Hubbry Logo
Strong ground motionStrong ground motionMain
Open search
Strong ground motion
Community hub
Strong ground motion
logo
8 pages, 0 posts
0 subscribers
Be the first to start a discussion here.
Be the first to start a discussion here.
Strong ground motion
Strong ground motion
from Wikipedia
ShakeMap for the 2001 Nisqually earthquake

In seismology, strong ground motion is the strong earthquake shaking that occurs close to (less than about 50 km from) a causative fault. The strength of the shaking involved in strong ground motion usually overwhelms a seismometer, forcing the use of accelerographs (or strong ground motion accelerometers) for recording. The science of strong ground motion also deals with the variations of fault rupture, both in total displacement, energy released, and rupture velocity.

As seismic instruments (and accelerometers in particular) become more common, it becomes necessary to correlate expected damage with instrument-readings. The old Modified Mercalli intensity scale (MM), a relic of the pre-instrument days, remains useful in the sense that each intensity-level provides an observable difference in seismic damage.

After many years of trying every possible manipulation of accelerometer-time histories, it turns out that the extremely simple peak ground velocity (PGV) provides the best correlation with damage.[1][2] PGV merely expresses the peak of the first integration of the acceleration record. Accepted formulae now link PGV with MM Intensity. Note that the effect of soft soils gets built into the process, since one can expect that these foundation conditions will amplify the PGV significantly.

"ShakeMaps" are produced by the United States Geological Survey, provide almost-real-time information about significant earthquake events, and can assist disaster-relief teams and other agencies.[3]

Correlation with the Mercalli scale

[edit]

The United States Geological Survey created the Instrumental Intensity scale, which maps peak ground velocity on an intensity scale comparable to the felt Mercalli scale. Seismologists all across the world use these values to construct ShakeMaps.

Instrumental
Intensity
Velocity
(cm/s)
Perceived shaking Potential damage
I < 0.0215 Not felt None
II–III 0.135 – 1.41 Weak None
IV 1.41 – 4.65 Light None
V 4.65 – 9.64 Moderate Very light
VI 9.64 – 20 Strong Light
VII 20 – 41.4 Very strong Moderate
VIII 41.4 – 85.8 Severe Moderate to heavy
IX 85.8 – 178 Violent Heavy
X+ > 178 Extreme Very heavy

Notable earthquakes

[edit]
PGV
(max recorded)
Mag Depth Fatalities Earthquake
318 cm/s[4] 7.7 33 km 2,415 1999 Jiji earthquake
215 cm/s[5] 7.8 10 km 62,013 2023 Turkey-Syria Earthquakes
183 cm/s[6] 6.7 18.2 km 57 1994 Northridge earthquake
170 cm/s[4] 6.9 17.6 km 6,434 1995 Great Hanshin earthquake
152 cm/s[4] 6.6 10 km 11 2007 Chūetsu offshore earthquake
147 cm/s[4] 7.3 1.09 km 3 1992 Landers earthquake
145 cm/s[4] 6.6 13 km 68 2004 Chūetsu earthquake
138 cm/s[4] 7.2 10.5 km 356 injured 1992 Cape Mendocino earthquakes
117.41 cm/s 9.1[7] 29 km 19,747 2011 Tohoku earthquake and tsunami
108 cm/s[8] 7.8 8.2 km 8,857 April 2015 Nepal earthquake
38 cm/s[9] 5.5 15.5 km 0 2008 Chino Hills earthquake
20 cm/s (est)[10] 6.4 10 km 115-120 1933 Long Beach earthquake

See also

[edit]

