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ABSTRACT Maximum lunar seismic activity corresponds to the rise of the pulsar CP1133 at the site. Other agreement with Earth based experiments suggests that they have a common origin. Access
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SIMILAR CONTENT BEING VIEWED BY OTHERS MAGNETAR SPIN-DOWN GLITCH CLEARING THE WAY FOR FRB-LIKE BURSTS AND A PULSED RADIO EPISODE Article 12 January 2023 GRAVITY-INDUCED SEISMICITY MODULATION
ON PLANETARY BODIES AND THEIR NATURAL SATELLITES Article Open access 28 January 2024 TECTONICS OF CERBERUS FOSSAE UNVEILED BY MARSQUAKES Article 27 October 2022 REFERENCES * Latham, G., _et
al._, _Science_, 174, 687 (1971). Article ADS CAS Google Scholar * Sadeh, D., and Meidav, M., _Nature_, 240, 136 (1972). Article ADS Google Scholar Download references AUTHOR
INFORMATION Author notes * DROR SADEH: And E. O. Hulburt Center for Space Research, Naval Research Laboratory, Washington DC 20390. AUTHORS AND AFFILIATIONS * Physics and Astronomy
Department, F. and G. Wise Observatory, University of Tel-Aviv, Tel-Aviv, Israel DROR SADEH Authors * DROR SADEH View author publications You can also search for this author inPubMed Google
Scholar RIGHTS AND PERMISSIONS Reprints and permissions ABOUT THIS ARTICLE CITE THIS ARTICLE SADEH, D. Possible Sidereal Period for the Seismic Lunar Activity. _Nature_ 240, 139–140 (1972).
https://doi.org/10.1038/240139a0 Download citation * Received: 26 June 1972 * Issue Date: 17 November 1972 * DOI: https://doi.org/10.1038/240139a0 SHARE THIS ARTICLE Anyone you share the
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