BOMEX bulletin, no. 10
Radiosonde and radar echo measurements on area of air/sea interactions over tropical ocean surface with numerical weather forecasting
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Lidar observations in relation to the atmospheric winds aloft
Lidar observations of visually clear troposphere compared with simultaneous rawinsonde data for relationship between lidar echoes and atmospheric winds aloft
Collis, R. T. H.↗
Ultrasonic measurement of thin layers
Pulse echo ultrasonic measurement of thin film layer between thick media, using real time computation
Lees, S.↗
Map of lunar radar reflectivity at 7.5-m wavelength
Lunar radar reflectivity mapping at 7.5 m wavelength for maria and highlands echo powers, using interferometric techniques
Thompson, T. W.↗
Functional dependences of bistatic-radar frequency spectra and cross sections on surface scattering laws
Bistatic radar frequency spectra and cross sections dependence on surface scattering laws, studying echo bandwidth
Ingalls, D. H. H.↗
Anomalous ultrasonic attenuation in pure superconducting Nb
Anomalous ultrasonic attenuation in pure superconducting Nb from pulse echo amplitude measurements
Daniel, A. C.↗
Improved ultrasonic biomedical measuring apparatus
Device for making measurements of organs in living specimens and recording movements of organs is described. System uses series of ultrasonic pulses beamed into body of animal and reflected echo pulses are picked up by transducers and recorded. Diagram of equipment required and method of application is included.
Lee, R. D.↗
Ionospheric nf sub H resonances: Frequency shifts versus plasma conditions
The Alouette 2 resonances observed near the harmonics of the electron cyclotron frequency f sub H reveal frequency shifts (relative to the n(f sub H) values derived from model field calculations) which can be interpreted in terms of plasma wave dispersion effects. These effects are observed on the 2(f sub H) resonance when it is near the resonance observed close to the upper hybrid frequency f sub T. The observations suggest that an oblique echo model may be required to give a proper interpretation of the 2(f sub H) resonance. Cyclotron damping can be ignored only when the angle between the propagation vector and the direction perpendicular to the earth's magnetic field B is less than a few degrees for the 2(f sub H) wave, and less than a few tenths of a degree for the n(f sub H) waves with n 2. The negative offset of the absolute value of B inferred from the plasma resonance observations is consistent with expectations based on recent OGO 3 and OGO 5 rubidium magnetometer observations at higher altitudes in the equatorial regions.
Benson, R. F.↗
Testing general relativity: Progress, problems, and prospects
The results from ground-based experimental testing are presented. Prospects for improving these experiments are discussed. Radar echo time delays, perihelion advance and solar oblateness, time variation of the gravitational constant, and radio wave deflection are considered. Ground-based and spacecraft techniques are compared on an accuracy vs. cost basis.
Shapiro, I. I.↗
Research investigation directed toward extending the useful range of the electromagnetic spectrum
The lifetimes and fine structure of He(-) were studied using time-of-flight techniques and quenching by a static axial magnetic field. Using level-crossing spectroscopy the hyperfine constants A and B and the lifetime of the 3 2P3/2 state of Li-7 were measured. Polarization of the Ru 7S level was created as a first step in determining the hyperfine structure of the alkali excited S state. The parametric interaction between light and microwaves in optically pumped Rb-87 vapor were investigated. Measurements and analyses of transitions in formaldehyde and its isotopic species and in the lowest two excited vibrational states of H2CO were also made, as well as of transitions in furan, pyrrole, formic acid, and cyanoacetylene. The Hanle effect was studied in the NO molecule, and RF oscillators were developed with flat, wideband output to observe excited state hyperfine transitions at zero field. Data was generated on the time-dependent behavior of photon echoes in ruby. Stimulated Raman scattering was studied in atomic Tl vapor. A Q switched, temperature-tuned ruby laser was developed which operates between 6934 and 6938 A. The frequency shift due to resonant interaction between identical radiating atoms was calculated.
Hartmann, S. R.↗
Bistatic-radar investigation
A bistatic-radar study during the Apollo 15 flight is reviewed, with the orbiting command module as one terminal. Bistatic-radar slopes are compared to geological maps of Copernicus and Riphaeus mountain regions and Kepler region. Basic theory is discussed, including the radar echoes composed of the sum of the reflections from the moon area that is mutually visible from the spacecraft and earth. A signal receiving system and data processing system are outlined schematically.