References

[edit]
Revisions and contributorsEdit on WikipediaRead on Wikipedia
from Grokipedia
Strong ground motion refers to the intense shaking of the Earth's surface caused by seismic waves from earthquakes, particularly near the fault rupture where accelerations can exceed those perceptible to humans and cause significant structural damage. This phenomenon is primarily associated with moderate to large earthquakes (typically magnitude 5 or greater) and is distinguished from weaker motions by its potential to generate forces capable of toppling buildings, triggering landslides, and inducing . The measurement of strong ground motion relies on specialized instruments known as strong-motion seismometers or accelerographs, which record accelerations up to several times the acceleration due to gravity (g ≈ 9.8 m/s²), unlike broadband seismometers designed for weaker signals. Key parameters include , which quantifies the maximum rate of change in velocity and correlates with damage potential; peak ground velocity (PGV), indicating the overall energy of shaking; frequency content, which determines how vibrations interact with structures of varying natural periods; and duration, the length of time strong shaking persists, often defined using the integral of squared acceleration exceeding a threshold. These metrics are influenced by factors such as magnitude, source-to-site distance, fault rupture directivity (where shaking intensifies in the direction of rupture propagation), and local site conditions like and basin geometry. Strong ground motion is central to and , providing data for probabilistic maps, ground motion prediction equations (GMPEs), and the design of resilient infrastructure. Organizations like the U.S. Geological Survey (USGS) maintain networks such as the National Strong Motion Project, which operates over 660 stations to collect for events worldwide, informing tools like ShakeMap for rapid damage assessment. Historical records, including those from the (M6.7), demonstrate how near-fault effects amplify motions, leading to advancements in building codes that incorporate site-specific hazard levels with a defined probability of exceedance, such as a 2% chance in 50 years. Ongoing research focuses on modeling and empirical predictions to estimate motions from future events, emphasizing the role of source heterogeneities in controlling amplitude and variability.

Fundamentals

Definition

Strong ground motion refers to the intense shaking experienced near the source of an earthquake, characterized by high amplitudes of ground acceleration, velocity, or displacement that can cause damage to structures and infrastructure. Specifically, it encompasses motions where parameters such as peak ground acceleration (PGA) exceed thresholds like 0.1g (where g is the acceleration due to gravity), marking the approximate lower limit for motions relevant to engineering design and potential structural impacts. These motions are typically defined by their capacity to produce significant forces on buildings, with higher thresholds such as PGA > 0.2g often classifying the shaking as particularly strong in engineering standards. The term "strong ground motion" emerged in the early following the and the 1929 World Engineering Congress, which highlighted the need for recording intense near-source shaking. This led to the design of the first U.S. strong-motion accelerographs by the National Bureau of Standards in 1931 (based on the Wood-Anderson ), with installations managed by the U.S. Coast and Geodetic Survey in the early , capturing records from events like the . This period marked the shift from traditional , which saturated during large events, to devices designed for high-amplitude recordings. In contrast to weaker seismic waves that attenuate over distance and are recorded globally by sensitive instruments, strong ground motion emphasizes near-field effects—typically within about 50 km of the fault—where high-amplitude shaking dominates due to direct rupture propagation and site amplification. These motions correlate with higher levels on intensity scales, such as Modified Mercalli Intensity VI or greater, where damage becomes evident.

Characteristics

Strong ground motion is characterized by several key parameters that quantify its intensity and impact. (PGA) measures the maximum acceleration experienced at the ground surface, typically ranging from 0.1g to 1.0g during strong shaking, though extreme events can exceed 2g in the horizontal direction. Peak ground velocity (PGV) represents the maximum ground , generally between 0.5 cm/s and 200 cm/s, with higher values near the fault. Peak ground displacement (PGD) indicates the maximum ground displacement, often 0.1 cm to 100 cm, reflecting longer-period motions that can cause significant structural deformation. These parameters are derived from accelerograms and highlight the rapid, intense nature of shaking in the near-source region. The frequency content of strong ground motion primarily spans 0.1 Hz to 30 Hz, encompassing a broad spectrum that excites structures across various natural periods. Within this range, low frequencies (below 1 Hz) dominate long-period responses, while higher frequencies (up to 30 Hz) contribute to short-period accelerations. Near-fault effects, such as forward directivity, introduce pulse-like motions with concentrated energy in the 0.5–10 Hz band, amplifying velocities and displacements perpendicular to the rupture propagation. Duration assesses the persistence of strong shaking, often defined as the significant duration between 5% and 95% (or 75%) of the Arias intensity, which integrates the squared acceleration over time to quantify cumulative energy (typically 1–2000 cm/s). This duration, ranging from 1 s to 50 s, influences fatigue in structures, with longer durations (e.g., 10–50 s for large events) increasing damage potential by prolonging energy input. Site effects significantly modify strong ground motion through local soil conditions, with soft soils amplifying amplitudes by factors of 2–5 compared to rock sites, particularly at site-specific resonant frequencies. This amplification arises from impedance contrasts and wave trapping in sedimentary basins, exacerbating motions in areas like alluvial plains or soft clay deposits. Variability in strong ground motion is influenced by fault type and hypocentral distance, leading to asymmetric shaking patterns. Strike-slip faults often produce more directional pulses due to , while thrust faults generate hanging-wall effects that intensify near-surface motions. Hypocentral distance further modulates this variability, with intraevent standard deviations increasing up to 20–35 km before stabilizing, as and effects dominate farther from the source.

