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Age of the sea floor. Much of the dating information
comes from magnetic anomalies.
GeophysicsFrom Wikipedia, the free encyclopedia
Geophysics /di ofzks/ is the physics of the Earthand its
environment in space; also the study of theEarth using quantitative
physical methods. The termgeophysics sometimes refers only to the
geologicalapplications: Earth's shape; its gravitational
andmagnetic fields; its internal structure and composition;its
dynamics and their surface expression in platetectonics, the
generation of magmas, volcanism and
rock formation.[1] However, modern geophysicsorganizations use a
broader definition that includes thehydrological cycle including
snow and ice; fluiddynamics of the oceans and the atmosphere;
electricityand magnetism in the ionosphere and magnetosphereand
solar-terrestrial relations; and analogous problems
associated with the Moon and other planets.[1][2][3]
Although geophysics was only recognized as a separate discipline
in the 19th century, its origins go back to ancienthistory. The
first magnetic compasses were lodestones, appearing in written
records, found in early survivingdescriptions from China, India and
Greece, with a modern magnetic compass dating back to the fourth
century BCand the first seismoscope was built in 132 BC.
Geophysical methods were developed for navigation; Isaac
Newtonapplied his theory of mechanics to the tides and the
precession of the equinox; and instruments were developed tomeasure
the Earth's shape, density and gravity field, as well as the
components of the water cycle. In the 20thcentury, geophysical
methods were developed for remote exploration of the solid Earth
and the ocean, andgeophysics played an essential role in the
development of the theory of plate tectonics.
Geophysics is applied to societal needs, such as mineral
resources, mitigation of natural hazards and environmental
protection.[2] Geophysical survey data are used to analyze
potential petroleum reservoirs and mineral deposits,locate
groundwater, find archaeological relics, determine the thickness of
glaciers and soils, and assess sites forenvironmental
remediation.
Contents
1 Physical phenomena
1.1 Gravity
1.2 Heat flow
1.3 Vibrations
1.4 Electricity
1.5 Electromagnetic waves
1.6 Magnetism
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1.7 Radioactivity
1.8 Fluid dynamics
1.9 Mineral physics
2 Regions of the Earth
2.1 Size and form of the Earth
2.2 Structure of the Earth
2.3 Magnetosphere
3 Methods
3.1 Geodesy
3.2 Space probes
4 History
4.1 Ancient and classical eras
4.2 Beginnings of modern science
5 See also
6 Notes
7 References
8 External links
Physical phenomena
Geophysics is a highly interdisciplinary subject and
geophysicists contribute to every area of the Earth sciences.
Toprovide a clearer idea of what constitutes geophysics, this
section describes phenomena that are studied in physicsand how they
relate to the Earth and its surroundings.
Gravity
Main article: Gravity of Earth
Further information: Physical geodesy, Gravimetry
The gravitational pull of the Moon and Sun give rise to two high
tides and two low tides every lunar day, or every24 hours and 50
minutes. Therefore, there is a gap of 12 hours and 25 minutes
between every high tide and
between every low tide.[4]
Gravitational forces make rocks press down on deeper rocks,
increasing their density as the depth increases.[5]
Measurements of gravitational acceleration and gravitational
potential at the Earth's surface and above it can be
used to look for mineral deposits (see gravity anomaly and
gravimetry).[6] The surface gravitational field providesinformation
on the dynamics of tectonic plates. The geopotential surface called
the geoid is one definition of theshape of the Earth. The geoid
would be the global mean sea level if the oceans were in
equilibrium and could be
extended through the continents (such as with very narrow
canals).[7]
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A map of deviations in gravity from a
perfectly smooth, idealized Earth.
A model of thermal convection in the Earth's
mantle. The thin red columns are mantle
plumes.
Heat flow
Main article: Geothermal gradient
The Earth is cooling, and the resulting heat flow generates
theEarth's magnetic field through the geodynamo and plate
tectonics
through mantle convection.[8] The main sources of heat are
theprimordial heat and radioactivity, although there are
alsocontributions from phase transitions. Heat is mostly carried to
thesurface by thermal convection, although there are two
thermalboundary layers the core-mantle boundary and the
lithosphere
in which heat is transported by conduction.[9] Some heat is
carriedup from the bottom of the mantle by mantle plumes. The heat
flow
at the Earth's surface is about 4.2 1013 W, and it is a
potential source of geothermal energy.[10]
Vibrations
Main article: Seismology
Seismic waves are vibrations that travel through the Earth's
interioror along its surface. The entire Earth can also oscillate
in forms thatare called normal modes or free oscillations of the
Earth. Groundmotions from waves or normal modes are measured
usingseismographs. If the waves come from a localized source such
asan earthquake or explosion, measurements at more than one
location can be used to locate the source. The
locations of earthquakes provide information on plate tectonics
and mantle convection.[11][12]
Measurements of seismic waves are a source of information on the
region that the waves travel through. If thedensity or composition
of the rock changes suddenly, some of the waves are reflected.
