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A time-ordered sequence of ancient magnetic pole positions inferred from dated remanent magnetization in a continental block. The apparent motion includes the block's movement relative to the rotation axis and can include true polar wander. Consistent paths after a fixed relative rotation support an interval of shared motion; conventional paleomagnetism does not independently determine absolute longitude.

A geomagnetic reversal changes the large-scale polarity of Earth's intrinsic magnetic field. Crustal remanent magnetization records past reversals. The reversal times are not a regular clock; their occurrence reflects time-dependent dynamo action rather than rigid rotation of a permanent magnet.

An iron oxide, $\alpha \text{-}\mathrm{F}{\mathrm{e}}_2{\mathrm{O}}_3$. It typically has weaker induced magnetic susceptibility than magnetite but can preserve stable remanent magnetization.

The magnetization caused by an applied magnetic field strength. The displayed scalar linear law assumes isotropic susceptibility and neglects magnetic self-interaction; remanent magnetization is an additional component that need not align with the present field.

Magnetic coercivity is the magnitude of a reverse applied magnetic field intensity required to bring a previously magnetized specimen's magnetization to zero on a specified hysteresis branch. It depends on material, preparation and measurement history. It differs from remanent magnetization, which is the remaining magnetization at zero applied field.

Teaching examples show how total-field magnetic anomalies depend on magnetic inclination, survey direction, geometry and remanent magnetization.

The difference $\Delta \mathbf{M}={\mathbf{M}}_{\mathrm{target}}-{\mathbf{M}}_{\mathrm{reference}}$ between a target region and the reference material it replaces. A weakly magnetic crater infill inside magnetic basalt can have a negative induced contrast, even though both materials have positive magnetic susceptibility. The sign and direction of this contrast, including remanent magnetization, determine a total-field magnetic anomaly together with geometry and the ambient field. Geophysical density contrast does not determine magnetic contrast.

Compare the scatter of remanent magnetization directions before and after correcting for folding. Improved agreement after restoring bedding supports acquisition before folding; agreement only in present coordinates supports a younger overprint. Partial unfolding can indicate acquisition during deformation or more complicated histories. The test constrains relative timing, rather than supplying an absolute age.

Test whether normal- and reversed-polarity remanent magnetization directions are statistically antipodal after suitable structural correction. Agreement supports recording of opposite polarities of the same large-scale magnetic field; failure can reveal overprints or other complications. Passing is not, by itself, proof of primary acquisition.

Paleomagnetism reconstructs past magnetic fields from remanent magnetization in rocks and other materials. Cooling volcanic minerals can acquire thermoremanent magnetization; later heating, alteration or mineral growth can change the record.

An oriented field sample preserves the relation between the measured magnetic direction and its geological setting. Shielded laboratory magnetometers and stepwise heating or alternating-field treatment help separate components acquired at different times. Combined with independent ages and structural corrections, the results test continental reconstruction and past field reversals.^[ref]

If removal restores the original random-domain magnetic state, the magnetostrictive strain and induced voltage return toward their original values. Elastic strain transfer then relaxes the stress on the central layer.

A ferromagnetic nickel layer can retain remanent magnetization and an altered domain population, so removing the external field does not guarantee removal of all magnetostriction. The electrical time response also depends on leakage and the input impedance of the voltmeter: an open-circuit strain-induced voltage can decay through a finite resistance even while some strain remains. The final observed voltage is therefore history- and circuit-dependent.

A planetary magnetic field is evidence about electrical conductivity, fluid motion and thermal evolution, but its presence alone does not identify a present planetary dynamo. One must separate internal global fields, crustal remanent magnetization and currents driven by the solar wind. The following discussion uses the observational picture available by 2009, including the early MESSENGER flybys and the Voyager, Galileo and Cassini results.

Outside a planet's internal electric currents, the internal component is approximately a potential magnetic field. Its spherical harmonic of degree $\ell$ decreases as $r^{-(\ell +2)}$. Measurements at different positions and altitudes can therefore distinguish a deep, low-degree source from localized crustal anomalies and external magnetospheric currents. Repeated observations, radio emissions, aurorae and particle measurements supply complementary evidence for a magnetosphere, while slow secular variation and records of past reversals test the internal field's evolution.