Measurement

Instruments

Strong ground motion is primarily recorded using accelerographs and strong-motion seismometers, which are designed to capture high-amplitude accelerations during earthquakes that exceed the capabilities of standard seismometers. Accelerographs measure ground acceleration directly, while strong-motion seismometers often employ force-balance accelerometers to achieve high fidelity in recording. These instruments typically feature a dynamic range exceeding 111 dB (equivalent to full-scale accelerations of ±2 g or more with micro-g resolution) and a flat frequency response from 0.02 to 50 Hz, enabling accurate capture of both low- and high-frequency components of shaking. The development of these instruments began in the early 20th century with analog devices. In the 1930s, the first strong-motion seismographs, such as mechanical accelerographs, were introduced to record peak accelerations during damaging earthquakes, with pioneers like Kyoji Suyehiro in Japan and John Freeman in the United States advocating for their use following the 1923 Tokyo earthquake. These early analog systems used film or paper records and had limited dynamic range, often clipping at accelerations above 0.2 g. The transition to digital recording occurred in the late 1970s, with the introduction of digital accelerographs that offered improved resolution and broader bandwidth, revolutionizing data quality and enabling real-time processing. By the 1980s and 1990s, broadband digital sensors became standard, incorporating force-balance feedback mechanisms for linear response across a wide amplitude range. Key networks have been instrumental in deploying these instruments globally. The U.S. Geological Survey's National Strong-Motion Program (NSMP), established in 1931 under the Coast and Geodetic Survey, pioneered systematic recording in the United States, initially focusing on and expanding to over 700 stations by the . In , the K-NET (Kyoshin Network) and KiK-net (Kiban Kyoshin Network) were launched in the late 1990s by the National Research Institute for Earth Science and Disaster Resilience following the 1995 ; K-NET comprises about 1,000 surface stations for free-field measurements, while KiK-net includes 700 borehole pairs for site response studies. The Strong-Motion Database (ESM), developed through EU-funded projects starting in the late 1990s and formalized in its current form by the Istituto Nazionale di Geofisica e Vulcanologia around 2010, aggregates data from national networks across and the Mediterranean, supporting over 10,000 records from events since the 1930s. Deployment strategies prioritize high-risk seismic zones to maximize data utility for engineering and hazard assessment. Instruments are sited in free-field locations near faults, as well as on structures like buildings, bridges, and dams to evaluate site-specific amplification and structural response. Triggering mechanisms are set to activate recording at low acceleration thresholds, typically above 0.01 g, to capture moderate events while minimizing false triggers from non-seismic noise; modern digital systems often use continuous recording to eliminate triggering biases altogether. installations, as in KiK-net, provide baseline data unaffected by surface soils. Calibration ensures instrument reliability, with standards requiring traceability to national institutes. The (ISO) 16063 series, particularly Part 21 for comparison methods using reference transducers, guides calibration procedures to achieve accuracy within 5% and phase accuracy within 5 degrees over the 0.1–100 Hz range. In the United States, calibrations follow NIST-traceable protocols, while specific strong-motion guidelines emphasize periodic field verification to maintain performance during deployment.

