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DICTIONARY OF GEOPHYSICS, ASTROPHYSICS, and ASTRONOMY

DICTIONARY OF GEOPHYSICS, ASTROPHYSICS, and ASTRONOMY

DICTIONARY OF GEOPHYSICS, ASTROPHYSICS, and ASTRONOMY

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or more km where the magma resides before an<br />

eruption occurs <strong>and</strong> it ascends to the surface.<br />

magmatic water Water that forms in phase<br />

separation from magma. This water carries<br />

large amounts of dissolved minerals which it deposits<br />

in veins as it travels to the surface of the<br />

Earth. Also called juvenile water.<br />

magnetic anomaly The local deviation of<br />

the geomagnetic field from the global field generated<br />

by the dynamo in the core <strong>and</strong> the external<br />

field, due to the magnetization of nearby<br />

crust. This is usually obtained by measuring<br />

the local magnetic field <strong>and</strong> then subtracting the<br />

prediction of a global field model such as an<br />

IGRF. Crustal rock may be magnetized in situ<br />

after a heating event by cooling down through<br />

its Curie temperature in the ambient magnetic<br />

field of the Earth, or else magnetized particles<br />

may be oriented on or after deposition in a sedimentary<br />

environment by the Earth’s field so that<br />

the rock is left with net magnetization. Magnetic<br />

anomalies in oceanic plate show reversals<br />

in magnetization as one travels perpendicular to<br />

the mid-ocean ridge that produced them, due to<br />

the occasional reversal of the Earth’s magnetic<br />

fieldsothatrockthatcoolsatdifferenttimesmay<br />

have oppositely oriented magnetization. This<br />

provided evidence for the hypothesis of sea floor<br />

spreading. Continental anomalies may be associated<br />

with geological structures such as subductionorcollisionzonesorvolcanos,<br />

wherethe<br />

crust has been heated. Many anomalies, including<br />

one at Bangui in Africa, are large enough to<br />

be detected through satellite magnetic measurements.<br />

magnetic bay A dip in the trace of a highlatitude<br />

magnetogram, resembling a bay in a<br />

shoreline. Magnetic bays observed this way<br />

in the 1950s <strong>and</strong> earlier were later identified as<br />

magnetic substorms.<br />

magnetic carpet The distribution of magnetic<br />

field in small scales over the quiet sun<br />

which is observed to be recycled over a period<br />

of 40 h. A discovery of the Michelson Doppler<br />

Imager on the SOHO spacecraft.<br />

© 2001 by CRC Press LLC<br />

magnetic field<br />

magnetic cloud The interplanetary counterparts<br />

of coronal mass ejections (CMEs) that exhibit<br />

the topology of helical magnetic flux ropes.<br />

Magnetic clouds make up about one third of all<br />

solar wind streams that are identified as interplanetary<br />

consequences of CMEs.<br />

magnetic crochet Accompanying a solar<br />

flare, dayside magnetic fields may show a sharp<br />

change, called a crochet, starting with the flare,<br />

but shorter-lived, due to electric currents set up<br />

in the lower ionosphere as a result of the flare induced<br />

ionization <strong>and</strong> conductivity changes. See<br />

short wave fadeout.<br />

magnetic declination The azimuth, measured<br />

from geographic north, of the geomagnetic<br />

field vector at a given location.<br />

magnetic diffusivity A measure of the ability<br />

of a magnetic field to diffuse out of a volume<br />

of plasma. A perfectly conducting plasma has<br />

zero magnetic diffusivity. The solar atmosphere<br />

has a magnetic diffusivity comparable to that<br />

of copper wire. However, because of the large<br />

scales involved on the sun, compared to the typical<br />

length of a copper wire, the diffusion times<br />

are extremely long.<br />

magnetic dipole The simplest source of a<br />

magnetic field envisaged to consist of two magnetic<br />

poles of equal strengths but opposite signs<br />

a small distance apart. The first-order geomagnetic<br />

field is a dipole field.<br />

magnetic field In general, the conceptualization<br />

due to Faraday, <strong>and</strong> rigorized by Maxwell<br />

of the laws relating the magnetic forces between<br />

current loops (or fictitious magnetic monopoles)<br />

as embodied in a space-filling collection of vectors<br />

(a field) which collectively define magnetic<br />

flux tubes. In geophysics, the magnetic of the<br />

Earth or of other planets. On Earth, the field is<br />

closely approximated by that of a dipole. The<br />

north <strong>and</strong> south magnetic poles are relatively<br />

close to the geographic poles. The magnetic<br />

field is generated by dynamo processes in the<br />

Earth’s liquid, iron-rich core. The rotation of<br />

the Earth plays an important role in the generation<br />

of the magnetic field <strong>and</strong> this is the reason<br />

for the close proximity of the magnetic <strong>and</strong> ge-<br />

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