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Analysis and comparison of Fourier and Wavelet transforms: application to the study of seismic source parameters of the 2001 Arequipa Earthquake
Análisis y comparación de las transformadas de Fourier y Wavelet: aplicación para el estudio de parámetros de la fuente sísmica del Terremoto de Arequipa del 2001
DOI:
https://doi.org/10.15446/rbct.n58.118962Palabras clave:
Fourier Transform (FFT), Wavelet Transform (WT), radiated energy, source parameters, Arequipa earthquake (en)Transformada de Fourier (FFT), Transformada Wavelet (WT), energía radiada, parámetros fuente, terremoto de Arequipa (es)
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This study focuses on the characterization of the June 23, 2001, Arequipa earthquake by applying the Fourier Transform (FFT) and Wavelet Transform (WT) together to estimate source parameters and radiated energy, aiming to improve seismic risk management in southern Peru. FFT results showed seismic moments ranging from 3.55×10¹⁶ to 1.41×10¹⁸ N·m, stress drops between 0.46 and 3.99 MPa, and fracture radii from 0.61 to 1.94 km. WT enabled the estimation of dominant frequencies between 0.18–0.24 Hz, radiated energy ranging from 24.52 to 32.19 J, and rupture durations from 40.02 to 105.98 s. The combined use of FFT and WT allowed for a more detailed characterization of the 2001 Arequipa earthquake. FFT proved effective for spectral analysis of source parameters, while WT provided accurate estimates of radiated energy and rupture duration—key factors for enhancing seismic risk assessment in the region.
Este estudio se centra en la caracterización del terremoto de Arequipa del 23 de junio de 2001, aplicando conjuntamente la Transformada de Fourier (FFT) y la Transformada Wavelet (WT) para estimar los parámetros de fuente y la energía radiada, con el objetivo de mejorar la gestión del riesgo sísmico en el sur de Perú. Los resultados de FFT mostraron momentos sísmicos entre 3.55×10¹⁶ y 1.41×10¹⁸ N·m, caídas de estrés entre 0.46 y 3.99 MPa, y radios de fractura de 0.61 a 1.94 km. La WT permitió estimar frecuencias dominantes entre 0.18–0.24 Hz, energía radiada entre 24.52 y 32.19 J, y duraciones de ruptura entre 40.02 y 105.98 s. El uso combinado de FFT y WT permitió una caracterización más detallada del terremoto de 2001. La FFT resultó eficaz para el análisis espectral de los parámetros de fuente, mientras que la WT proporcionó estimaciones precisas de la energía radiada y la duración de la ruptura, factores clave para mejorar la evaluación del riesgo sísmico en la región.
Recibido: 20 de febrero de 2025; Revisión recibida: 31 de julio de 2025; Aceptado: 1 de agosto de 2025
Abstract
This study focuses on the characterization of the June 23, 2001, Arequipa earthquake by applying the Fourier Transform (FFT) and Wavelet Transform (WT) together to estimate source parameters and radiated energy, aiming to improve seismic risk management in southern Peru. FFT results showed seismic moments ranging from 3.55×10¹⁶ to 1.41×10¹⁸ N·m, stress drops between 0.46 and 3.99 MPa, and fracture radii from 0.61 to 1.94 km. WT enabled the estimation of dominant frequencies between 0.18-0.24 Hz, radiated energy ranging from 24.52 to 32.19 J, and rupture durations from 40.02 to 105.98 s. The combined use of FFT and WT allowed for a more detailed characterization of the 2001 Arequipa earthquake. FFT proved effective for spectral analysis of source parameters, while WT provided accurate estimates of radiated energy and rupture duration-key factors for enhancing seismic risk assessment in the region.
Keywords:
Fourier Transform (FFT), Wavelet Transform (WT), radiated energy, source parameters, Arequipa earthquake.Resumen
Este estudio se centra en la caracterización del terremoto de Arequipa del 23 de junio de 2001, aplicando conjuntamente la Transformada de Fourier (FFT) y la Transformada Wavelet (WT) para estimar los parámetros de fuente y la energía radiada, con el objetivo de mejorar la gestión del riesgo sísmico en el sur de Perú. Los resultados de FFT mostraron momentos sísmicos entre 3.55×10¹⁶ y 1.41×10¹⁸ N·m, caídas de estrés entre 0.46 y 3.99 MPa, y radios de fractura de 0.61 a 1.94 km. La WT permitió estimar frecuencias dominantes entre 0.18-0.24 Hz, energía radiada entre 24.52 y 32.19 J, y duraciones de ruptura entre 40.02 y 105.98 s. El uso combinado de FFT y WT permitió una caracterización más detallada del terremoto de 2001. La FFT resultó eficaz para el análisis espectral de los parámetros de fuente, mientras que la WT proporcionó estimaciones precisas de la energía radiada y la duración de la ruptura, factores clave para mejorar la evaluación del riesgo sísmico en la región.
