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Earth, Planets and Space
Fig. 3 | Earth, Planets and Space

Fig. 3

From: Modeling and inversion of the microtremor H/V spectral ratio: physical basis behind the diffuse field approach

Fig. 3

(Left) Stratigraphy profiles of model N104 studied within the SESAME Project. (Right) Black line shows H/V computed at the surface of model N104 excited with synthetic noise. The bars indicate the standard deviation. With black continuous line and gray dotted line, the results of the computations using the DFA with no damping (1/Q = 0) and with 1/Q = 0.005 (Q = 200), respectively

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