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We use the cosine-type source time function for convolution of waveforms for these five smaller events.
Source time histories for different source components can be kept independent, so that superposition of different physical phenomena can be retrieved, even in cases where they occur with different timing.
8 source time function for FDM simulations.
2, 3, 4, 5, and 6 source time functions for FDM simulations.
Hypocentral distance variations for amplitude level variance in a random inhomogeneous media using medium model A and the no. 1 and 6 source time functions for FDM simulations.
Spatial and hypocentral distance distribution of wave amplitudes in random inhomogeneous media using medium model A and the no. 1 and 6 source time functions for FDM simulations.
Source time functions for subfaults and temporal rupture images suggest that repeated slips occurred in the primary rupture, which is consistent with that from seismic waveforms.
Tetrakis(dimethylamino)hafnium (Hf[N(CH3 2]4) and H2O are used as precursor sources; pulse times for hafnium source and water source are both 15 ms per circle.
Furthermore, this estimation significantly depends on the pulse width of the source time function used for calculating the convolution.
Fig. 10 Amplitude variations for different source time durations.
Hypocentral distance variations of amplitude level variance for different source time functions using medium model A and the no. 1, 6, 7, and 8 source time functions for FDM simulations.
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