Finite and infinite H-plane bifurcation waveguide with anisotropic plasma medium.
H-plane bifurcation of parallel plate waveguide filled with anisotropic plasma
SEARCH · Search NASA
Search indexed NASA NTRS and DOE OSTI research on propulsion, heat transfer, battery materials and energy systems. Follow report and document links to the original sources.
Quote a phrase for an exact phrase match. Source license links do not imply unrestricted reuse.
H-plane bifurcation of parallel plate waveguide filled with anisotropic plasma
Point matching method calculation of cut-off frequencies and field configurations of waveguides with general cross section
Propagation of optical-waveguide modes in dielectric slab bisected by metal sheel
Coupled waveguides structure proposed as leaky- wave antenna, extending previous coupled-mode theory
Higher order diffraction concept applied to computation of parallel-plate waveguide aperture radiation patterns
Reflection coefficient of transverse electromagnetic mode parallel plate waveguide illuminating perfectly reflecting sheet
Acceleration of plasmoids in waveguides by superhigh-frequency electromagnetic wave
Aperture reflection coefficient of parallel plate waveguide by wedge diffraction analysis
Design, fabrication, and testing of optical waveguides and components for laser applications
Input admittance of rectangular waveguide antenna radiating into inhomogenous lossy plasma slab and dielectric constant variations
Mutual coupling between TEM and TE 01 parallel- plate waveguides calculated, using wedge diffraction techniques
Point matching method, solving boundary value problem in uniform cylindrical waveguide with inserted conductor within conducting tube
Rectangular to cylindrical waveguide transducer which couples dominant rectangular and cylindrical transverse electromagnetic modes
Optical detector using length of single mode optical waveguide with photodetector at output for null detection
None given. Paper covers the NASA Deep Space Network (DSN) Goldstone Complex in Mojave, California, and their beam-waveguide (BWG) antenna complex. They discuss system noise temperature,its major contributor, and its correction.
At the NASA Deep Space Network (DSN) Goldstone Complex, a 34-meter- diameter beam-waveguide antenna, DSS-13, was constructed in 1988-1990 and has become an integral part of an advanced systems program and a test bed for technologies being developed to introduce Ka-band (32 GHz) frequencies into the DSN. A method for compensating the gravity- induced structural deformations in this large antenna is presented.
A 34m diameter antenna, built for NASA/JPL in 1990 at Goldstone, California, utilizes a beam-waveguide (BWG) design. It was discovered that if a dichroic plate is installed in a BWG antenna environment, high noise temperatures can result if the receiver system passband is greater than the passband for which the plate was designed. A method is presented for accurately calculating dichroic plate noise temperature for these conditions.
A novel split-waveguide mount for millimeter and submillimeter wave frequency multipliers and harmonic mixers is presented. It consists of only two pieces, block halves, which are mirror images of each other.