Results of research on a single-component system for a liquid-metal MHD converter
Single component closed loop, liquid potassium magnetohydrodynamic generator
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Single component closed loop, liquid potassium magnetohydrodynamic generator
Electrical conductivity of two phase liquid metal flow in magnetohydrodynamic generator
Injector characteristics using wet steam in connection with magnetohydrodynamic generator applications
Experimental results on two phase supersonic nozzle used in liquid metal magnetohydrodynamic generators
Development of combined turbine-magnetohydrodynamic generator operating in Brayton cycle with NERVA nuclear reactor for space and ground applications
The matrix method of calculating linear induction machine performance as a function of winding current distribution was extended to determine the winding current distribution for maximum efficiency. Application of the method to typical magnetohydrodynamic generator geometries showed that electrical efficiencies of 0.5 to 0.6 are possible with fractional wavelength windings and without insulating vanes in the flow.
An atomic iodine laser, a candidate for the direct solar pumped lasers, was successfully excited with a 4 kW beam from a xenon arc solar simulator, thus proving the feasibility of the concept. The experimental set up and the laser output as functions of operating conditions are presented. The preliminary results of the iodine laser amplifier pumped with the HCP array to which a Q switch for giant pulse production was coupled are included. Two invention disclosures - a laser driven magnetohydrodynamic generator for conversion of laser energy to electricity and solar pumped gas lasers - are also included.
Vortex magnetohydrodynamic power generator
Transverse current MHD conduction generators for AC power generation
Vortex magnetohydrodynamic power generator, alkali metal carbonates to seed combustion plasmas
Influence of compressibility on conduction type magnetohydrodynamic ac generators
Operation of large inert gas magnetohydrodynamic power generator
Electrothermal instabilities effects on Brayton and Rankine cycle magnetohydrodynamic space power generation systems
Validity range of Saha equation for radiationless decay of high-density plasmas in magnetohydrodynamic power generation
A multimegawatt-class nuclear fission powered closed cycle magnetohydrodynamic space power plant using a helium/xenon working gas has been studied, to include a comprehensive system analysis. Total plant efficiency was expected to be 55.2 percent including pre-ionization power. The effects of compressor stage number, regenerator efficiency, and radiation cooler temperature on plant efficiency were investigated. The specific mass of the power generation plant was also examined. System specific mass was estimated to be 3 kg/kWe for a net electrical output power of 1 MWe, 2-3 kg/kWe at 2 MWe, and approx.2 kg/KWe at >3 MWe. Three phases of research and development plan were proposed: (1) Phase I-proof of principle, (2) Phase II-demonstration of power generation, and (3) Phase III-prototypical closed loop test.
Calculations of preionized plasma flow with finite recombination rate - magnetohydrodynamic power generator study
Liquid-metal magnetohydrodynamic (MHD) power generator with solar oven as its heat source has potential to produce electric power in space and on Earth at high efficiency. Generator focuses radiation from Sun to heat driving gas that pushes liquid metal past magnetic coil. Power is extracted directly from electric currents set up in conducting liquid. Using solar energy as fuel can save considerable costs and payload weight, compared to previous systems.
An investigation is presented on the way in which the generation of magnetohydrodynamic waves by turbulent motions in stellar convection zones depends on the star's effective temperature, surface gravity, and magnetic field strength. It is shown that the emitted Alfven wave flux (and acoustic slow wave flux in a very strong magnetic field) is in reasonable agreement with the general trend of observed chromospheric radiative losses in stars, and with the observations of three stars for which magnetic field strength, surface area covered by strong fields, and radiative losses have all been measured.