For Earth, ground observatories and satellite measurements reveal a predominantly dipolar field of several tens of microtesla at the surface, tilted relative to the rotation axis and changing with time. Magnetic minerals in rocks record a much older field and repeated geomagnetic reversals. These observations, together with seismic evidence for a liquid outer core, support an operating planetary dynamo in conducting iron alloy. Core temperatures exceed the relevant Curie temperatures, so ordinary permanent remanent magnetization cannot explain the main field. Thermal convection, cooling and compositional convection associated with inner-core growth supply buoyancy; the Coriolis force organizes the motion. The observed nonaxisymmetric components and time dependence are consistent with a dynamic source, rather than a fixed bar magnet.

Mariner 10 and the first two MESSENGER flybys established a weak but coherent intrinsic field at Mercury, with roughly dipolar structure closely aligned with its rotation axis. It is much weaker than Earth's surface field, but its global character favors a deep source over an explanation solely by localized crustal patches. A planetary dynamo in a fluid part of Mercury's large iron-rich core is the natural interpretation, supported by evidence for a molten core component. Light elements can depress the alloy's freezing temperature, and thermal or compositional buoyancy can maintain motion. Slow rotation is not enough to rule out dynamo action. The limited pre-orbital measurements do not uniquely determine the detailed core structure or the mechanism responsible for the field's weakness.

For Venus, spacecraft including Pioneer Venus found no appreciable internally generated global field. Nevertheless its ionosphere interacts with the solar wind, producing magnetic draping, a bow shock and an induced magnetosphere. Those external signatures are not evidence for an internal planetary dynamo. Venus is comparable to Earth in size and may possess a substantial conducting core; the absence of a detectable dynamo therefore need not mean that all of its core is solid. Insufficient core heat loss or stable stratification can prevent the required convection. Its slow rotation can affect flow organization, but rotation rate by itself is not a sufficient explanation of the contrast with Earth or Mercury.

For Mars, Mars Global Surveyor found strong, spatially localized crustal anomalies, especially in ancient southern terrain, rather than an appreciable present global dipole. This is remanent magnetization, indicating that an ancient field magnetized the crust while it formed and cooled. The distribution of anomalies and weakly magnetized major impact basins constrain when that ancient planetary dynamo operated; crustal magnetization is a record of past activity, not a present global dynamo. Modern interaction with the solar wind also produces an induced magnetosphere. Cooling and changes in core heat extraction can explain the cessation of dynamo-driving convection; the observations alone do not prove complete solidification of the core.

For Jupiter, radio emissions, its intense radiation belts and measurements by Pioneer, Voyager and Galileo demonstrate a strong global intrinsic field and an enormous magnetosphere. The field is broadly dipolar but tilted and contains higher multipoles. It is generated in a deep conducting fluid rather than by a permanent solid magnet: the principal conducting region is metallic hydrogen in the high-pressure interior. Cooling and gravitational energy release maintain convection, while rapid rotation organizes the flow. Plasma supplied by Io and currents in the magnetosphere strongly modify the observed external field, but cannot account for the internally sourced planetary component. Jupiter's large magnetic moment also reflects its large size; a moment ratio should not be confused with the ratio of local surface field strengths.

For Saturn, Pioneer, Voyager and Cassini measurements likewise show an intrinsic field and a magnetosphere, with a dipole strikingly close to the rotation axis. A planetary dynamo in conducting metallic hydrogen is supported by the same broad interior argument as for Jupiter. Interior cooling and differentiation can provide power, including energy associated with helium separation. The near alignment does not invalidate the Cowling anti-dynamo theorem: that theorem excludes an exactly axisymmetric isolated dynamo field, not a predominantly axisymmetric exterior with undetected nonaxisymmetric structure in its source region. A stably stratified conducting layer above the active region is one possible way to attenuate the observable nonaxisymmetric components; it is a model, not a uniquely established consequence of the observations.

For Uranus, Voyager 2 in 1986 observed an intrinsic field with a dipole tilted by about $59^{\circ }$ to the rotation axis and significantly displaced from the centre. Higher multipoles are substantial, so a centred dipole is an inadequate description. The field and associated magnetosphere indicate an active planetary dynamo, despite the planet's small intrinsic heat flux. That low luminosity constrains its thermal evolution and may indicate inhibited deep mixing; it does not demonstrate an absence of all conducting-fluid motion. A conducting, volatile-rich fluid shell is a plausible source region. The term ice giant describes bulk composition, not a claim that the dynamo region is ordinary frozen ice.

