Figure 13.
Synthetic RF for station Novo obtained by forward modelling (Kind et al. 1995) with a slowness of 6.4 s deg−1. We took the velocity depth model retrieved from a seismic experiment (Kogan 1992), which is denoted with KOGAN and a red dotted line. As a second model we took the IASP91 Earth model (red solid line). The model with the abbreviation LVZ on the right side (blue line) contains a low-velocity zone (LVZ) within the upper mantle. The black dashed lines are the sum trace of 10 single RF.

Synthetic RF for station Novo obtained by forward modelling (Kind et al. 1995) with a slowness of 6.4 s deg−1. We took the velocity depth model retrieved from a seismic experiment (Kogan 1992), which is denoted with KOGAN and a red dotted line. As a second model we took the IASP91 Earth model (red solid line). The model with the abbreviation LVZ on the right side (blue line) contains a low-velocity zone (LVZ) within the upper mantle. The black dashed lines are the sum trace of 10 single RF.

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