Integrated Remote Sensing and Geophysical Investigations of the Geodynamic Activities at Lake Magadi, Southern Kenyan Rift

Figure 16

(a) Hill-shaded aster DEM subset showing the surface lineaments and the extracted aeromagnetic flight line 322. (b) Scatter Plots showing the subsurface relationship between magnetic sources on flight line 322, the hypocenters and the Curie-point (heat source). The magnetic sources are generated from 2D Euler deconvolution using structural index of 1 (i.e., contacts, faults) with inclinations and declination angles of −26.3° and 0.002°, respectively. R1 and R2 are the resistivity profiles 1 and 2, respectively.