The Seismic Signature of Turbiditic Channels Using Outcrops Analogs and Process-Based Simulations, from the Pab Sandston

2006 ◽  
Author(s):  
R. E. Eschard ◽  
T. Euzen ◽  
S. Lopez ◽  
A. Bourgeois
Keyword(s):  
Seismic Signature

Seismic Signature and Methodology Standard

2001 ◽  
Author(s):  
BIOLOGICAL LAB COLD SPRING HARBOR NY
Keyword(s):  
Seismic Signature

Analyzing bulk flow characteristics of debris flows using their high frequency seismic signature

2021 ◽  
Author(s):  
Zhen Zhang ◽  
Fabian Walter ◽  
Brian W. McArdell ◽  
Tjalling Haas ◽  
Michaela Wenner ◽  
...  
Keyword(s):  
High Frequency ◽  
Debris Flows ◽  
Flow Characteristics ◽  
Bulk Flow ◽  
Seismic Signature

scholarly journals Seismic signature of a hydrous mantle transition zone

2016 ◽  
Vol 250 ◽  
pp. 46-63 ◽  
Author(s):  
Vincent Thio ◽  
Laura Cobden ◽  
Jeannot Trampert
Keyword(s):  
Transition Zone ◽  
Mantle Transition Zone ◽  
Seismic Signature

scholarly journals Seismic signature of active intrusions in mountain chains

2018 ◽  
Vol 4 (1) ◽  
pp. e1701825 ◽  
Author(s):  
Francesca Di Luccio ◽  
Giovanni Chiodini ◽  
Stefano Caliro ◽  
Carlo Cardellini ◽  
Vincenzo Convertito ◽  
...  
Keyword(s):  
Seismic Signature

The Seismic Signature of the Eifel Plume

Mantle Plumes ◽  
2007 ◽  
pp. 379-404 ◽  
Author(s):  
Joachim R. R. Ritter
Keyword(s):  
Seismic Signature

scholarly journals On The Seismic Signature of the HeII Ionization Zone in Stellar Envelopes

1998 ◽  
Vol 185 ◽  
pp. 317-318
Author(s):  
Mário J.P.F.G. Monteiro ◽  
Michael J. Thompson
Keyword(s):  
Equation Of State ◽  
Stellar Structure ◽  
Ionization Zone ◽  
Characteristic Signal ◽  
Oscillation Frequencies ◽  
Stellar Envelopes ◽  
Seismic Signature ◽  
Better Than

Sharp variations of the structure of the star create a characteristic signal in its frequencies of oscillation (e.g. [3]). The zone of the second ionization of helium is such a localized feature of the structure whose properties depend mainly on the abundance of helium and the equation of state. Considering that such a signal should easily be detectable provided the frequencies are measured to rather better than 1μHz accuracy (the COROT project should measure oscillation frequencies with an accuracy of 0.1μHz), we present here a tool to study this aspect of stellar structure.

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