Palabras clave:
Transformada de Fourier (FFT), Transformada Wavelet (WT), energía radiada, parámetros fuente, terremoto de Arequipa.1. Introduction
The characterization of seismic signals using spectral and time-frequency analysis techniques is essential for understanding earthquake rupture dynamics and improving early warning and hazard mitigation models. Due to their inherently non-stationary nature, seismic signals pose significant challenges to classical techniques such as the Fourier Transform (FT), which, although effective in identifying dominant frequencies, loses information about the temporal evolution of the spectral content [1]
As an alternative, the Wavelet Transform (WT)-in both its continuous and discrete forms-offers a multiresolution representation in the time-frequency domain, enabling the analysis of signals with dynamic variations and abrupt transitions [2]. Its application has proven effective in studies such as the 2015 Kathmandu Valley earthquake, where the temporal distribution of seismic energy was evaluated [3], and in regional-scale source parameter estimation [4].
In various regions worldwide, FT has been employed to estimate seismic source parameters such as seismic moment, corner frequency, and radiated energy. For example, in Cuba [5], South Africa [6], and Colombia [7], these methods have contributed to regional seismic characterization. In California, [8] used WT and the Brune model to evaluate energy release across events of varying magnitude, while [9] established empirical relationships between seismic moment and stress drop that remain foundational in modern seismology.
In the Peruvian context, [10] applied FT and the Brune model to the aftershocks of the 2001 Arequipa earthquake, revealing patterns of rupture and energy release. Similarly, [11] used FT to estimate source parameters from the aftershocks of the 2018 Lomas earthquake (Mw 7.1), assessing interactions between the mainshock and its aftershocks.
Despite these advances, an important gap remains: integrated approaches that combine spectral (FT) and time-frequency (WT) techniques are still scarce, particularly for complex events such as the 2001 Arequipa earthquake. This earthquake, with a magnitude of Mw 8.4, prolonged duration, multiple moment release pulses, and unilateral rupture propagation, represents an ideal case for applying and comparing both techniques jointly.
This study proposes the simultaneous application of FT and WT to seismic records from the 2001 Arequipa earthquake and its ten main aftershocks, to estimate source parameters such as seismic moment, stress drop, fracture radius, and radiated energy. By comparing the results from both transforms, the study seeks to demonstrate how the integration of these approaches enables a more complete and dynamic characterization of the seismic source, thereby enhancing seismic hazard assessment capabilities in southern Peru.
1.1. Study area
The study area is located in southern Peru, spanning from 15.6° to 18.2° south latitude, and from 68.7° to 76.2° west longitude. This region was affected by the 2001 earthquake, which had 134 aftershocks distributed southeastward, suggesting that the rupture propagated in that direction [12]. Fig. 1 illustrates the location of the study area and the distribution of aftershocks according to their magnitude. Blue circles correspond to aftershocks with Mw between 5 and 5.5, green circles from 5.5 to 6.5, and red circles from 6.5 to 7.5.
Figure 1: Geographic distribution of the study area, 2001 Arequipa earthquake epicenter, and spatial pattern of aftershocks by magnitude
The main Arequipa 2001 earthquake is represented by a yellow star, while the rupture zone is marked with a green rectangle.
The 2001 earthquake in southern Peru caused numerous fatalities and severe damage in Tacna, Arequipa, Ayacucho, and Moquegua, as well as in Arica and Iquique (Chile), with an intensity of VII-VIII on the Modified Mercalli scale [13]. The aftershock analysis identified a rupture area of 370 x 150 km², with propagation towards the southeast [14]. More than 80 localities were affected, with 217,400 people impacted and 17,580 houses destroyed [15]. Key seismic source parameters were determined through advanced studies, as reflected in Table 1, while Fig. 2 illustrates its focal mechanism and intensities.
