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Geophone
Geophone
from Wikipedia
Geophone (SM-24), frequency band 10 Hz to 240 Hz, standard resistance 375 Ω

A geophone is a device that converts ground movement (velocity) into voltage, which may be recorded at a recording station. The deviation of this measured voltage from the base line is called the seismic response and is analyzed for structure of the Earth.

Etymology

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The term geophone derives from the Greek word "γῆ (ge) " meaning "earth" and "phone" meaning "sound".

Construction

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Geosource Inc. MD-79—8 Hz, 335 Ω geophone

Geophones have historically been passive analog devices and typically comprise a spring-mounted wire coil moving within the field of a case-mounted permanent magnet to generate an electrical signal.[1] Recent designs have been based on microelectromechanical systems (MEMS) technology which generates an electrical response to ground motion through an active feedback circuit to maintain the position of a small piece of silicon.

The response of a coil/magnet geophone is proportional to ground velocity, while MEMS devices usually respond proportional to acceleration. MEMS have a much higher noise level (50 dB velocity higher) than geophones and can only be used in strong motion or active seismic applications.

Frequency response

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The frequency response of a geophone is that of a harmonic oscillator, fully determined by corner frequency (typically around 10 Hz) and damping (typically 0.707). Since the corner frequency is proportional to the inverse square root of the moving mass, geophones with low corner frequencies (< 1 Hz) become impractical. It is possible to lower the corner frequency electronically, at the price of higher noise and cost.

Although waves passing through the Earth have a three-dimensional nature, geophones are normally constrained to respond to single dimension - usually the vertical. However, some applications require the full wave to be used and three-component or 3-C geophones are used. In analog devices, three moving coil elements are mounted in an orthogonal arrangement within a single case.

Distinction from seismometers

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Geophones are similar to seismometers in their design and are also used to register seismic waves. In the past, there were clear differences between geophones and seismometers. Compared to conventional geophones, seismometers are more suitable for detecting extremely small ground movements as they cover a wider frequency band, including the frequency range below their natural frequency, usually from 0.01 to 50 Hz.[2] In conventional geophones, the frequency band is in the range of 1-15 Hz. They are cheaper than seismometers and are therefore more commonly used in arrays for large area detection with better specialised resolution.[2] However, with the development of new technologies, the frequency coverage in compact devices has also increased significantly, so that geophones can cover frequency bands from 0 to 500 Hz and the boundaries between geophones and seismometers are becoming blurred.[2]

Uses

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Man using a geophone
Single End Spread[3] & Split Stread[4]
Source Receivers single fold-3 Fold
Royal Rumble[5]

The majority of geophones are used in reflection seismology to record the energy waves reflected by the subsurface geology. In this case the primary interest is in the vertical motion of the Earth's surface. However, not all the waves are upwards traveling. A strong, horizontally transmitted wave known as ground-roll also generates vertical motion that can obliterate the weaker vertical signals. By using large areal arrays tuned to the wavelength of the ground-roll the dominant noise signals can be attenuated and the weaker data signals reinforced.

Analog geophones are very sensitive devices which can respond to very distant tremors. These small signals can be drowned by larger signals from local sources. It is possible though to recover the small signals caused by large but distant events by correlating signals from several geophones deployed in an array. Signals which are registered only at one or few geophones can be attributed to unwanted, local events and thus discarded. It can be assumed that small signals that register uniformly at all geophones in an array can be attributed to a distant and therefore significant event.

The sensitivity of passive geophones is typically 30 volts per (meter per second), so they are in general not a replacement for broadband seismometers.[clarification needed]

Conversely, some applications of geophones are interested only in very local events. A notable example is in the application of remote ground sensors (RGS) incorporated in unattended ground sensor (UGS) systems. In such an application there is an area of interest which when penetrated a system operator is to be informed, perhaps by an alert which could be accompanied by supporting photographic data.

Geophones were used on the Moon for a number of active and passive experiments as part of the Apollo Lunar Surface Experiments Package.

