geomagnetic$31379$ - definizione. Che cos'è geomagnetic$31379$
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Cosa (chi) è geomagnetic$31379$ - definizione

Geomagnetic variations

Geomagnetic pole         
  • Illustration of the difference between geomagnetic poles (N<sub>m</sub> and S<sub>m</sub>) and geographical poles (N<sub>g</sub> and S<sub>g</sub>)
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ONE OF TWO ANTIPODAL POINTS IN THE ARCTIC AND IN THE ANTARCTIC WHERE THE AXIS OF A BEST-FITTING DIPOLE INTERSECTS THE SURFACE OF EARTH
Geomagnetic North Pole; Geomagnetic north pole; North geomagnetic pole; Geomagnetic Pole; Geomagnetic poles; South geomagnetic pole
The geomagnetic poles are antipodal points where the axis of a best-fitting dipole intersects the surface of Earth. This theoretical dipole is equivalent to a powerful bar magnet at the center of Earth, and comes closer than any other point dipole model to describing the magnetic field observed at Earth's surface.
Geomagnetic excursion         
A geomagnetic excursion, like a geomagnetic reversal, is a significant change in the Earth's magnetic field. Unlike reversals, an excursion is not a "permanent" re-orientation of the large-scale field, but rather represents a dramatic, typically a (geologically) short-lived change in field intensity, with a variation in pole orientation of up to 45° from the previous position.
Boulder Geomagnetic Observatory         
GEOMAGNETIC OBSERVATION FACILITY NEAR BOULDER, COLORADO, UNITED STATES
Boulder (BOU) Geomagnetic Observatory
Boulder Geomagnetic Observatory (BOU) is a geomagnetic observation facility operated by the United States Geological Survey (USGS). It is located near Boulder, Colorado at .

Wikipedia

Geomagnetic excursion

A geomagnetic excursion, like a geomagnetic reversal, is a significant change in the Earth's magnetic field. Unlike reversals, an excursion is not a "permanent" re-orientation of the large-scale field, but rather represents a dramatic, typically a (geologically) short-lived change in field intensity, with a variation in pole orientation of up to 45° from the previous position.

Excursion events typically only last a few thousand to a few tens of thousands of years, and often involve declines in field strength to between 0 and 20% of normal. Unlike full reversals, excursions are generally not recorded around the entire globe. This is certainly due in part to them not registering well in the sedimentary record, but it also seems likely that excursions may not typically extend through the entire global geomagnetic field. There are significant exceptions, however.