Source: Adapted from Tavera, H. and Antayhua, 2022.Table 1: Source and impact parameters of the 2001 Arequipa earthquake (Mw 8.4).
Parameter
Value/Description
Date and time
June 23, 2001, at 15:33 (20:33 UTC)
Magnitude
8.4 Mw (Moment Magnitude Scale)
Epicenter
16.265°S, 73.641°W; 120km southwest
Focal Depth
33 km depth
Tsunami
Camaná, Peru
Duration
Between 60 and 120 seconds
Released Energy
Equivalent to 32 megatons of TNT
Focal Mechanism
Reverse Fault (Thrust Fault)
Strike
Approximately 308°
Dip
Around 20°
Rake
Around 72° (compressional movement)
Figure 2: Focal mechanism and tectonic context of the 2001 Arequipa earthquake (Mw 8.4). The beach ball symbol illustrates a reverse fault mechanism. Red arrows indicate compressive forces from the Nazca Plate subducting beneath the South American Plate at ~6.9 cm/year. The rupture zone, aftershock distribution (colored by magnitude), and Modified Mercalli intensities across southern Peru are also depicted, highlighting the regional seismic impact.
2. Theoretical framework
2.1. Fourier Transform (FFT)
The FFT is essential in seismology for analyzing seismic signals, decomposing them into their frequency components, and facilitating the interpretation of seismic phenomena [9]. The Fourier Series allows the representation of any periodic function as an infinite sum of sine and cosine functions at different frequencies. The coefficients aₖ and bₖ indicate the contribution of each frequency in the function [17].
The Short-Time Fourier Transform (STFT) is essential for analyzing non-stationary signals, as it segments the signal into time windows to track changes in its frequency content [1]. The STFT enables a time-frequency analysis, where each window reveals the spectral distribution at that moment [18]. The result is a time-frequency graph, where the horizontal axis represents time and the vertical axis represents frequency, showing how frequencies evolve (Fig. 3).
Figure 3: Schematic representation of the STFT for time-frequency analysis of seismic signals
2.2. Wavelet Transform (WT)
Unlike Fourier, the WT uses a mother wavelet, an oscillatory function localized in time and frequency, allowing the decomposition of signals into scaled and translated components [17]. This method enables concurrent analysis in both time and frequency domains, facilitating the identification of trends and oscillations [19]. CWT spectra, amplitudes are represented through a chromatic scale where warm colors (reds/oranges) indicate higher energy magnitudes, while cool colors (blues/greens) correspond to lower amplitudes [2]. Eq. (2) defines a scaled and translated wavelet used in the Continuous Wavelet Transform (CWT) [20].
Fig. 4 shows the process of the WT, a technique for analyzing signals in the time and scale domains [21]. The input signal represents a vibration that varies over time [22]. During the Wavelet Transform process, the signal is decomposed into different scales to identify its frequency content over time [23]. The analysis reveals that large scales correspond to low frequencies, while small scales capture high frequencies, enabling more detailed resolution than the Fourier Transform [2]. In Table 2, a comparison of FFT and WT in terms of seismology is presented.
Figure 4: Conceptual diagram of the WT for multiscale time-frequency analysis of seismic signals
Source: Adapted from Bessissi et al., 2009.Table 2: Analysis and Comparison of Fourier Transform and Wavelet Transform - Seismology
Characteristic
Fourier Transform (FFT)
Wavelet Transform (WT)
Domain
Frequency
Time-Frequency
Transient Signal Analysis
Not suitable for transient signal analysis
Suitable for transient signal analysis
Temporal Resolution
Poor
Good temporal resolution
Frequency Resolution
High frequency resolution
Variable frequency resolution
High applicability in seismic signal analysis
Good for periodic or stationary signals
Ideal for non-stationary seismic signals, such as earthquakes and transient events
Fixed vs Variable Window
Fixed Window vs Variable Window
Use a variable window, shorter for high frequencies and longer for low frequencies.
Ability to detect local events.
It is not effective in detecting seismic events.
Very effective for detecting local events, such as earthquakes or seismic ruptures.
Computational Complexity
Less computationally expensive.
More computationally expensive.
Use in frequency identification
Good for identifying dominant frequencies throughout the signal.
Can identify frequencies that vary over time, useful for non-constant seismic events.
