Published April 1964 | Version public
Journal Article

Microseisms and an attempted application to exploration

Abstract

A study of microseisms is made to determine some of their statistical properties and to investigate the feasibility of their use in determining the structures in the upper several kilometers of the earth's crust by the phase‐velocity method. It is found that the microseisms in the period range of 1 to 6 sec arrive from several directions with comparable strength and at the same time. There are occasional short intervals of 10 to 40 sec during which microseisms are mostly unidirectional. It is also found that these relatively short‐period microseisms are not stationary in the wide sense over time intervals longer than 5 or 10 minutes. The phase velocities of microseisms recorced with an array of eight instruments are measured in four different locations. The velocities, although scattered, are found to be in agreement with the computed theoretical dispersion curve for the fundamental Rayleigh mode, based on the available seismic velocity information. An error analysis is made and the confidence limits are placed within ±20 percent of the measured velocities. It is concluded that in determining shallow crustal structures the microseism‐phase‐velocity method potentially is at least as effective as the gravity method, although it is not as suitable for routine work as the gravity method.

Additional Information

© 1964 Society of Exploration Geophysicists. The author is indebted to Professor Frank Press for suggesting the problem and for his support and guidance throughout this study. The microseism recordings in Tulsa, Oklahoma, were made by the Jersey Production Research Company. Grateful acknowledgment is given to the Company and especially to Mr. F. G. Boucher for giving us the data. In China Lake, the recording was carried out within the Naval Ordnance Test Station. The author is grateful to Captain C. Blenman, Jr., the Commander, NOTS, for granting permission; and to Drs. P. St. Arnaud, K. Odencratz, and to Mr. R. Zbur for their valuable assistance. Mr. N. Motta's most valuable help in design and building of instruments for microseism recording is acknowledged. This research was supported by Grant No. AF-AFOSR-25-63 of the Air Force Office of Scientific Research as part of the Advanced Research Projects Agency Project VELA, and by the National Science Foundation.

Additional details

Identifiers

Eprint ID
122094
DOI
10.1190/1.1439344
Resolver ID
CaltechAUTHORS:20230701-403291000.3

Related works

Describes
10.1190/1.1439344 (DOI)

Funding

Air Force Office of Scientific Research (AFOSR)
AF-AFOSR-25-63
Advanced Research Projects Agency (ARPA), project Vela

Dates

Created
2023-07-05
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Updated
2023-07-05
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Caltech Custom Metadata

Other Numbering System Name
Caltech Division of Geological Sciences
Other Numbering System Identifier
1192