Howard, H. T.↗
Methods of quantitative and qualitative analysis of bird migration with a tracking radar
Methods of analyzing bird migration by using tracking radar are discussed. The procedure for assessing the rate of bird passage is described. Three topics are presented concerning the grouping of nocturnal migrants, the velocity of migratory flight, and identification of species by radar echoes. The height and volume of migration under different weather conditions are examined. The methods for studying the directions of migration and the correlation between winds and the height and direction of migrating birds are presented.
Bruderer, B.↗
Neurophysiological findings relevant to echolocation in marine animals
A review of echolocation mechanisms in marine mammals, chiefly porpoises, is given. Data cover peripheral auditory and central neurophysiological specializations favorable to the analysis of echolocating clicks and their echoes. Conclusions show (1) signals are received from 50 up to at least 135 kHz, (2) sound is received through the mandible skin, and (3) the midbrain sites are insensitive to low frequencies (below 6 kHz).
Bullock, T. H.↗
Correlation between convection electric fields in the nightside magnetosphere and several wave and particle phenomena during two isolated substorms.
Correlation of several magnetoionospheric wave and particle phenomena previously linked observationally to magnetospheric substorms and inferred to involve convection electric fields with whistler measurements of convection activity during two relatively isolated substorms. The events occurred at about 0600 UT on July 15, 1965, and about 0500 UT on Oct. 13, 1965. The correlated phenomena include cross-L inward plasma drifts near midnight within the plasmaphere, diffuse auroral radar echoes observed near the dusk meridian, IPDP micropulsations (intervals of pulsations of diminishing period) in the premidnight sector, apparent contractions and expansions of the plasma sheet at about 20 earth radii in the magnetotail, and Pc 1/Pi 1 micropulsation events near or before midnight. Two new vlf phenomena occurred during the October 13 event - a noise band within the plasmasphere associated with a convecting whistler path, and ?hisslers,' falling-tone auroral-hiss forms repeated at intervals of about 2 sec.
Carpenter, D. L.↗
Radar studies of the equatorial electrojet at three frequencies.
Radar measurements at 16.25, 49.92, and 146.25 MHz of plasma irregularities in the equatorial electrojet were carried out with the objective to investigate the dependence upon wavelength of the properties of the type I and type II irregularities and to see to what extent this dependence is consistent with present theoretical ideas. The equipment and experimental procedure employed is discussed in detail, and the data obtained are analyzed. The following conclusions have been drawn: the Doppler velocity of the type I echoes corresponds to the acoustic velocity rather than the electron streaming velocity; the acoustic velocity varies with wavelength in at least approximate agreement with theory; and the type II irregularities are probably not excited directly, but rather result from nonlinear interactions among larger irregularities.
Balsley, B. B.↗
Radar observations of land breeze fronts.
Description of a radar-observed apparent land breeze front 12 to 14 n mi off the coast of Wallops Island, Va. Accompanying meteorological data show the land breeze at the shore to be a layer of cold air less than 300 ft deep moving seaward at approximately 2 knots. The radar observations show the land breeze vertical frontal surface sloping landward at about 20 deg, with convection over the warm water increasing the layer thickness to 2000 ft near the frontal zone. The radar-observed horizontal frontal surface is a sharp scalloped line echo in the lower 1000 ft, but becomes diffuse above. As the local circulation during daylight hours changes to a sea breeze, the land breeze front recedes toward land and dissipates.
Meyer, J. H.↗
Theory of discrete wave packets in the solar wind.
Discrete wave packets were observed by Ogo 5 and earlier satellites. These waves were believed to be in the whistler mode. Since their group velocities were found to be smaller than the solar-wind speed, these waves could not have been generated in the bow shock and could not have propagated upstream later. The present theory discusses a mechanism similar to that of the echo phenomenon in plasma physics discovered in recent years. The present theory enables us to explain (a) why the wave packets were associated with the bow shock, (b) why the wave packets were characterized by coherent oscillations, and (c) why the wave packets had group velocities smaller than the solar wind and yet could still occur in the solar wind. In short, our theory is able to interpret all the essential features deduced from the observational data.
Wu, C. S.↗
Venus - Topography revealed by radar data.
Surface height variations over the entire equatorial region on Venus have been estimated from extended series of measurements of interplanetary radar echo delays. Most notable is a mountainous section of about 3-kilometer peak height located at a longitude of 100 degrees (International Astronomical Union coordinate system). The eastern edge has an average inclination of about 0.5 degrees, which is unusually steep for a large-scale slope on Venus. The resolution of the radar measurements along the surface of Venus varied between about 200 and 400 kilometers with a repeatability in altitude determination generally between 200 and 500 meters. The mean equatorial radius was found to be 6050.0 plus or minus 0.5 kilometers.
Campbell, D. B.↗