Reflections can provide
information on near-surface structure.[6] Changes in the travel
direction, called refraction, can be used to infer the
deep structure of the Earth.[12]
Earthquakes pose a risk to humans. Understanding their
mechanisms, which depend on the type of earthquake(e.g., intraplate
or deep focus), can lead to better estimates of earthquake risk and
improvements in earthquake
engineering.[13]
Electricity
Although we mainly notice electricity during thunderstorms,
there is always a downward electric field near the
surface that averages 120 V m1.[14] Relative to the solid Earth,
the atmosphere has a net positive charge due to
bombardment by cosmic rays. A current of about 1800 A flows in
the global circuit.[14] It flows downward fromthe ionosphere over
most of the Earth and back upwards through thunderstorms. The flow
is manifested by lightningbelow the clouds and sprites above.
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Illustration of the deformations of a block by
body waves and surface waves (see seismic
wave).
A variety of electric methods are used in geophysical
survey.Some measure spontaneous potential, a potential that arises
in theground because of man-made or natural disturbances.
Telluriccurrents flow in Earth and the oceans. They have two
causes:electromagnetic induction by the time-varying,
external-origingeomagnetic field and motion of conducting bodies
(such as
seawater) across the Earth's permanent magnetic field.[15]
Thedistribution of telluric current density can be used to
detectvariations in electrical resistivity of underground
structures.Geophysicists can also provide the electric current
themselves (seeinduced polarization and electrical resistivity
tomography).
Electromagnetic waves
Electromagnetic waves occur in the ionosphere andmagnetosphere
as well as the Earth's outer core. Dawn chorus isbelieved to be
caused by high-energy electrons that get caught inthe Van Allen
radiation belt. Whistlers are produced by lightningstrikes. Hiss
may be generated by both. Electromagnetic wavesmay also be
generated by earthquakes (see seismo-electromagnetics).
In the Earth's outer core, electric currents in the highly
conductiveliquid iron create magnetic fields by electromagnetic
induction (seegeodynamo). Alfvn waves are magnetohydrodynamic waves
inthe magnetosphere or the Earth's core. In the core, they probably
have little observable effect on the geomagnetic
field, but slower waves such as magnetic Rossby waves may be one
source of geomagnetic secular variation.[16]
Electromagnetic methods that are used for geophysical survey
include transient electromagnetics andmagnetotellurics.
Magnetism
Further information: Earth's magnetic field and
paleomagnetism
The Earth's magnetic field protects the Earth from the deadly
solar wind and has long been used for navigation. It
originates in the fluid motions of the Earth's outer core (see
geodynamo).[16] The magnetic field in the upper
atmosphere gives rise to the auroras.[17]
The Earth's field is roughly like a tilted dipole, but it
changes over time (a phenomenon called geomagnetic
secularvariation). Mostly the geomagnetic pole stays near the
geographic pole, but at random intervals averaging 440,000to a
million years or so, the polarity of the Earth's field reverses.
These geomagnetic reversals, analyzed within aGeomagnetic Polarity
Time Scale, contain 184 polarity intervals in the last 83 million
years, with change infrequency over time, with the most recent
brief complete reversal of the Laschamp event occurring 41,000
yearsago during the last glacial period. Geologists observed
geomagnetic reversal recorded in volcanic rocks,
throughmagnetostratigraphy correlation (see natural remanent
magnetization) and their signature can be seen as parallellinear
magnetic anomaly stripes on the seafloor. These stripes provide
quantitative information on seafloor
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Earth's dipole axis (pink line) is
tilted away from the rotational axis
(blue line).