See also

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References

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Revisions and contributorsEdit on WikipediaRead on Wikipedia
from Grokipedia
A geophone is an electromagnetic designed to detect and record ground motion, particularly seismic waves, by converting mechanical vibrations into proportional electrical signals. It operates on the principle of a suspended inertial —typically a coil or —moving relative to a fixed or coil, inducing a voltage via Faraday's law that corresponds to the of the ground. The core components include a spring-suspended proof , a permanent , and a coil, with the device's determining its sensitivity to vibrations in specific bandwidths, often tuned between 4 and 100 Hz for land-based applications. Geophones originated in the early , with initial developments by French physicists during to detect underground mining and tunneling vibrations through electromagnetic transduction. In the , American inventors like the Petty brothers refined the technology for oil exploration, connecting multiple geophones to galvanometers for seismic reflection surveys that revolutionized geophysical . Modern geophones come in various configurations, including single-component (vertical or horizontal) and multi-component (three-axis) models, often deployed in arrays to capture wave propagation patterns. These sensors are essential in exploration geophysics for mapping subsurface structures in oil and gas surveys, as well as in environmental and contexts like for hydrologic studies and pavement deflection analysis. They also support monitoring and near-surface investigations, such as detection and contamination site assessments, where arrays of geophones measure wave arrival times and amplitudes to infer geological properties. Advancements include integration with for enhanced resolution in passive and active seismic arrays.

History and Development

Invention and Early History

The geophone originated during , when French scientists developed it as a device to detect vibrations from enemy tunneling operations underground. Initially acoustic in nature, it was adapted to electromagnetic principles for more sensitive detection. By 1919, American physicist J. Clarence Karcher had developed and patented the reflection seismograph, incorporating geophones as velocity detectors to capture ground motion from blasts. These devices were designed specifically to aid in locating petroleum reservoirs by recording reflected seismic signals, marking a pivotal advancement in geophysical prospecting over prior manual and techniques. Early mechanical geophones operated on the principle of , where a coil suspended within a moved relative to the ground vibrations, generating voltage proportional to the velocity of seismic waves propagating through the . This design allowed for sensitive detection of particle motion, converting from subsurface reflections into electrical signals for analysis. Geophones found their initial widespread application in amid the 1920s U.S. oil boom, particularly in regions like and , where they superseded rudimentary dynamite-based surveys by providing clearer images of stratigraphic layers and potential traps. This shift enabled more precise targeting of drilling sites, contributing to discoveries such as the 1921 reflection profile that validated the method's efficacy. A significant milestone came in the 1930s with the adoption of geophone arrays by leading oil companies, including , which integrated them into large-scale subsurface mapping operations along the Gulf Coast to delineate salt domes and structures. This commercialization accelerated exploration efficiency, with 's seismic crews achieving notable successes in identifying productive fields. Over subsequent decades, geophones evolved from purely mechanical systems to incorporate electronic enhancements, improving signal and field portability.

Evolution and Modern Advancements

During the and , geophone technology transitioned toward more advanced electronic designs, incorporating improved components that enhanced sensitivity, reduced physical size, and minimized electronic noise while expanding bandwidth for better seismic signal capture. These developments were driven by post-World War II advancements in , allowing for more compact and reliable sensors that could handle larger ground motions without distortion and provide stable over broader frequency ranges. The marked the widespread introduction of three-component (3C) geophones, which enabled the detection of vector motion by recording vertical and two orthogonal horizontal components simultaneously, facilitating the analysis of converted waves (P-to-S) for improved subsurface imaging in seismic exploration. This innovation, building on earlier prototypes, gained prominence through research initiatives like the CREWES Project, which emphasized 3C technology for enhanced wavefield separation and polarization analysis. In the 2000s, the advent of digital geophones and micro-electro-mechanical systems () revolutionized sensor arrays by integrating compact silicon-based accelerometers with onboard , enabling wireless deployments and higher rates up to 500 Hz. These sensors, first commercialized around 2001, offered advantages such as lower noise floors (down to 15 ng/√Hz by mid-decade) and greater (up to 128 dB), supporting large-scale, autonomous arrays for efficient field operations. Post-2020 advancements have focused on integrating for real-time data processing, including noise suppression and signal enhancement directly at the sensor level in digital geophones, alongside capabilities extending to 200 Hz for applications in . For instance, nodal systems with 3C geophones have been deployed for high-resolution urban activity tracking, sampling at 200 Hz to capture subtle anthropogenic vibrations. These enhancements, combined with low-frequency compensation algorithms, extend effective response below 0.2 Hz while maintaining high sensitivity, supporting diverse monitoring tasks like geohazard assessment.

