Design and construction of a lunar seismograph progress report no. 10, 1 oct. - 31 dec. 1961
Lunar seismograph design and construction, Ranger data analysis equipment installation, and Surveyor project seismograph system testing
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Lunar seismograph design and construction, Ranger data analysis equipment installation, and Surveyor project seismograph system testing
Design and construction of a lunar seismograph
Lunar seismograph for surveyor
Ranger spacecraft lunar seismograph
Spherical and torsional oscillations of moon by long-period seismograph for investigation of internal lunar structures
Vertical component seismograph for use in Surveyor lunar landing missions
Recording equipment for rocket engine vibration is adaptable to determining the structural strength of building materials. This seismographic system is portable and is capable of measuring displacements in the direction of three mutually perpendicular axes.
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Scattering in a high-Q medium has been the best hypothesis to date for explaining the observation of a long, reverberating train of waves in lunar seismographs. To test this hypothesis qualitatively, two experiments were devised which simulated this scattering and reproduced actual lunar seismographs. Pulses were propagated across a plate with grooves cut half-way through, and then were propagated along the edge of a plate with holes drilled within a skin depth of the edge. The seismographs of near impacts and moonquakes recorded by the Apollo 12 station in two frequency bands were studied. The impacts were those of S4B Saturn boosters and LM ascent stages. Interpretation of these data suggests the existence of a scattering layer 25 km thick with a Q of 5000. The density of the scatterers decreases with depth, suggesting that they are associated with cratering, or that they consist of cracks which anneal with depth.
The Satellite Telemetry Earthquake Monitoring Program was started to evaluate the applicability of satellite relay telemetry in the collection of seismic data from a large number of dense seismograph clusters laid out along the major fault systems of western North America. Prototype clusters utilizing phone-line telemetry were then being installed by the National Center for Earthquake Research in 3 regions along the San Andreas fault in central California; and the experience of installing and operating the clusters and in reducing and analyzing the seismic data from them was to provide the raw materials for evaluation in the satellite relay telemetry project. The principal advantages of the satellite relay system over commercial telephone or microwave systems were: (1) it could be made less prone to massive failure during a major earthquake; (2) it could be extended readily into undeveloped regions; and (3) it could provide flexible, uniform communications over large sections of major global tectonic zones. Fundamental characteristics of a communications system to cope with the large volume of raw data collected by a short-period seismograph network are discussed.
Seismographic study of spheroidal free periods of earth oscillation
Transistor low noise seismic amplifier for fractional mv signals at ELF in ocean bottom seismographs and magnetic variometer
Design of three-axes seismographic system for Apollo lunar landing mission
Seismograph used for measuring natural seismic activity and similar man-made disturbances like large rocket firings, showing propagation of disturbance by ground and not by atmosphere
Four-component, three-axis, feedback-controlled seismograph incorporates electronic circuitry for leveling and for monitoring the feedback signal required for servo-centering. Viscous damping of the earth-motion signal, compensation of the residual long-term drift, and centering of the seismometers are provided by automatic mechanisms.
Secondary ejecta explanation to seismograph of Apollo 12 LM impact