Dielectric constant of vegetation at 8.5 GHz
Measurement of dielectric constant of vegetation at microwave frequencies by cavity perturbation method
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.
Measurement of dielectric constant of vegetation at microwave frequencies by cavity perturbation method
Dielectric cover effects on radiation properties of cross slots in rectangular antenna
Input admittance of rectangular waveguide antenna radiating into inhomogenous lossy plasma slab and dielectric constant variations
Optical scattering cross sections for polydispersions of dielectric spheres, showing dependence on ratio of third to second moment of shape and size distribution function
Dielectric constant of homogeneous fully ionized two-temperature plasma for determining conditions under which ion waves can be found
Composite metallic and dielectric insulators for high current arc electrodes
Dielectric relaxation of gases and sharp rise in microwave absorption coefficient in Cytherean atmosphere
Plane electromagnetic wave reflection and refraction by semiinfinite dielectric medium moving uniformly parallel to surface analyzed for arbitrary incidence plane orientation
Electric breakdown, dielectric constant and dissipation factors of cryogenic liquid nitrogen, hydrogen and helium
Thin films deposited onto substrates cooled to low temperatures investigated for transition temperature in structures of superconductor- dielectric-superconductor
Dielectric cover effect on resonant frequency of slots in rectangular waveguide, using Stevenson free space theory and plane-wave reflection coefficient
Surface wave pole contribution to admittance of rectangular waveguide-fed slot into dielectric slab
This paper describes how expansions in leaky (or improper) modes may be used to represent the continuous spectrum in an open radiating waveguide. The technique requires a thorough knowledge of the life history of the improper modes as they migrate from improper to proper Riemann surfaces. The method is illustrated by finding the electric field resulting from an impulsively forced current located in the free space above a grounded dielectric slab.
The scattering properties of perfectly conducting and resistive strips are predicted for strips which are located on a dielectric slab backed by a perfectly conducting ground plane. The spectral domain Green's function is used to relate the currents and fields on the strip, and the resulting integral equation is solved using the method of moments. Both TE and TM strips are examined using piecewise linear and pulse subdomain basis functions, respectively, to model the current on the strip. Calculated results are compared with results measured at the NASA Langley Research Center.
Design and implementation of a system for the automated and continous in situ monitoring of the dielectric constant of woody vegetation tissue is presented.
This presentation addresses the progress made so far in the development of an antenna array with reconfigurable transmission line feeds connecting each element in series. In particular, 2D traveling wave array employing trapezoidal Dielectric Wedge for Beam Steering will be discussed. The presentation includes current status of the effort and suggested future work. The work is being done as part of the NASA Office of the Chief Technologist's Space Technology Research Fellowship (NSTRF).
Cassini is an international spacecraft mission facilitated by NASA and ESA which seeks to understand the Saturn planetary system, including rings and moons. Launched in 1997, the Cassini spacecraft contains two major components: the Cassini orbiter that has been orbiting Saturn since October 2004, and the European-built Huygens probe that landed on Titan's surface in December 2004 to study its geology and atmosphere. Titan, Saturn's largest moon and the second largest moon in the solar system, possesses surface and atmospheric features similar to those of Earth, including lakes, seas, and mountains. A physical characterization of these features is critical to understanding the origin and evolution of Titan, whose surface composition reflects its geological history. Because Titan's atmosphere is largely composed of methane, it is believed that surfaces lakes are filled with mixtures of liquid hydrocarbons. The Cassini orbiter's RADAR instrument has been scanning Titan's surface at the atmosphere-penetrating microwave frequency of 13.8 Gigahertz since 2004. However, accurate interpretation of these data is limited by a lack of knowledge regarding dielectric properties of liquid hydrocarbons at cryogenic temperatures. Therefore, it is of specific interest to experimentally determine values for the complex permittivities of various liquid hydrocarbon mixtures at the surface conditions of Titan. In particular, more accurate values for complex permittivity would improve estimates of lake depth and surface composition obtained from the instrument's altimetry and backscatter modes.
We are concerned with the design of inhomogeneous, all dielectric (lossless) periodic structures which act as filters.