Example of a radioactive decay chain
(see Radiometric dating).
spreading, a part of plate tectonics. They are the basis of
magnetostratigraphy, which correlates magnetic reversals
with other stratigraphies to construct geologic time scales.[18]
In addition, the magnetization in rocks can be used to
measure the motion of continents.[16]
Radioactivity
Further information: Radiometric dating and geotherm
Radioactive decay accountsfor about 80% of the Earth'sinternal
heat, powering thegeodynamo and plate
tectonics.[19] The main heat-producing isotopes arepotassium-40,
uranium-238,uranium-235, and thorium-
232.[20] Radioactive elementsare used for radiometric dating,the
primary method forestablishing an absolute timescale in
geochronology.Unstable isotopes decay atpredictable rates, and
the
decay rates of different isotopes cover several orders of
magnitude,so radioactive decay can be used to accurately date both
recent
events and events in past geologic eras.[21]
Fluid dynamics
Main article: Geophysical fluid dynamics
Fluid motions occur in the magnetosphere, atmosphere, ocean,
mantle and core. Even the mantle, though it has anenormous
viscosity, flows like a fluid over long time intervals (see
geodynamics). This flow is reflected inphenomena such as isostasy,
post-glacial rebound and mantle plumes. The mantle flow drives
plate tectonics and
the flow in the Earth's core drives the geodynamo.[16]
Geophysical fluid dynamics is a primary tool in physical
oceanography and meteorology. The rotation of the Earthhas profound
effects on the Earth's fluid dynamics, often due to the Coriolis
effect. In the atmosphere it gives rise tolarge-scale patterns like
Rossby waves and determines the basic circulation patterns of
storms. In the ocean they
drive large-scale circulation patterns as well as Kelvin waves
and Ekman spirals at the ocean surface.[22] In the
Earth's core, the circulation of the molten iron is structured
by Taylor columns.[16]
Waves and other phenomena in the magnetosphere can be modeled
using magnetohydrodynamics.
Mineral physics
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Further information: Mineral physics
The physical properties of minerals must be understood to infer
the composition of the Earth's interior fromseismology, the
geothermal gradient and other sources of information. Mineral
physicists study the elastic propertiesof minerals; their
high-pressure phase diagrams, melting points and equations of state
at high pressure; and therheological properties of rocks, or their
ability to flow. Deformation of rocks by creep make flow possible,
althoughover short times the rocks are brittle. The viscosity of
rocks is affected by temperature and pressure, and in turn
determines the rates at which tectonic plates move (see
geodynamics).[5]
Water is a very complex substance and its unique properties are
essential for life.[23] Its physical properties shapethe
hydrosphere and are an essential part of the water cycle and
climate. Its thermodynamic properties determineevaporation and the
thermal gradient in the atmosphere. The many types of precipitation
involve a complex mixture
of processes such as coalescence, supercooling and
supersaturation.[24] Some of the precipitated water
becomesgroundwater, and groundwater flow includes phenomena such as
percolation, while the conductivity of watermakes electrical and
electromagnetic methods useful for tracking groundwater flow.
Physical properties of water
such as salinity have a large effect on its motion in the
oceans.[22]
The many phases of ice form the cryosphere and come in forms
like ice sheets, glaciers, sea ice, freshwater ice,
snow, and frozen ground (or permafrost).[25]
Regions of the Earth
Size and form of the Earth
Main article: Figure of the Earth
The Earth is roughly spherical, but it bulges towards the
Equator, so it is roughly in the shape of an ellipsoid (seeEarth
ellipsoid). This bulge is due to its rotation and is nearly
consistent with an Earth in hydrostatic equilibrium. Thedetailed
shape of the Earth, however, is also affected by the distribution
of continents and ocean basins, and to
some extent by the dynamics of the plates.[7]
Structure of the Earth
Main article: Structure of the Earth
Evidence from seismology, heat flow at the surface, and mineral
physics is combined with the Earth's mass andmoment of inertia to
infer models of the Earth's interior its composition, density,
temperature, pressure. Forexample, the Earth's mean specific
gravity (5.515) is far higher than the typical specific gravity of
rocks at thesurface (2.73.3), implying that the deeper material is
denser. This is also implied by its low moment of inertia (
0.33 M R2, compared to 0.4 M R2 for a sphere of constant
density). However, some of the density increase iscompression under
the enormous pressures inside the Earth. The effect of pressure can
be calculated using theAdamsWilliamson equation. The conclusion is
that pressure alone cannot account for the increase in density.
Instead, we know that the Earth's core is composed of an alloy
of iron and other minerals.[5]
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Seismic velocities and boundaries in the
interior of the Earth sampled by seismic
waves.
Schematic of Earth's magnetosphere. The solar
wind flows from left to right.
