in its development path)
Fe-9Cr steels: builds upon 9Cr-1Mo industrial experience and materials database (9-12 Cr ODS steels are a higher temperature future option) SiC/SiC: High risk, high performance option (early in its development path) W alloys: High performance option for PFCs (early in its development path)
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Irradiation leads to a operating temperature window for material
Additional considerations such as He embrittlement and chemical compatibility may impose further restrictions on operating window
Additional considerations such as He embrittlement and chemical compatibility may impose further restrictions on operating window
Radiation embrittlement
Thermal creep
Zinkle and Ghoniem, Fusion Engr. Des. 49-50 (2000) 709
Carnot=1-Treject/Thigh
Structural Material Operating Temperature Windows: 10-50 dpa
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Several blanket Concepts have been developed
Simple, low pressure design with SiC structure and LiPb coolant and breeder.
Innovative design leads to high LiPb outlet temperature (~1,100oC) while keeping SiC structure temperature below 1,000oC leading to a high thermal efficiency of ~ 60%.
Simple, low pressure design with SiC structure and LiPb coolant and breeder.
Innovative design leads to high LiPb outlet temperature (~1,100oC) while keeping SiC structure temperature below 1,000oC leading to a high thermal efficiency of ~ 60%.
Dual coolant with a self-cooled PbLi zone, He-cooled RAFS structure and SiC insert
Dual coolant with a self-cooled PbLi zone, He-cooled RAFS structure and SiC insert
Flow configuration allows for a coolant outlet temperature to be higher than maximum structure temperature
Flow configuration allows for a coolant outlet temperature to be higher than maximum structure temperature
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How to meet the Fusion Challenge
National Will & Resources Public funding of energy research is down 50% since
1980 (in real term). World energy R&D expenditure is 0.25% of energy market of $4.5 trillion.
Stable Funding
Man Power: Training next generation of engineers
Focusing on Fusion Energy Mission Science-based Engineering
National Will & Resources Public funding of energy research is down 50% since
1980 (in real term). World energy R&D expenditure is 0.25% of energy market of $4.5 trillion.
Stable Funding
Man Power: Training next generation of engineers
Focusing on Fusion Energy Mission Science-based Engineering
We can do it!
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Thank You