Common Applications in Seismology
Detection of fundamental frequency of seismic signals
Earthquake analysis and non-stationary signals. Identification of seismic phases.
3. Data and methodology
3.1. Database download
The data were obtained from the IRIS seismic network, specifically from the Ñaña station (NNA), located at latitude -11.988° and longitude -76.842°, selected for its proximity to the earthquake epicenter.
Fig. 5 shows the flowchart of the process followed in this research. The diagram outlines a detailed and structured approach to analyzing seismic signals using two complementary techniques: FFT and WT. The results from both methods were used to determine fundamental parameters about the seismic source, allowing for a better understanding of the nature of earthquakes and their aftershocks. Once the data (10 aftershocks) were downloaded, two main programs were used to process the data.
Figure 5: Flowchart of the methodological framework for seismic signal analysis using FFT and WT
The aftershock data were selected between June 23 and July 1, 2001, with magnitudes ranging from 5 to 10, and depths from 0 to 75 km. The selection of aftershocks was guided by the need to ensure waveform quality and consistency in depth and magnitude for reliable waveform analysis. Events with magnitudes ≥5.0 and depths ≤75 km were chosen to maintain a homogeneous dataset suitable for spectral and time-frequency analysis. This threshold also ensures that selected events generate records with a sufficient signal-to-noise ratio, essential for accurate estimation of source parameters. Although other events of lower magnitude exist, they were excluded due to limitations in data quality or lack of clear waveform characteristics. Table 3 shows the database of the 10 aftershocks, with their main characteristics (Date, time, latitude, longitude, depth, magnitude type, and location).
Source: The authorsTable 3: Seismological parameters of the 2001 Arequipa earthquake and its ten selected aftershocks
Item
Date
Time
Latitude
Longitude
Depth
Mag.
Mag
Location
Earthquake
23/06/2001
20:33:09
-16.303
-73.561
33.0
8.4
Mw
Coast of Peru
Aftershocks 1
23/06/2001
21:27:35
-17.181
-72.642
33.0
6.1
Mw
Coast of Peru
Aftershocks 2
23/06/2001
23:09:57
-16.657
-73.525
10.0
5.9
Mw
Coast of Peru
Aftershocks 3
25/06/2001
3:48:58
-16.044
-74.755
33.0
5.3
Mw
Coast of Peru
Aftershocks 4
25/06/2001
6:38:48
-16.875
-73.772
38.0
5.7
Mw
Coast of Peru
Aftershocks 5
26/06/2001
4:18:32
-17.831
-71.63
33.0
6.7
Mw
Coast of Peru
Aftershocks 6
26/06/2001
8:47:09
-16.624
-74.168
33.0
5.4
Mw
Coast of Peru
Aftershocks 7
27/06/2001
0:21:06
-17.903
-71.480
33.0
5.4
Mw
Coast of Peru
Aftershocks 8
28/06/2001
21:35:24
-17.588
-72.463
33.0
5.3
Mw
Coast of Peru
Aftershocks 9
30/06/2001
8:57:19
-17.707
-72.093
33.0
5.3
Mw
Coast of Peru
Aftershocks 10
01/07/2001
11:06:30
-17.186
-72.984
33.0
5.4
Mw
Coast of Peru
3.2. Determination of seismic source parameters with FFT
The Seismic Analysis Code (SAC) software is a widely used tool in seismology for the management and analysis of seismic data in time series [25]. It allows the application of FFT to calculate the spectrum of a signal and uses high-pass, low-pass, and band-pass filters to remove noise and enhance seismic detection [26].
SAC is essential for determining seismic source parameters such as 𝑀o, source radius, corner frequency 𝑓𝑐, and stress drop (Δ𝜎), allowing the analysis of fault dynamics and potential damage.
For seismic signal processing, high-pass, low-pass, and band-pass filters were applied using SAC software to eliminate noise and enhance spectral detection. Signals were corrected to physical units suitable for calculating parameters such as Mo and Δ𝜎. In the Wavelet analysis, signals were bandpass filtered between 2 and 4 Hz, amplitudes were squared, absolute values were taken, then smoothed, and normalized to unity.
The 𝑓𝑐 is related to the rupture size and earthquake duration, being lower in high-magnitude events and higher in smaller ones [27]. The flat part of the spectrum (Ω₀) is found at low frequencies, where the amplitude is constant, indicating a uniform distribution of energy [28] (Fig. 6).