For Neptune, Voyager 2 in 1989 also found a highly non-dipolar, displaced intrinsic field, with a dipole tilt near $47^{\circ }$. Its field, radio emissions and magnetosphere imply another active planetary dynamo. Its larger intrinsic heat flux than Uranus supplies evidence for substantial continuing interior energy transport. Electrically conducting water-ammonia-rich mixtures at high pressure, with ionic or otherwise mobile charges, can supply the conducting region without requiring the metallic hydrogen layer characteristic of gas giants. Numerical dynamos in convecting shells surrounding more stably stratified interiors can produce strongly nonaxisymmetric, multipolar fields resembling those of the two ice giants. Such models show that their unusual field geometry is compatible with dynamo action, but field measurements do not uniquely identify the shell's composition or thickness.

The maintenance mechanism is governed by the resistive induction equation,A conducting fluid needs a sufficiently large magnetic Reynolds number and a flow geometry that regenerates magnetic flux rather than merely amplifying one component temporarily. Three-dimensional stretching and twisting can couple poloidal and toroidal fields; strictly planar regeneration and a strictly axisymmetric magnetic field are restricted by the relevant anti-dynamo theorems. Rotation influences this regeneration through the Coriolis force, but does not provide an inexhaustible power source merely by being present.

Without regeneration, the characteristic magnetic diffusion time is ${\tau }_{\eta }\sim L^2/\eta$. For a terrestrial core scale of order $10^6$ metres and diffusivity of order one square metre per second, this is of order $10^4$–$10^5$ years, far shorter than geological ages. Long-lived global fields therefore require continual energy input. A schematic magnetic energy balance iswhen boundary energy fluxes vanish. Mechanical work against the Lorentz force density supplies the energy lost as Ohmic heating. Thermal cooling, latent heat release, compositional convection and differentiation supply that mechanical power. Magnetic feedback eventually changes the flow and saturates the field. Strong conductivity without an adequate energy source is not sufficient for a dynamo.

The 2009 observations support active global dynamos in Mercury, Earth, Jupiter, Saturn, Uranus and Neptune; Venus has no detected appreciable intrinsic dynamo field, and Mars preserves evidence of an extinct earlier dynamo in its crust. Induced fields and surviving remanence explain why planets without a current global dynamo can still display magnetic phenomena. The diversity of field geometries and strengths constrains, rather than uniquely solves, the diversity of planetary conducting regions and their convective histories.

Magnetization $\mathbf{M}$ is magnetic dipole moment per unit volume. In SI units,in a linear isotropic response. The internal field matters: for a uniformly magnetized ellipsoid it is ${\mathbf{H}}_{\mathrm{int}}={\mathbf{H}}_{\mathrm{applied}}-{\mathbf{N}}_d\mathbf{M}$. Sample shape therefore affects an apparent magnetic susceptibility.

Diamagnetism opposes the applied field, giving small negative magnetic susceptibility from the induced orbital response. It is often only weakly temperature dependent. Paramagnetism aligns pre-existing moments and gives positive magnetic susceptibility; independent localized moments obey approximately $\chi =C/T$ in weak fields before saturating. Pauli paramagnetism of conduction electrons is a different, weakly temperature-dependent mechanism.

Ferromagnetism involves collective exchange-driven alignment and spontaneous magnetization below the Curie temperature. A specimen can nevertheless have nearly zero total moment because magnetic domains point in different directions. Field-driven domain-wall motion and rotation change the net magnetization. Antiferromagnets have compensating ordered sublattices below a Néel temperature; ferrimagnets have oppositely ordered but unequal sublattice moments and retain a net moment. Ferrites are useful examples of electrically resistive ferrimagnetic core materials.

Ferromagnetic response is nonlinear and history dependent. A hysteresis loop displays remanent magnetization, magnetic coercivity and saturation. A single constant magnetic permeability cannot describe the entire loop: differential magnetic permeability describes its local slope. The quasistatic energy loss per unit volume and cycle is the loop area $\oint HdB$. Soft magnetic materials have low magnetic coercivity and usually high useful magnetic permeability; hard magnetic materials retain magnetization and suit permanent magnets.

An electromagnet normally uses a soft, high-permeability core to guide flux generated by a coil. For a uniform-section core with length ${\ell }_c$ and air gap $g$, neglecting leakage and fringing,An air gap can dominate the magnetic reluctance even when the core magnetic permeability is large. Core saturation limits the improvement with current, while winding resistance causes heating. For alternating operation, laminations suppress eddy-current loops in metallic cores; high-resistivity ferrites also reduce those losses. Low hysteresis loss is important in repeatedly cycled cores, whereas high magnetic coercivity is valuable in a permanent magnet. Useful design therefore depends on the full magnetic response, electrical losses and operating frequency, rather than the largest quoted magnetic permeability alone.

