Term | Definition |
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Fault Distance | The fault distance (RF) is one of the measures of the source-site distance currently used in the engineering and seismology applications. It is defined as the minimum distance between the observation point and the earthquake fault. Different source-to-site distances are commonly used, such as: Hypocentral distance (M1): distance from the earthquake hypocenter; Epicentral distance (M2) = distance from the earthquake epicenter; Distance from the most energetic zone (M3) = distance from the zone of maximum energy release; Distance from the seismic source or distance from the fault (M4) = minimum distance between the site and the earthquake fault; Distance from the surface projection of the fault (Joyner-Boore distance) = minimum distance between the site and the fault projection on the ground surface (M5).
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