Limits on the seismic velocity profile of the moon's outer layers determined by the tau method

Details Limits on the seismic velocity profile of the moon's outer layers determined by the tau method Limits on the seismic velocity profile of the moon's outer layers determined by the tau method

Aug 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975sval....1..172b&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 1, Aug. 1975, p. 37-42.) Soviet Astronomy Letters, vol. 1, July-Aug. 1975, p. 172-174.

Astronomy and Astrophysics

Astronomy

Lunar Mantle, Moonquakes, Propagation Velocity, Seismic Waves, Curve Fitting, Hodographs, Lunar Maria, Selenology, Velocity Distribution

Scientific paper

The body wave travel time data obtained from the Apollo program are analyzed. Using a spherically symmetric model of the moon, these seismic data were inverted by the tau-method. The upper and lower bounds for the seismic velocity structure up to depth of 100 km in Fra Mauro region in Oceanus Procellarum are constructed. One velocity-depth curve within this area fitting travel times is given.

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