The decisive change was from moving continents within a supposedly permanent ocean floor to moving coherent tectonic plates that include both continental and oceanic lithosphere. Several independent observations made that change testable.

Continental connections supplied the initial problem. In the early twentieth century, Alfred Wegener assembled matching continental margins, correlatable rock belts and mountain chains, shared fossil assemblages, and paleoclimate indicators into the case for continental drift. Reassembling Gondwana, for example, makes geographically separated glacial deposits and striation directions compatible with one ice-sheet system. Fits at the continental shelf edge are physically more meaningful than exact fits to modern coastlines, which have been modified by erosion and sea-level change. The evidence suggested relative movement, but did not justify the proposed forces: continents cannot readily plough independently through strong oceanic rock. A convincing mechanism and independent motion measurements were missing.

Oceanography changed the boundary conditions. Echo-sounding surveys revealed a connected spreading ridge system, axial valleys, subduction trenches and long fracture zones. Seismic refraction surveys established systematic differences between continental and oceanic crust. Thin oceanic sediment cover, high ridge heat flux and the lack of very old exposed oceanic basement made permanent, ancient ocean basins increasingly implausible. Harry Hammond Hess proposed creation of oceanic lithosphere at ridges and recycling at trenches: seafloor spreading without requiring an expanding Earth. Slow mantle convection supplied a physically plausible connection between surface transport and internal heat loss. The mechanism need not have been completely quantified before its kinematic predictions could be tested.^[ref]

Magnetic records supplied a clock and a speedometer. Dated continental lavas established a sequence of geomagnetic reversals. Marine magnetometers then found elongated, approximately paired marine magnetic stripes on either side of ridges. The 1963 interpretation by F. J. Vine and D. H. Matthews combined repeated reversals with seafloor spreading: cooling basalt locks in remanent magnetization, and continuous motion converts a time sequence into a spatial sequence. If a polarity interval lasts $\Delta t$ and occupies width $w$ on one ridge flank, its half-spreading rate is $w/\Delta t$. Matching several reversals tests the predicted sequence, rather than merely fitting a single stripe.^[ref] Different apparent polar wander paths for different continents also became mutually consistent after continental reconstruction, favoring relative continental motion over independent magnetic-pole histories.

Earthquakes identified creation, translation and consumption. Improved global seismology located shallow earthquakes along ridges and transforms, and dipping Wadati-Benioff zones beneath trenches. Their progressive focal depths identified cold, coherent slabs entering the mantle. Focal mechanisms showed extension at spreading boundaries, tangential slip at transforms and convergence at trenches. In 1965, John Tuzo Wilson's transform fault interpretation made a particularly discriminating prediction: active slip occurs between offset ridge segments, with a sense that can be opposite to that inferred by treating the entire lineament as an ordinary offset fault. The outer fracture zones are inherited traces, not continuing active plate boundaries. Agreement of focal mechanisms with the transform prediction linked magnetic and seismic evidence.

The late-1960s synthesis made these observations one quantitative theory. Relative motion of rigid tectonic plates on a sphere can be described by an Euler angular velocity vector, with $\mathbf{v}=\mathbf{\omega }\times \mathbf{r}$. Spreading rates, transform azimuths and slip directions must fit the same rotation, and relative angular velocities must close around plate circuits. The resulting framework accounted for global boundary geometry and earthquake mechanisms without moving continents separately from the seafloor. Deep-ocean drilling beginning in 1968 subsequently confirmed that basement and overlying sediments generally become older away from ridges; this was a powerful confirmation of an already emerging synthesis, not a prerequisite discovered decades earlier.^[ref]

Thus plate tectonics succeeded through agreement between geological reconstruction, magnetic chronology, ocean-floor structure, seismology and rigid-plate kinematics. Modern satellite geodesy verifies motions directly, but belongs to the later confirmation of the theory, not its original 1960s evidence.

Repeated assembly and dispersal are supported by mutually consistent paleogeography, paleomagnetism, dated collision belts and subsequent rifted margins. A useful reconstruction must explain both former connections and later separation, at the same geological ages.

