Amplitude variations of 15-GHz radio waves transmitted through clear air and through rain
Point to point and radar return attenuation measurements at SHF through clear air and rain
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Point to point and radar return attenuation measurements at SHF through clear air and rain
Plasma lasers, investigating striation oscillations and excess noise phenomena and generation mechanisms
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Investigating dynamic nonshock properties of microscale fluctuations in interplanetary medium using plasma and magnetic field data from Mariner 5 space probe
Aluminum panel flutter tests at supersonic Mach numbers
Cosmic ray intensity mean diurnal variation, taking into account angle between solar corotational velocity and earth equatorial plane
Auroral pulsation analysis from rocket soundings, investigating oxygen green linear excitation sources
At Ancon, Peru, simultaneous observations of 1550-MHz and 136-MHz signals from the ATS 5 and Intelsat-1 spacecraft showed ionospheric fading as great as 27 db at 136 MHz and 6 db at 1550 MHZ. The observations were made on 48 days during the 1970 autumnal and 1971 vernal equinox periods. Comparison of the two frequencies, in respect to rates and depths of fades, is made. Statistical distributions of the received signal levels during ionospheric scintillation occurrences are presented which may be of use to communications system engineers with operational requirements in the equatorial regions. The distributions show that during expected periods of scintillation, the L band signal typically falls 1.1 db below the median for 1.0 percent of the time, and the VHF signal falls 11.5 db below the median for 1.0 percent of the time.
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Description of the design and performance of a dual-band electronically despun, high-gain, earth-coverage satellite antenna for use on the Synchronous Meteorological Satellite. The SMS satellite is designed to take high-resolution cloud cover pictures from synchronous altitude. Several unique design features are described, including a scheme for steering energy around the array in a continuous fashion to avoid 'phase jumps' caused by sudden energy switches.
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Beam may be smoothly scanned around ring array without instantaneous phase transitions while maintaining constant radiated power by gradually transferring power from receding element to element next to leading edge of driven segment, and by accomplishing antenna element switching during intervals when no power is being applied to elements being switched.
The design and construction of inductive transducers for measuring the vibrations in metal bars at ultrasonic frequencies are discussed. Illustrations of the inductive transducers are provided. The quantitative relations that are useful in designing the transducers are analyzed. Mathematical models are developed to substantiate the theoretical considerations. Results obtained with laboratory equipment in testing specified metal samples are included.
A stable excitation supply for measurement transducers is described. It consists of a single-transistor oscillator with a coil connected to the collector and a capacitor connected from the collector to the emitter. The output of the oscillator is rectified and the rectified signal acts as one input to a differential amplifier; the other input being a reference potential. The output of the amplifier is connected at a point between the emitter of the transistor and ground. When the rectified signal is greater than the reference signal, the differential amplifier produces a signal of polarity to reduce bias current and, consequently, amplification.
The geometry of the bending of a linear triatomic molecule is analyzed, and an expression for the average rotational constant is derived. A harmonic oscillator model of C3 is fitted to the observed rotational constant within 0.6%. The bond distance between atoms at zero bending is 1.287 A according to this model; this is noticeably larger than the average internuclear distance of 1.277 A for the vibrational ground state. The first order perturbation solutions for the vibrational energy levels, taking into account the effect of a quartic perturbation potential, closely match observed levels. For a square well potential model of C3, the effect of curvilinear motion in bending is similar to that found for the harmonic oscillator model, though the decreases in energy are about twice as large. In both models, the average energy decrease is relatively constant at approximately 10% over a wide range of vibrational quantum number.
Intensity variations in the Rayleigh-Jeans portion of the solar continuum spectrum, longward of 1 micron, permit direct observations of the temperature structure of the solar atmosphere. A table indicates the source heights in the HSRA model atmosphere (Gingerich et al. 1971) for several of the infrared windows available for ground-based observations. The existence of 300-sec oscillations in the infrared continuum provides a powerful new tool for the exploration of this phenomenon: variation with altitude, spatial structure, relative phase of temperatures and velocity variations, etc. The initial observations at 20 micron are reported.