Electronic Supplement to
Preparing for InSight: An Invitation to Participate in a Blind Test for Martian Seismicity

by J. F. Clinton, D. Giardini, P. Lognonné, B. Banerdt, M. van Driel, M. Drilleau, N. Murdoch, M. Panning, R. Garcia, D. Mimoun, M. Golombek, J. Tromp, R. Weber, M. Böse, S. Ceylan, I. Daubar, B. Kenda, A. Khan, L. Perrin, and A. Spiga

This electronic supplement includes figures for each candidate 1D model for use in the InSight (Interior exploration using Seismic Investigations, Geodesy and Heat Transport) blind test that are not shown in the main article.

---

Figures

Figure S1. Vertical profile of (a) seismic velocities and density, (b) flat Earth transformed seismic velocities, (c) dispersion curves, and (d) travel times for model EH45Tcold. Low-velocity zones (LVZ, regions with a negative velocity gradient for either or both P and S) are indicated in gray in (b). The LVZ may or may not lead to shadow zones for direct-arriving phases shown in (d).

Figure S2. Same as Figure S1 for model EH45TcoldCrust1.

Figure S3. Same as Figure S1 for model EH45TcoldCrust1b.

Figure S4. Same as Figure S1 for model EH45ThotCrust2b.

Figure S5. Same as Figure S1 for model DWThot.

Figure S6. Same as Figure S1 for model DWThotCrust1.

Figure S7. Same as Figure S1 for model DWThotCrust1b.

Figure S8. Same as Figure S1 for model Gudkova.

Figure S9. Same as Figure S1 for model LFAK.

Figure S10. Same as Figure S1 for model MAAK.

Figure S11. Same as Figure S1 for model SANAK.

Figure S12. Same as Figure S1 for model TAYAK.

[ Back ]