Figure 6: Fourier spectrum, calculating the corner frequency 𝑓𝑐 and the flat part Ω₀, of the 2001 Arequipa earthquake.
3.2.1. Calculation of seismic moment (Mo)
The Mo was calculated using the flat part of the displacement spectrum (Ωo), following the classical formulation proposed by [28. This equation relates the observed spectral amplitude to source parameters, accounting for density, wave velocity, epicentral distance, and radiation pattern, as expressed in Eq. (3):
Ω0 = Flat part, calculated from the spectrum
Mo = Seismic moment.
ρ = Density of the medium; 2.8 gr/cm3
R = Epicentral distance
= P-wave velocity; 5 Km/seg
ψ0 = Radiation pattern, assumed as 0.4 based on a double-couple source model with isotropic take-off angle distribution [28] (Brune, 1970).
3.2.2. Calculation of the fracture radius
The fracture radius is a crucial parameter that defines the spatial extent of the rupture zone during an earthquake. Its estimation helps improve understanding of the fault's geometry and the energy release scale. Based on the fc obtained from spectral analysis, the fracture radius (Eq. 4) can be calculated using standard formulations derived from source theory models.
α = represents the speed of the P-wave
3.2.3. Calculation of stress drop (Δσ)
Stress drop indicates the difference in shear stress on a fault before and after rupture and is directly linked to the energy released during an earthquake. It is a key parameter for understanding rupture behavior and seismic efficiency. Using the previously estimated Mo and fracture radius, Δσ (Eq. 5) can be calculated using classical source scaling relationships.
3.3. Determination of seismic source parameters with WT
MATLAB is a key tool in technical scientific programming, enabling seismic signal analysis through digital processing, including the interpretation of phases, amplitude, and polarity [29]. Additionally, it facilitates the use of the Continuous Wavelet Transform (CWT) to represent non-stationary signals in the time-frequency domain [30].
The use of MATLAB and the Wavelet Transform allows for the analysis of non-stationary seismic signals, decomposing them into different frequency and time scales to characterize the dynamics of the seismic source [31]. The seismic signal shows energy variations over time, with higher energy at low frequencies (surface waves) in the first minutes, which decreases over time. In Fig. 7, high scales correspond to low frequencies, associated with surface waves, while low scales represent high frequencies of P or S waves. High intensity peaks indicate energy release, and the decrease towards the end reflects the reduction in seismic activity.
Figure 7: 3D wavelet spectrogram CWT of the 2001 Arequipa earthquake, generated in MATLAB
3.3.1. Calculation of rupture time
The rupture time was estimated following the methodologies of [32]. The vertical BHZ component was filtered between 2-4 Hz, squared, and normalized to enhance signal clarity. Rupture duration was then measured from the P-wave onset to the point where the amplitude decayed to 20% of its maximum, providing reliable results without the need for instrumental response correction.
The seismic record used for this analysis corresponds to a vertical BHZ component, with a velocity equivalent to that of a broadband station, allowing for a detailed study of the waveforms [33] (Fig.8a). To enhance the clarity of the signal, a bandpass filter is applied to the record, restricting frequencies to a range of 2 to 4 Hz, which effectively isolates the relevant seismic frequencies while minimizing noise interference (Fig. 8b).
Figure 8: (a) Vertical component seismic signal of the Arequipa Earthquake of 2001, (b) Normalized seismic signal (P-wave), (c) Calculation of rupture duration, (d) Calculation of maximum radiated energy MaxEa (J)
Once the filtered signal is obtained, its amplitude values are squared, making them proportional to the seismic energy radiation. Additionally, to facilitate further processing, the absolute values of the amplitudes are taken, smoothed, and normalized to unity, ensuring a consistent comparison across different signals [34]. This transformation allows a better understanding of the energy distribution and variations within the seismic event.
In terms of signal decay analysis, the duration of the pause is measured from the initial arrival of the P-wave until the amplitude reduces to 20% of its maximum value, providing insights into the dissipation of seismic energy over time. This approach highlights the gradual attenuation of the seismic waves and their energy release patterns [35].
It is also crucial to emphasize that, since the analysis focuses only on the temporal component of the seismic signal, adjusting the instrumental response is not required. This simplifies the workflow while maintaining the integrity of the data, ensuring that the results remain reliable and representative of the actual seismic phenomenon under investigation. Since the analysis relies on the signal’s temporal evolution rather than absolute amplitude, instrumental correction is unnecessary. The waveform shape remains intact, preserving data integrity and ensuring reliable, representative results of the seismic event (Fig. 8c).
