Abstract—The formation of impact craters on the Earth’s surface is accompanied by the effect of shock waves on rocks. The shock wave compression results in rocks heating up to the point of melting and evaporation during unloading. The direct mechanical action of shock compression and residual heating change the magnetic properties of rocks. Geophysical modeling is used to determine the sources of the magnetic anomaly by interpreting the fields measured on the surface, but such modeling does not take into account the impact demagnetization of rocks. This work gives an example of analysis of the magnetic anomaly over the well-studied Bosumtwi crater (Ghana, 10.5 km diameter, 1 million years old), including the numerical modeling of the crater formation process and the construction of a magnetic anomaly model based on the simulated shock compression parameters and crater drilling data. It is shown that the morphological features of the crater— the crater rim and the central uplift—form positive magnetic anomalies around and inside the crater.
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The authors are deeply grateful to the reviewers for their careful examination of the manuscript and their valuable suggestions for its improvement. The authors have tried to take into consideration the comments as much as possible.
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Kuzmicheva, M.Y., Ivanov, B.A. Modeling the Magnetic Anomaly of the Bosumtwi (Ghana) Complex Meteorite Crater by Taking Into Account the Impact Demagnetization and Morphological Features. Izv., Phys. Solid Earth 57, 795–804 (2021). https://doi.org/10.1134/S1069351321050128
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DOI: https://doi.org/10.1134/S1069351321050128