Design and Construction

Core Components

A standard geophone consists of an inertial , typically comprising a coil or weighing 10-20 grams in 10 Hz models, suspended by springs within a waterproof case to detect ground motion through relative displacement. The case, often made of rugged or metal with a of 25-30 mm, encloses the components and protects them from environmental factors while allowing the assembly to move with ground vibrations. The electromagnetic forms the core sensing element, featuring a moving coil in a fixed or a moving relative to a fixed coil, which generates a voltage output proportional to the velocity of ground motion via . Springs, usually delicate types, attach the inertial to the case, providing the restoring that enables in response to seismic waves. Damping is achieved through viscous fluid or electromagnetic means, such as resistance in the coil circuit, to control the inertial mass's oscillations and ensure a critically damped response for accurate velocity measurement. The base includes a spiking mechanism, often steel spikes, for firm ground coupling, with the geophone oriented vertically or horizontally to achieve sensitivity to specific motion directions. These components assemble into a compact unit, where the case integrates the fixed magnet (in moving-coil designs) and springs, while leads connect the coil for signal output. Variations in these elements, such as coil versus magnet as the moving part, adapt the geophone for different frequency responses.

Types and Variations

Geophones are categorized by their orientation to capture specific types, with vertical geophones designed to detect primarily compressional P-waves through vertical ground motion, while horizontal geophones target shear S-waves via lateral displacements. These are frequently integrated into three-component (3C) arrays, combining one vertical and two orthogonal horizontal sensors to record motion in all directions for comprehensive vector analysis. Variations also arise from natural frequency responses tailored to exploration depths, where low-frequency geophones around 4.5 Hz are suited for deep seismic surveys by capturing longer-period waves with reduced high-frequency noise. In contrast, high-frequency models up to 100 Hz excel in shallow surveys, providing sharper resolution for near-surface features through sensitivity to shorter wavelengths. Geophones differ further in signal processing, with analog versions generating a direct voltage output proportional to velocity, whereas digital variants incorporate onboard analog-to-digital conversion to minimize transmission noise and enhance data integrity over long cables. Specialized designs address unique environments, including broadband geophones that extend the response range from 0.1 Hz to 100 Hz for capturing a wider spectrum of seismic signals in varied terrains. Ocean-bottom cable (OBC) geophones are ruggedized for marine deployment, often paired with hydrophones in multicomponent setups laid on the seafloor to record both pressure and particle velocity data. Borehole models, typically triaxial and clamped to well walls, enable downhole measurements in vertical or deviated wells for precise subsurface imaging. Emerging technologies include fiber-optic geophones, which use interferometric sensing for distributed vibration detection immune to , and laser-based variants that operate reliably in high-temperature geothermal environments exceeding 200°C.

Operating Principles

Physical Mechanism

Geophones convert mechanical ground motion into electrical signals primarily through the principle of . In a typical moving-coil , a permanent is fixed to the geophone case, while a coil attached to an inertial mass moves relative to it when the ground vibrates. This relative motion changes the magnetic flux Φ\Phi linking the coil, inducing an electromotive force according to Faraday's law: V=NdΦdt,V = -N \frac{d\Phi}{dt}, where VV is the induced voltage and NN is the number of coil turns. The induced voltage is proportional to the rate of change of flux, which depends on the relative velocity between the coil and . The core of this mechanism relies on the inertial response of the suspended mass. The inertial mass—either the coil or the —is attached to springs and housed within the geophone case, which follows ground motion. Due to , the mass resists and lags behind the case's movement, generating relative displacement and between the coil and magnet. For operating frequencies well above the system's , this relative becomes approximately equal to the ground , enabling the geophone to function as a . The relationship between the output signal and ground motion is captured by the transfer function in the Laplace domain, where the output velocity voutv_{\text{out}} (proportional to the induced voltage) relates to the ground velocity vgroundv_{\text{ground}} as vout=s2s2+2ζωns+ωn2vground,v_{\text{out}} = \frac{s^2}{s^2 + 2\zeta \omega_n s + \omega_n^2} \, v_{\text{ground}}, with ss as the Laplace variable, ζ\zeta the ratio, and ωn\omega_n the natural . This second-order system describes how the relative motion responds to input vibrations. is typically adjusted near critical to flatten the above . The springs play a crucial role by providing the restoring force that opposes the inertial 's displacement, defining the system's dynamics. The natural is given by fn=12πkm,f_n = \frac{1}{2\pi} \sqrt{\frac{k}{m}},
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