Standard Back-Projections (BPs) use P phase recordings at large aperture
arrays within teleseismic distances (30°-90°) to image earthquake
sources. However, the majority of sizable arrays are in the northern
hemisphere, leaving many southern hemisphere earthquakes beyond the
teleseismic range. We extend the BP method by utilizing seismic waves
traveling through the Earth’s core, expanding our capability to image
earthquakes worldwide. Our core phase BPs incorporate PKIKP (150°-180°)
and PKP (145°-175°) phases. We evaluate their theoretical resolutions
using 1-D and 2-D array response functions and test uncertainties by
adding white noise to coherent waveforms. Tests show that core phase BPs
achieve resolutions and uncertainties comparable to P phase BP. We
validate the method using a synthetic model of a unilateral rupture (Mw
7.45, 2 km/s) and demonstrate accurate recovery of rupture direction,
length, and speed. Applying core phase BPs to the 2010 Mw 8.8 Chile and
2015 Mw 7.1 southeast Indian Ridge earthquakes, we compare our results
with published BPs and/or slip models, confirming the feasibility and
reliability of core phase BPs. We then apply core phase BPs to five
understudied earthquakes in the southwest Pacific region, providing
insights into these pelagic earthquakes. Core phase BPs play a crucial
role in scenarios where teleseismic arrays are unavailable, and have
weaker array-dependent effect and better performance in bilateral
rupture imaging. Finally, we discuss the limitations of core phase BPs
and outline potential avenues for future research.