3.3.2. Calculation of Maximum Radiated Energy (MaxEa)
The maximum radiated energy (MaxEa) is obtained by summing the amplitudes from the wavelet spectrogram in a specific frequency band (2-4 Hz in this study), following the energy integration method [36]. The temporal distribution of seismic energy, which is crucial for estimating Mo and magnitude, shows a progressive decrease, indicating rapid dissipation of waves in events with high attenuation. The radiated energy can be obtained by calculating the sum of the amplitudes of the WT spectrogram in a specific frequency band (Fig. 8d).
4. Results and discussion
The Fourier spectra were plotted for the 10 aftershocks of the Arequipa earthquake of 2001, determining the flat part (Ω₀) and the 𝑓𝑐, essential for calculating the seismic source parameters. The Wavelet analysis of the 10 aftershocks from the 2001 Arequipa earthquake was carried out using MATLAB, where the methodology was fully implemented.
4.1. Comparison of the parameters of the Arequipa 2001 earthquake and its aftershocks
Table 4 presents the main source parameters: Mo, R, and Δσ estimated using FFT; and Fc, MaxEa, and Tr obtained using WT. These values provide complementary information on the event's size, energy release, and rupture dynamics.
Source: The authors.Table 4: Seismic source parameters and corresponding estimation methods using FFT and WT
Parameter
Unit
Method
Seismic Moment (Mo)
N·m
FFT
Fracture Radius
km
FFT
Stress Drop (Δσ)
MPa
FFT
Frequency Content
Hz
WT
Maximum Radiated Energy (MaxEa)
J
WT
Rupture Duration
s
WT
Table 5 summarizes the seismic source parameters obtained through FFT and WT transforms, comparing the mainshock (Mw 8.4) and its aftershocks (Mw 5.3-6.7), including M₀, fracture radius, stress drop (Δσ), radiated energy (MaxEa), and rupture durations.
Source: The authorsTable 5: Seismic source parameters derived from FFT (M₀, fracture radius, Δσ) and WT (dominant frequency, MaxEa, duration) for the 2001 Arequipa mainshock and aftershocks.
Ítem
FFT
WT
Depth (km)
Mw
Mo (N.m)
Radio (Km)
Δσ (Mpa)
Frec (Hz)
MaxEa (J)
Dur Rupt. (s)
Earthquake
33.0
8.4
1.58×10²¹
3.15
38.08
0.30
40.80
146.12
Aftershock 1
33.0
6.1
3.55×10¹⁷
1.82
2.88
0.18
29.22
95.18
Aftershock 2
10.0
5.9
1.12×10¹⁷
1.71
1.83
0.20
28.27
82.00
Aftershock 3
33.0
5.3
3.55×10¹⁶
0.73
0.57
0.19
24.52
40.02
Aftershock 4
38.0
5.7
8.91×10¹⁶
1.36
1.79
0.24
26.82
70.18
Aftershock 5
33.0
6.7
1.41×10¹⁸
1.94
3.99
0.19
32.19
105.98
Aftershock 6
33.0
5.4
4.47×10¹⁶
1.11
1.48
0.19
25.21
54.21
Aftershock 7
33.0
5.4
4.47×10¹⁶
1.13
1.46
0.18
25.78
59.58
Aftershock 8
33.0
5.3
3.55×10¹⁶
0.61
0.64
0.19
24.69
43.93
Aftershock 9
33.0
5.3
3.55×10¹⁶
0.76
0.46
0.18
24.78
45.08
Aftershock 10
33.0
5.4
4.47×10¹⁶
1.12
1.58
0.19
25.99
50.89
4.2. Seismic Moment (Mo)
Fig. 9 illustrates the seismic moment (Mo) of the main shock and aftershocks using a logarithmic scale on the vertical axis to capture the wide range of values. The main shock, represented in red, exhibits a seismic moment of 1.58 × 10²¹ N·m. This reflects the immense amount of energy released during the primary rupture. In contrast, the aftershocks, shown in blue, have significantly lower moments, ranging from 3.55 × 10¹⁶ N·m to 1.41 × 10¹⁸ N·m. These events mainly contributed to the release of residual stresses and had a much smaller impact on the overall deformation. The use of a logarithmic scale emphasizes the contrast in energy between the main event and the subsequent seismic.