Reconstructions of seismic waves in the deep interior of the
Earth show that there are no S-waves in the outer core.This
indicates that the outer core is liquid, because liquids cannot
support shear. The outer core is liquid, and themotion of this
highly conductive fluid generates the Earth's field (see
geodynamo). The inner core, however, is solid
because of the enormous pressure.[7]
Reconstruction of seismic reflections in the deep interior
indicate some major discontinuities in seismic velocities
thatdemarcate the major zones of the Earth: inner core, outer core,
mantle, lithosphere and crust. The mantle itself isdivided into the
upper mantle, transition zone, lower mantle and D layer. Between
the crust and the mantle is the
Mohorovii discontinuity.[7]
The seismic model of the Earth does not by itself determine the
composition of the layers. For a complete model ofthe Earth,
mineral physics is needed to interpret seismic velocitiesin terms
of composition. The mineral properties are temperature-dependent,
so the geotherm must also be determined. Thisrequires physical
theory for thermal conduction and convectionand the heat
contribution of radioactive elements. The main modelfor the radial
structure of the interior of the Earth is the preliminaryreference
Earth model (PREM). Some parts of this model havebeen updated by
recent findings in mineral physics (see post-perovskite) and
supplemented by seismic tomography. The mantleis mainly composed of
silicates, and the boundaries between layers
of the mantle are consistent with phase transitions.[5]
The mantle acts as a solid for seismic waves, but under
highpressures and temperatures it deforms so that over millions
ofyears it acts like a liquid. This makes plate tectonics
possible.Geodynamics is the study of the fluid flow in the mantle
and core.
Magnetosphere
Main article: Magnetosphere
If a planet's magnetic field is strong enough, its
interactionwith the solar wind forms a magnetosphere. Early
spaceprobes mapped out the gross dimensions of the Earth'smagnetic
field, which extends about 10 Earth radii towardsthe Sun. The solar
wind, a stream of charged particles,streams out and around the
terrestrial magnetic field, andcontinues behind the magnetic tail,
hundreds of Earth radiidownstream. Inside the magnetosphere, there
are relativelydense regions of solar wind particles called the Van
Allen
radiation belts.[17]
Methods
Geodesy
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Main article: Geodesy
Geophysical measurements are generally at a particular time and
place. Accurate measurements of position, alongwith earth
deformation and gravity, are the province of geodesy. While geodesy
and geophysics are separate fields,the two are so closely connected
that many scientific organizations such as the American Geophysical
Union, the
Canadian Geophysical Union and the International Union of
Geodesy and Geophysics encompass both.[26]
Absolute positions are most frequently determined using the
global positioning system (GPS). A three-dimensionalposition is
calculated using messages from four or more visible satellites and
referred to the 1980 GeodeticReference System. An alternative,
optical astronomy, combines astronomical coordinates and the local
gravityvector to get geodetic coordinates. This method only
provides the position in two coordinates and is more difficultto
use than GPS. However, it is useful for measuring motions of the
Earth such as nutation and Chandler wobble.
Relative positions of two or more points can be determined using
very-long-baseline interferometry.[26][27][28]
Gravity measurements became part of geodesy because they were
needed to related measurements at the surfaceof the Earth to the
reference coordinate system. Gravity measurements on land can be
made using gravimetersdeployed either on the surface or in
helicopter flyovers. Since the 1960s, the Earth's gravity field has
beenmeasured by analyzing the motion of satellites. Sea level can
also be measured by satellites using radar altimetry,
contributing to a more accurate geoid.[26] In 2002, NASA
launched the Gravity Recovery and Climate Experiment(GRACE),
wherein two twin satellites map variations in Earth's gravity field
by making measurements of thedistance between the two satellites
using GPS and a microwave ranging system. Gravity variations
detected byGRACE include those caused by changes in ocean currents;
runoff and ground water depletion; melting ice sheets
and glaciers.[29]
Space probes
Space probes made it possible to collect data from not only the
visible light region, but in other areas of theelectromagnetic
spectrum. The planets can be characterized by their force fields:
gravity and their magnetic fields,which are studied through
geophysics and space physics.
Measuring the changes in acceleration experienced by spacecraft
as they orbit has allowed fine details of the gravityfields of the
planets to be mapped. For example, in the 1970s, the gravity field
disturbances above lunar maria weremeasured through lunar orbiters,
which led to the discovery of concentrations of mass, mascons,
beneath the
Imbrium, Serenitatis, Crisium, Nectaris and Humorum
basins.[30]
History
Main article: History of geophysics
Geophysics emerged as a separate discipline only in the 19th
century, from the intersection of physical geography,
geology, astronomy, meteorology, and physics.[31][32] However,
many geophysical phenomena such as theEarth's magnetic field and
earthquakes have been investigated since the ancient era.