For the youngest well-constrained example, Pangaea, matching continental outlines become more compelling when the fit uses the continental edges rather than mobile modern shorelines. More discriminating evidence includes the continuation of mountain belts, sedimentary successions and distinctive basement rocks across now-separated continents. Correlated terrestrial fossil assemblages and the distribution of glacial deposits become geographically coherent when the continents are restored. Each observation alone can have alternatives, but a single reconstruction that satisfies several independent tests is much harder to explain by coincidence.

For older examples, the most useful surviving record lies within the cratons and their margins. Dated suture zones, ophiolites, metamorphic belts and pressure-temperature-time paths document former ocean closure and continental collision. Restoring now-separated belts to continuity tests an assembly. Subsequent continental rifting, matching dike swarms, large igneous provinces and the transition to passive margins test its breakup. Uranium-lead dating of zircon, including detrital zircon populations and sedimentary provenance, helps establish whether the proposed connections existed at the same time.

Paleomagnetism supplies an independent quantitative test. A primary remanent magnetization constrains ancient latitude and orientation. After a proposed relative rotation brings two blocks together, compatible apparent polar wander paths over an interval support their travelling together; divergence of those paths can document separation. Radiometric dating, a paleomagnetic fold test and a paleomagnetic reversal test help identify primary records and distinguish them from remagnetization. There remain important ambiguities: conventional paleomagnetism does not fix absolute longitude, and sparse ages, later deformation and true polar wander complicate a reconstruction.

The broad succession is Columbia or Nuna, assembled mainly around 1.9–1.6 billion years ago; Rodinia, assembled mainly around 1.1–0.9 billion years ago and dispersed in stages during the later Proterozoic; and Pangaea, assembled by roughly 300 million years ago and breaking apart from roughly 200 million years ago. These are broad intervals rather than synchronous global events. A quantitative Nuna reconstruction combines paleomagnetism with the histories of continental margins rather than relying only on matching rock ages.^[ref]

Repeated global peaks in dated magmatism and metamorphism offer supporting evidence, but cannot prove a supercontinent cycle by themselves: erosion, burial and preferential preservation also change the observed age distribution. The persuasive case is the recurrence of dated assembly–breakup sequences in different continental configurations, with stronger geometric constraints for Pangaea than for the older supercontinents. A Wilson cycle describes an individual ocean's opening and closure; a supercontinent cycle concerns the much larger-scale continental assembly and dispersal.

In a weak applied field, magnetic susceptibility relates magnetization to magnetic field intensity, $M=\chi H$. Its sign, temperature dependence and nonlinear field dependence distinguish several mechanisms.

Diamagnetism is the orbital response opposing an applied magnetic field, with $\chi <0$. Closed-shell atoms and filled bands generally give a weak, nearly temperature-independent response. In a simple free electron metal, Landau diamagnetism contributes ${\chi }_L=-{\chi }_P/3$; the factor is specific to the isotropic parabolic-band model and is not universal in crystals.

Paramagnetism gives $\chi >0$. Localized magnetic moments align statistically with the field against thermal disorder. For independent moments of angular momentum $J$,which is the Curie law. Exchange interactions often lead approximately to the Curie–Weiss law, $\chi =C/(T-\Theta )$, sufficiently far above any ordering temperature. The sign of $\Theta$ suggests predominantly parallel or antiparallel exchange, though it is not a complete classification. Conduction electrons instead exhibit Pauli paramagnetism:for $g\simeq 2$ and a spin-summed density of states per unit volume. Only states close to the Fermi energy change occupation, making this response nearly temperature independent when $k_{B}T\ll E_F$.

Ferromagnetism has spontaneous parallel magnetic order below a Curie temperature. Exchange interaction, not simply classical dipole attraction, provides the dominant alignment mechanism. In the convention $H=-J_{\mathrm{ex}}{\sum }_{⟨ij⟩}{\mathbf{S}}_i\cdot {\mathbf{S}}_j$, positive $J_{\mathrm{ex}}$ favours alignment. Magnetic domains can make a ferromagnet's total magnetization vanish before an external field aligns its domains. Domain motion and anisotropy produce saturation, hysteresis, remanent magnetization and a reverse field measured by magnetic coercivity.

