Publications

The gain of shallow paraboloid reflector antennas with random surface deviations has been derived by Ruze.

Recently, a standard horn was used as a calibration reference in measuring the gain of a 400-square foot aperture horn-reflector antenna at 4080 mcs.1 Since the horn-reflector antenna is currently

The gain of a highly efficient erbium-doped fiber amplifier was measured when pumped at wavelengths between 1.46microns and 1.51microns.

The use of a directional terminal antenna on a wireless link can enhance received power by as much as the antenna gain. In local scattering, however, the enhancement will be smaller.

The gain saturation of optical amplifiers due to changes in wavelength-division-multiplexed channel loading is characterized using a technique that determines the saturation effect on each channel.

We present a device which produces changes in the slope of its transmitted spectra via an applied bias, a Spectrally Linear Optical Power Equalizer, or SLOPE device.

We report on the spatial uniformity of the gain M of InP/InGaAsP/InGaAs avalanche photodiodes with separate absorption, grading, and multiplication regions (SAGM-APDs).

This work enables one to obtain the potential gain (G(T)) characteristics with the associated source (Z(S)) and load (Z(L)) termination functions, depending upon the input mismatching (V-i), noise

Optical notch and long-period grating (LPG) gain-equalizing filters are modeled and studied, and their performances are compared and contrasted for the case of optical waveguide amplifiers for inte

Modes in cylindrical structures with refractive index boundaries are well known.