Figure 9: Seismic Moment Values for the Arequipa Earthquake (Main Shock) and its Aftershocks.
4.3. Fracture Radius
Fig. 10 presents the fracture radius (in kilometers) for each seismic event. The main shock, again in red, displays the largest fracture radius-3.15 km-indicating a much greater rupture area compared to the aftershocks, which are shown in green. The aftershocks generally range between 0.6 km and 2 km in radius. This graph clearly highlights the spatial extent of the main rupture compared to the more localized failures of the smaller seismic events. The use of contrasting colors once more helps differentiate the dominant main shock from the supporting seismic sequence.
Figure 10: Fracture Radius for the Arequipa Earthquake (Main Shock) and its Aftershocks
Fig. 11 displays the log-log relationship between Mo (N·m) and fracture radius (r), with lines representing different values of stress drop (Δ𝜎 = 0.1, 1, 10, and 100 MPa). The red star marks the mainshock, located above the 10 MPa line, while the aftershocks cluster near the same line, suggesting similar stress drop magnitudes. This graphical representation follows the scaling law Δ𝜎 ∝ M₀ / r³, allowing for visual interpretation of rupture mechanics.
Figure 11: Log-Log Plot of Seismic Moment vs Fracture Radius with Stress Drop (Δσ) Iso-Lines
4.4. Maximum radiated energy
The main earthquake radiated 40.80 J of energy, while the aftershocks had values ranging from 21.19 J to 26.29 J, according to analysis using the WT.
Fig. 12 shows the relationship between rupture duration (in seconds) and radiated energy in a seismic context, specifically for a Tsunami Generator (TG). The x-axis measures rupture duration, and the y-axis represents radiated energy (blue). Each point in the graph represents a seismic event, differentiated by colors and shapes. The main earthquake is highlighted with a red star, located in the upper left corner, indicating that it had the longest rupture duration and the highest radiated energy. The other points correspond to aftershocks, labeled in the legend as Aftershock 1, Aftershock 2, etc., with different colors and symbols. It is observed that as the rupture duration decreases, the radiated energy also decreases, suggesting a positive correlation between both variables. The aftershocks exhibit lower energy and shorter rupture durations compared to the main event, which is expected in a seismic sequence.
Figure 12: Relationship between rupture duration and radiated energy for the 2001 Arequipa mainshock and its aftershocks
5. Conclusions
This study applied and compared the Fourier Transform (FFT) and the Wavelet Transform (WT) to analyze the seismic source parameters of the 2001 Arequipa earthquake and ten aftershocks, using SAC and MATLAB. The combined use of both methods enabled a comprehensive characterization of the mainshock and its associated events.
The main earthquake (Mw 8.4) exhibited a seismic moment (Mo) of 1.58×10²¹ Nm, significantly higher than the aftershocks, which ranged from 1.12×10¹⁷ to 1.41×10¹⁸ N·m, confirming that the mainshock accounted for the majority of energy release along the fault.
The fracture radius for the mainshock was 3.15 km. In comparison, aftershock values ranged from 0.61 km to 1.94 km, indicating that the main rupture encompassed a substantially larger fault area, which triggered the subsequent events.
Stress drop (Δσ) for the main event reached 38.08 MPa, compared to 0.46-3.99 MPa for aftershocks, showing a direct correlation with Mo and supporting rupture mechanics scaling laws.
Radiated energy (MaxEa), estimated through WT, was 40.80 J for the mainshock and between 24.52 J and 32.19 J for aftershocks, highlighting the main event’s dominance in energy dissipation across the seismic sequence.
Rupture duration was 146.12 s for the mainshock, versus 40.02-105.98 s for aftershocks, reflecting its greater magnitude and destructive potential.
FFT proved effective in extracting spectral parameters such as Mo, Δσ, and corner frequency, while WT enabled detailed time-frequency analysis, particularly for radiated energy and rupture duration.
Together, FFT and WT offer a complementary framework for seismic source analysis, improving the understanding of fault dynamics and enhancing regional seismic hazard assessment.
Acknowledgments
The authors would like to thank UNSA INVESTIGA (Project PTTMD-42 2023-UNSA) for funding this research work
References
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