Ancient and classical eras
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Replica of Zhang Heng's
seismoscope, possibly the
first contribution to
seismology.
The magnetic compass existed in China back as far as the fourth
century BC. It was used as much for feng shui asfor navigation on
land. It was not until good steel needles could be forged
thatcompasses were used for navigation at sea; before that, they
could not retain theirmagnetism long enough to be useful. The first
mention of a compass in Europe
was in 1190 AD.[33]
In circa 240 BC, Eratosthenes of Cyrene deduced that the Earth
was round andmeasured the circumference of the Earth, using
trigonometry and the angle of theSun at more than one latitude in
Egypt. He developed a system of latitude and
longitude.[34]
Perhaps the earliest contribution to seismology was the
invention of a
seismoscope by the prolific inventor Zhang Heng in 132 AD.[35]
This instrumentwas designed to drop a bronze ball from the mouth of
a dragon into the mouth ofa toad. By looking at which of eight
toads had the ball, one could determine thedirection of the
earthquake. It was 1571 years before the first design for
aseismoscope was published in Europe, by Jean de la Hautefeuille.
It was never
built.[36]
Beginnings of modern science
One of the publications that marked the beginning of modern
science was William Gilbert's De Magnete (1600), areport of a
series of meticulous experiments in magnetism. Gilbert deduced that
compasses point north because the
Earth itself is magnetic.[16]
In 1687 Isaac Newton published his Principia, which not only
laid the foundations for classical mechanics andgravitation but
also explained a variety of geophysical phenomena such as the tides
and the precession of the
equinox.[37]
The first seismometer, an instrument capable of keeping a
continuous record of seismic activity, was built by James
Forbes in 1844.[36]
See also
List of geophysicists
Outline of geophysics
Notes
1. ^a b Sheriff 1991
2. ^a b IUGG 2011
3. ^ AGU 2011
4. ^ Ross 1995, pp. 236242
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5. ^a b c d Poirier 2000
6. ^a b Telford, Geldart & Sheriff 1990
7. ^a b c d Lowrie 2004
8. ^ Davies 2001
9. ^ Fowler 2005
10. ^ Pollack, Hurter & Johnson 1993
11. ^ Shearer, Peter M. (2009). Introduction to seismology (2nd
ed.). Cambridge: Cambridge University Press.
ISBN 9780521708425.
12. ^a b Stein & Wysession 2003
13. ^ Bozorgnia & Bertero 2004
14. ^a b Harrison & Carslaw 2003
15. ^ Lanzerotti & Gregori 1986
16. ^a b c d e f Merrill, McElhinny & McFadden 1996
17. ^a b Kivelson & Russell 1995
18. ^ Opdyke & Channell 1996
19. ^ Turcotte & Schubert 2002
20. ^ Sanders 2003
21. ^ Renne, Ludwig & Karner 2000
22. ^a b Pedlosky 1987
23. ^ Sadava et al. 2009
24. ^ Sirvatka 2003
25. ^ CFG 2011
26. ^a b c National Research Council (U.S.). Committee on
Geodesy 1985
27. ^ Defense Mapping Agency 1984
28. ^ Torge 2001
29. ^ CSR 2011
30. ^ Muller & Sjogren 1968
31. ^ Hardy & Goodman 2005
32. ^ Schrder, W. (2010). "History of geophysics". Acta
Geodaetica et Geophysica Hungarica 45 (2): 253261.
doi:10.1556/AGeod.45.2010.2.9
(http://dx.doi.org/10.1556%2FAGeod.45.2010.2.9).
33. ^ Temple 2006, pp. 162166
34. ^ Eratosthenes 2010
35. ^ Temple 2006, pp. 177181
36. ^a b Dewey & Byerly 1969
37. ^ Newton 1999 Section 3
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Commission on Geophysical Risk and Sustainability (GeoRisk),
International Union of Geodesy and
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Study of the Earth's Deep Interior, a Committee of IUGG
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Union Commissions (IUGG)
(http://www.iugg.org/about/commissions/)
USGS Geomagnetism Program (http://geomag.usgs.gov/)
Career crate: Seismic processor
(http://careercrate.com/video/266/Seismic-processor)
Society of Exploration Geophysicists (http://www.seg.org/)
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