Antiferromagnetism has oppositely ordered sublattices below a Néel temperature; equal opposing moments give zero net magnetization while retaining a nonzero staggered order parameter. A susceptibility anomaly and magnetic neutron diffraction reveal this order even when bulk magnetization vanishes. Ferrimagnetism also has opposing sublattices but unequal contributions, giving a nonzero spontaneous net moment. Above their ordering temperatures both can become paramagnetic. Measurements with a magnetometer as a function of field and temperature, supplemented by magnetic diffraction, therefore distinguishes a compensated ordered material from an ordinary paramagnet.

Collect a magnetic survey along the traverse with a calibrated total-field magnetometer, recording time, accurately surveyed position and sensor height. Extend observations beyond the crater to establish the background, repeat stations or tie lines to test consistency, and use a stationary base-station magnetometer to monitor temporal field changes. Keep the instrument away from vehicles, fences and magnetic equipment; map unavoidable cultural sources rather than treating them as geological signals.

Correct instrument offsets and heading effects where applicable, remove measured diurnal variation, reject or separately treat magnetic-storm intervals, and subtract the appropriate large-scale geomagnetic field at the survey epoch. Level overlapping traverses and state whether a local regional trend has also been removed. Unlike gravity, there is no universal rock-independent Bouguer correction for magnetic topography: a magnetic topographic effect needs a model of terrain and magnetization.

Measure representative magnetic susceptibility and remanent magnetization on oriented rock samples to interpret the profile. Total field alone does not tell whether a contrast comes from induced or remanent magnetization, crater excavation, or strongly magnetic material in the infill.

The supplied south–north profile has a large southern/interior negative trough and a sharp positive peak toward the northern rim. That is opposite to the simplest positive, presently induced magnetic body in question 5(d). It therefore does not justify interpreting the crater as a concentration of strongly magnetic meteorite material.

A negative magnetization contrast from replacing magnetic basalt already reverses the simple induced-body response. In addition, the target Deccan Traps can retain strong remanent magnetization whose direction differs from the present geomagnetic field; crater excavation and rim geometry then produce a strong magnetic topographic effect. Rock-magnetic measurements and forward modelling distinguish these contributions. A primary study of this crater attributes most of its anomaly to magnetized target basalts and topography, with a comparatively small contribution from the breccia and post-impact sediment.^[ref]

The curve alone is not a unique diagnosis of reversed polarity, impact-induced magnetization or a buried iron mass. The physical conclusion supported by the comparison is that a positive induced-body model is inadequate; inherited target-rock magnetization, its removal and geometry must be modelled.

Measure total magnetic field along the same south–north line with a calibrated magnetometer, recording position, time and sensor height. A simultaneous base-station magnetometer measures temporal variation so that diurnal changes can be removed from the moving survey. Avoid disturbed periods and magnetic contamination from vehicles, fences, power lines and equipment. Choose station spacing much smaller than the expected anomaly width, for example tens to hundreds of metres for a kilometre-scale target.

Subtract the epoch-appropriate International Geomagnetic Reference Field or another stated regional main-field model to obtain a total-field magnetic anomaly. Level overlapping traverses and remove offsets or drift where appropriate. Accurate terrain/sensor geometry is needed for comparison with a geological model, but there is no universal magnetic analogue of a constant-density Bouguer slab correction: the effect depends on the distribution and direction of magnetization. Measure magnetic susceptibility and remanent magnetization on representative greenstones, granite and host rock to test the assumed magnetic sources.

Assume the greenstone belt is more magnetically susceptible than the host rocks and granite, its magnetization is mainly induced magnetization, and the body is roughly east–west elongated so that the south–north line crosses it. At southern magnetic latitudes the main field has negative magnetic inclination in a north-and-down coordinate convention. The total-field magnetic anomaly is then generally asymmetric: the principal negative lobe is on the southern side and the positive lobe is displaced northward for the simple induced source illustrated here. The exact lobe sizes and peak positions depend on body geometry and the actual magnetic inclination.^[ref]

An explicit sketching model is an induced magnetic dipole at depth $d$. With northward coordinate $x$, $\mathbf{r}=(x,-d)$ and unit field direction $\hat{\mathbf{F}}=(\cos I,\sin I)$, its normalized total-field magnetic anomaly isThe plot uses $I=-36^{\circ }$ only as an illustrative dipole-field inclination for a latitude near $20^{\circ }$ south, not a measured modern field at the site. A wide greenstone belt would broaden the response and can produce prominent edge anomalies. Remanent magnetization or a magnetic granite could change the sketch substantially; gravity alone cannot identify the magnetic source.