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How we processed Apollo lunar seismic data

Authors :
H. J. Dorman
Yosio Nakamura
G. V. Latham
Source :
Physics of the Earth and Planetary Interiors. 21:218-224
Publication Year :
1980
Publisher :
Elsevier BV, 1980.

Abstract

The 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.

Details

ISSN :
00319201
Volume :
21
Database :
OpenAIRE
Journal :
Physics of the Earth and Planetary Interiors
Accession number :
edsair.doi...........cf3b522448694545d28d04b756b9d216
Full Text :
https://doi.org/10.1016/0031-9201(80)90071-0