Literature DB >> 17781450

Passive seismic experiment.

G V Latham, M Ewing, F Press, G Sutton, J Dorman, Y Nakamura, N Toksöz, R Wiggins, J Derr, F Duennebier.   

Abstract

Seismometer operation for 21 days at Tranquillity Base revealed, among strong signals produced by the Apollo 11 lunar module descent stage, a small proportion of probable natural seismic signals. The latter are long-duration, emergent oscillations which lack the discrete phases and coherence of earthquake signals. From similarity with the impact signal of the Apollo 12 ascent stage, they are thought to be produced by meteoroid impacts or shallow moonquakes. This signal character may imply transmission with high Q and intense wave scattering, conditions which are mutually exclusive on earth. Natural background noise is very much smaller than on earth, and lunar tectonism may be very low.

Year:  1970        PMID： 17781450     DOI： 10.1126/science.167.3918.455

Source DB:  PubMed          Journal:  Science        ISSN： 0036-8075            Impact factor:   47.728


  1 in total

Review 1.  SEIS: Insight's Seismic Experiment for Internal Structure of Mars.

Authors:  P Lognonné; W B Banerdt; D Giardini; W T Pike; U Christensen; P Laudet; S de Raucourt; P Zweifel; S Calcutt; M Bierwirth; K J Hurst; F Ijpelaan; J W Umland; R Llorca-Cejudo; S A Larson; R F Garcia; S Kedar; B Knapmeyer-Endrun; D Mimoun; A Mocquet; M P Panning; R C Weber; A Sylvestre-Baron; G Pont; N Verdier; L Kerjean; L J Facto; V Gharakanian; J E Feldman; T L Hoffman; D B Klein; K Klein; N P Onufer; J Paredes-Garcia; M P Petkov; J R Willis; S E Smrekar; M Drilleau; T Gabsi; T Nebut; O Robert; S Tillier; C Moreau; M Parise; G Aveni; S Ben Charef; Y Bennour; T Camus; P A Dandonneau; C Desfoux; B Lecomte; O Pot; P Revuz; D Mance; J tenPierick; N E Bowles; C Charalambous; A K Delahunty; J Hurley; R Irshad; Huafeng Liu; A G Mukherjee; I M Standley; A E Stott; J Temple; T Warren; M Eberhardt; A Kramer; W Kühne; E-P Miettinen; M Monecke; C Aicardi; M André; J Baroukh; A Borrien; A Bouisset; P Boutte; K Brethomé; C Brysbaert; T Carlier; M Deleuze; J M Desmarres; D Dilhan; C Doucet; D Faye; N Faye-Refalo; R Gonzalez; C Imbert; C Larigauderie; E Locatelli; L Luno; J-R Meyer; F Mialhe; J M Mouret; M Nonon; Y Pahn; A Paillet; P Pasquier; G Perez; R Perez; L Perrin; B Pouilloux; A Rosak; I Savin de Larclause; J Sicre; M Sodki; N Toulemont; B Vella; C Yana; F Alibay; O M Avalos; M A Balzer; P Bhandari; E Blanco; B D Bone; J C Bousman; P Bruneau; F J Calef; R J Calvet; S A D'Agostino; G de Los Santos; R G Deen; R W Denise; J Ervin; N W Ferraro; H E Gengl; F Grinblat; D Hernandez; M Hetzel; M E Johnson; L Khachikyan; J Y Lin; S M Madzunkov; S L Marshall; I G Mikellides; E A Miller; W Raff; J E Singer; C M Sunday; J F Villalvazo; M C Wallace; D Banfield; J A Rodriguez-Manfredi; C T Russell; A Trebi-Ollennu; J N Maki; E Beucler; M Böse; C Bonjour; J L Berenguer; S Ceylan; J Clinton; V Conejero; I Daubar; V Dehant; P Delage; F Euchner; I Estève; L Fayon; L Ferraioli; C L Johnson; J Gagnepain-Beyneix; M Golombek; A Khan; T Kawamura; B Kenda; P Labrot; N Murdoch; C Pardo; C Perrin; L Pou; A Sauron; D Savoie; S Stähler; E Stutzmann; N A Teanby; J Tromp; M van Driel; M Wieczorek; R Widmer-Schnidrig; J Wookey
Journal:  Space Sci Rev       Date:  2019-01-28       Impact factor: 8.017
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