Wide band receiver system frequency divider
Wideband receiver system frequency divider
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Wideband receiver system frequency divider
Low noise receivers - traveling wave maser development
S-band receiver exciter ranging subsystem Blocks IIB and IIIB
Amplifier design evaluations in study to provide wideband receiver front end for radio astronomy purposes
Sensitive S-band noise receiver for Mariner Mars 1964 spacecraft program
Optical superheterodyne receiver
Decision region receivers for Sunblazer space experiment
Optimization of receivers for demodulating FM SIGNAL corrupted by Gaussian noise, and solution to maximum likelihood equation
System performance of phase coherent receivers preceded by bandpass limiters
Polarization-diversity telemetry receivers for combining FM/FM penetrometer data, noting signal fading
Satellite tracking simultaneous-lobing monopulse receiving system utilizing polarization diversity in coherent and noncoherent operational modes
Optical communication experiments to compare coherent and noncoherent optical detection fading characteristics in different weather conditions, using laser transmitter and optical superheterodyne receiver
A 600 GHz - 635 GHz waveguide SIS heterodyne receiver was built and used for astronomical observations at the Caltech Submillimeter Observatory (CSO) in Hawaii.
The most sensitive heterodyne receivers used for millimeter wave and submillimeter wave radioastronomy employ superconductor-insulator-superconductor tunnel junctions as the nonlinear mixing element.
The most sensitive heterodyne receivers used for millimeter wave and submillimeter wave radioastronomy employ superconductor-insulator-superconductor (SIS) tunnel junctions as the nonlinear mixing element.
So far, the most sensitive heterodyne receivers in the millimeter-wave and submillimeter-wave frequency ranges have used the mixing response of the quasiparticle currents in SIS tunnel junctions.
The Receiver Lab Telescope (RLT) is a ground-based terahertz telescope; it is currently the only instrument producing astronmical data between 1 and 2 THz. We report on our first measurements o the high CO transitions, which represent the highest frequency detection ever made from the ground. We also present initial observations of {N II} and discuss the implications of this non-detection for the standard estimates of the strength of this line.