Effect of the motion of a strongly magnetized plasma on the emission of radiation by a finite dipole.
Magnetized cold plasma motion effect on electromagnetic wave propagation and radiation
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Magnetized cold plasma motion effect on electromagnetic wave propagation and radiation
RF harmonic and intermodulation distortion produced by glow discharge and high energy flame plasmas during electromagnetic wave propagation
Thermal anisotropy of electrons and instability of circularly polarized electromagnetic waves propagating along magnetic field in solar wind
Electromagnetic wave propagation in transversely magnetized warm plasma filled rectangular waveguide, analyzing TE and TM modes
Noise signals in earth magnetosheath interpreted as electromagnetic waves propagating in whistler mode
Slow electromagnetic wave propagation in superconducting thin film transmission lines, noting phase velocity dependence on film thickness and spacing
Very low frequency electromagnetic hiss propagation along geomagnetic field in earth magnetosphere
Parametric coupling between space-time harmonics of electromagnetic wave propagating in dielectrics modulated by pump wave
Monograph on ionosphere-satellite interactions, discussing ionosphere layers, plasma sheaths and wakes, electromagnetic wave propagation, spacecraft antennas, etc
Stochastic differential equations objectives, limitations and restrictive assumptions in physical problems, discussing electromagnetic wave propagation in random continuum or random dAlembertian operator
Ordinary mode electromagnetic wave propagation instability in high beta plasma, determining lower bound on growth rate
Investigating electromagnetic wave propagation in uniformly accelerated medium
Space station plasma physics experiments, investigating electron and ion wakes, resonance, VLF electromagnetic energy propagation and magnetospheric phenomena
General relativistic time delay of electromagnetic radiation propagation due to solar gravitational field measured from Mariner 6 and 7 range and Doppler data
Least squares and sequential estimation techniques application to Mariner 6 and 7 tracking data analysis, verifying Einstein relativity theory on electromagnetic radiation propagation
A theoretical analysis on the multiple scattering of electromagnetic waves propagating in a finite inhomogeneous medium is presented and applied to the study of wave propagation in a clear atmosphere (fine weather conditions). It is shown that the analysis offers a method of synthesizing the water vapor density profile in a clear atmosphere by measuring the resultant reflections from the density profile at several different frequencies. It is also shown that the resultant reflection emerges as the consequence of multiple scattering of partial reflections from various parts of the inhomogeneous medium. The solutions of the multiple scattering approach are shown to be more accurate than those of the WKB approach, which neglects the multiple scattering effects.
A computer program is used to evaluate a 25.4 cm X-ray telescope at a field angle of 20 minutes of arc by geometrical analysis. The object is regarded as a point source of electromagnetic radiation, and the optical surfaces are treated as boundary conditions in the solution of the electromagnetic wave propagation equation. The electric field distribution is then determined in the region of the image and the intensity distribution inferred. A comparison of wave analysis results and photographs taken through the telescope shows excellent agreement.
The electromagnetic waves propagating through a drifting semiconductor plasma are studied from a macroscopic point of view in terms of double-stream interaction. The possible existing waves (helicon waves, longitudinal waves, ordinary waves, and pseudolongitudinal waves) which depend upon the orientation of the dc external magnetic field are derived. A powerful impedance concept is introduced to investigate the wave behavior of longitudinal (space charge) waves or pseudolongitudinal waves in a semiconductor plasma. The impedances due to one- and two-carrier stream interactions were calculated theoretically.