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How we processed Apollo lunar seismic dataThe Apollo lunar seismic station network gathered data continuously at a rate of 3 x 10 to the 8th bits per day for nearly eight years until termination in September, 1977. The data were processed and analyzed using a PDP-15 minicomputer. On average, 1500 long-period seismic events were detected yearly. Automatic event detection and identification schemes proved unsuccessful because of occasional high noise levels and, above all, the risk of overlooking unusual natural events. The processing procedures which were finally chosen consist of plotting all the data on a compressed time scale, visually picking events from the plots, transferring event data to separate sets of tapes and performing detailed analyses using the latter. Many problems remain, especially in the automatic processing of extraterrestrial seismic signals.
Document ID
19800042043
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Nakamura, Y.
(Texas Univ. Galveston, TX, United States)
Latham, G. V.
(Texas Univ. Galveston, TX, United States)
Dorman, H. J.
(Texas, University Galveston, Tex., United States)
Date Acquired
August 10, 2013
Publication Date
February 1, 1980
Subject Category
Lunar And Planetary Exploration
Accession Number
80A26213
Funding Number(s)
CONTRACT_GRANT: NAS9-14580
CONTRACT_GRANT: NSG-7418
CONTRACT_GRANT: NAS9-14810
Distribution Limits
Public
Copyright
Other

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