Data Processing

Raw strong ground motion data, typically recorded as time series from seismometers or accelerographs, undergo a series of steps to correct for and environmental artifacts, ensuring the resulting datasets are reliable for engineering analysis and assessment. These steps transform noisy, uncalibrated recordings into corrected , , and displacement traces, as well as derived quantities like response spectra, while preserving the physical characteristics of the ground motion. Baseline correction is a fundamental initial step to remove low-frequency drifts in records caused by tilt, rotational effects, or electronic offsets during an . Common techniques include fitting, where a low-order (typically second- or third-degree) is least-squares fitted to the pre-event and post-event portions of the record to estimate and subtract the baseline trend, thereby minimizing artificial and displacement offsets. This method is widely adopted because it effectively handles inconsistent initial velocities and accelerations without introducing high-frequency artifacts, as demonstrated in applications to signals from seismic events. Filtering follows baseline correction to attenuate outside the band of interest while retaining the signal's dynamic content. Bandpass filters, such as fourth-order Butterworth filters with passbands from 0.05 to 50 Hz, are routinely applied to eliminate low-frequency instrumental (e.g., from tilt) and high-frequency electronic or site-generated , which can dominate in strong motion records. Care must be taken to avoid over-filtering, as aggressive high-frequency cutoffs above 20-25 Hz may distort peak accelerations and spectral amplitudes critical for engineering design, particularly in near-fault recordings where high-frequency content exceeds 30 Hz. Once is corrected and filtered, double integration yields and displacement , but this process amplifies baseline errors, leading to spurious long-period trends. To mitigate these, integration is often performed with concurrent baseline correction, such as iterative adjustment of the record to ensure zero net displacement over the event duration, or by incorporating instrument response simulations like those of the Wood-Anderson seismograph to validate the recovered displacements against expected low-frequency behavior. This approach has been validated in processing historical strong motion data, where uncorrected integrations can overestimate permanent displacements by factors of 2-5. Response spectra computation derives engineering-relevant parameters from the processed time series, quantifying the ground motion's potential to excite structures at various periods. Pseudo-acceleration spectra, which approximate the maximum acceleration of a single-degree-of-freedom oscillator, are calculated for a standard 5% critical damping ratio, as this value balances realism with computational efficiency for most civil structures and is enshrined in seismic design codes worldwide. The spectra are typically computed over periods from 0.01 to 10 seconds using numerical integration of the equation of motion, providing peak values that inform building code spectra and performance-based design. Quality control throughout processing ensures , with key metrics including (SNR) thresholds exceeding 3:1 in the primary frequency band to confirm the signal dominates over , particularly for low-amplitude records. Additionally, checks for clipping—where amplitudes saturate the instrument's —are performed by inspecting for flattened peaks in the or spectral irregularities, often using automated algorithms to flag and exclude affected portions, as clipped data can underestimate peak ground accelerations by up to 20-50%. These metrics, recommended in standard processing guidelines, help maintain dataset usability for hazard modeling.

Modeling and Prediction

Ground Motion Prediction Equations

Ground motion prediction equations (GMPEs), also known as attenuation relations, are empirical or semi-empirical models that estimate the intensity of strong ground motion, such as (PGA) or spectral acceleration, as a function of source parameters, propagation path, and site conditions. These equations are derived from regression analyses of recorded strong-motion data and are essential for assessment and engineering design. The general form of a GMPE is typically expressed in logarithmic space to account for the wide variability in ground motion amplitudes: log10Y=f(M,R,S)+ϵ\log_{10} Y = f(M, R, \mathbf{S}) + \epsilon where YY is the ground motion intensity measure (e.g., PGA), MM is the moment magnitude, RR represents source-to-site distance metrics (e.g., rupture distance RrupR_{rup} or Joyner-Boore distance RJBR_{JB}), S\mathbf{S} denotes site parameters (e.g., shear-wave velocity in the upper 30 m, VS30V_{S30}), and ϵ\epsilon captures aleatory variability, often assumed to be normally distributed with zero mean and standard deviation σ\sigma. One of the seminal GMPEs is the Boore-Joyner-Fumal (BJF) model of 1997 using strong-motion data from California earthquakes, which provided an early framework for predicting horizontal PGA and velocity on rock sites. The BJF equation takes the form logy=α+βMlogr+br\log y = \alpha + \beta M - \log r + b r, where yy is the ground motion parameter, r=d2+h2r = \sqrt{d^2 + h^2}
Add your contribution
Related Hubs
User Avatar
No comments yet.