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Geophysical Abstracts 152 January-March 1953

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30 GEOPHYSICAL ABSTRACTS <strong>152</strong>, JANUARY-MARCH <strong>1953</strong><br />

point source can be approximated by an explosion at a sufficient depth. Proof<br />

is presented that for distances r, greater than the length X of the wave, the<br />

amplitude of seismic wave can be represented by the formula A=Ao/r. Travel-<br />

time curves in the vicinity of the point source, for r\ they can be assumed to be rectilinear. These fundamental relations derived<br />

for amplitudes and travel-time curves of waves caused by harmonic source, can<br />

be extended to waves produced by impulses, generating quasi-sinusoidal<br />

vibrations. Author's summary, 8. T. V.<br />

14275. Kosminskaya, I. P. Interferentsiya seysmicheskikh voln, vyzyvayemykh<br />

garmonicheskim istochnikom [Interference of seismic waves from a<br />

harmonic source]: Akad. Nauk SSSR Izv., Ser. geofiz. no. 4, p. 33-54,<br />

1952.<br />

The interference of two seismic waves, sufficiently distant from the source of<br />

vibrations to be considered as plane, is discussed and formulas are given for the<br />

resulting amplitudes and for the phase of the composite wave. The derived<br />

formulas are then extended to the case of several waves, and a graphoanalytic<br />

method is suggested for construction of the resulting amplitudes and travel-time<br />

curves.<br />

By analysis of different shapes of the travel-time curves and of the curves of<br />

amplitudes of composite waves, examples can be shown of the dominant wave<br />

that has a greater or smaller velocity than the others. In certain cases this<br />

procedure makes it possible to find individual components from the seismograms.<br />

Master charts are suggested for such analysis. Indices are also established<br />

which show when a recorded seismic wave is a composite one, resulting from the<br />

interference of several simple waves. S. T. V.<br />

INSTBUMENTS AND METHODS OF OBSERVATION<br />

14276. Borisevich, Ye. S. Registriruyushchiye pribory dlya seysmicheskikh<br />

stantsiy [Recording apparatus for seismic stations]: Akad. Nauk SSSR<br />

Geofiz. Inst. Trudy no. 14 (141), p. 53-58,1952.<br />

This is general discussion of good recording equipment. The most important<br />

feature is said to be uniform rotation of the drum; variation in the length of the<br />

minute must be not greater than 0.3 percent. It is important to have both<br />

mechanical and optical recording. Precautions in installation and rules to be<br />

followed in the maintenance of the apparatus are given. Most of the article is<br />

devoted to a description and criticism of recording apparatus of Russian<br />

origin. 8. T. V.<br />

14277. Bwing, Maurice, and Press, Frank. Further study of atmospheric pres­<br />

sure fluctuations recorded on seismographs: Am. Geophys. Union Trans.,<br />

v. 34, no. 1, p. 95-100,<strong>1953</strong>.<br />

The predominant background disturbance on a long-period vertical seismograph<br />

is removed by providing compensation for atmospheric pressure fluctuations. A<br />

seismically-compensated, long-period microbarovariograph for study of pressure<br />

oscillations in the range 20-2000 sec is described. Comparison of records from<br />

the pressure-compensated seismograph and the seismically-compensated micro­<br />

barovariograph indicates that no significant ground motion is caused by direct<br />

coupling of atmospheric pressure fluctuations to the earth. Sample records are<br />

shown. Authors' Abstract

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