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Journal ArticleDOI

Geomagnetic field variations

R. P. Kane
- 01 Feb 1976 - 
- Vol. 18, Iss: 4, pp 413-540
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TLDR
In this article, an attempt has been made to describe the large variety of geomagnetic variations, both regular and irregular, both with a brief description of the Earth and its environment, different types of quiet-day variations are described and present ideas regarding their possible mechanisms.
Abstract
In this review, an attempt has been made to describe the large variety of geomagnetic variations, both regular and irregular. After a brief description of the Earth and its environment, different types of quiet-day variations are described and present ideas regarding their possible mechanisms are discussed. In general, periodicities exceeding several tens of years can be attributed to changes in the interior of the Earth while periodicities of 22 years or less seem to be related to phenomena connected with the Sun, through the interaction of solar wind with the Earth's magnetosphere. The morphology of irregular storm-time variations and its relationship with interplanetary plasma parameters is discussed with particular reference to the orientations of interplanetary magnetic field, particularly the southward B z component which seems to play a crucial role. Various storm-time phenomena occurring in the polar, auroral, mid-latitude and equatorial regions and their interconnections are described. Theoretical models offering explanations of many of these phenomena are discussed, the unsolved problems are outlined, and the direction of the present effort in solving these is indicated.

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Citations
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Journal ArticleDOI

The ionospheric disturbance dynamo

TL;DR: In this article, a numerical simulation study of the thermospheric winds produced by auroral heating during magnetic storms, and of their global dynamo effects, establishes the main features of the ionospheric disturbance dynamo.
Journal ArticleDOI

Dynamo Scaling Laws and Applications to the Planets

TL;DR: The scaling laws for planetary dynamos relate the characteristic magnetic field strength, characteristic flow velocity and other properties to primary quantities such as core size, rotation rate, electrical conductivity and heat flux as discussed by the authors.
Journal ArticleDOI

On the genesis of the Earth's magnetism

TL;DR: The geophysical relevance of the experiments and simulations is called into question: the dynamics of Earth's core are too complex, and operate across time and length scales too broad to be captured by any single laboratory experiment, or resolved on present-day computers.
Journal ArticleDOI

The equatorial counter-electrojet—a review of its geomagnetic aspects

TL;DR: In this paper, the equatorial counter-electrojet corresponds to a westward flow of currents within a narrow latitude band on either side of the dip-equator and negative depressions of the regular daily variation SR in the horizontal component which it induces at these latitudes can be considered as an unexpected and abnormal reversal of the SR.
Book ChapterDOI

Solar-Terrestrial Physics

V. L. Patel
TL;DR: The geomagnetic field at various latitudes and longitudes of the Earth has been studied also in space with the advent of rockets and satellites as discussed by the authors, where magnetic observatories monitor continuously the geomagnetism.
References
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Book

Atmospheric Tides

Book

Coronal Expansion and Solar Wind

TL;DR: In this paper, an alternative model of the Coronal expansion of the solar magnetic field was proposed, based on a one-fluid and two fluid models of the coronal expansion.
Book

The polar aurora

Carl Störmer
Journal ArticleDOI

World-Wide Correlation of Mesozoic Magnetic Anomalies, and Its Implications

TL;DR: In this article, the authors derived a magnetic reversal model for the Hawaiian lineation set and used this model to correlate the entire Hawaiian and Keathley lineation sets to the entire North Atlantic.
Journal ArticleDOI

Thermally driven diurnal tide in the atmosphere

TL;DR: The theory for the diurnal tide in the atmosphere is reviewed and the appropriate Hough Functions (including those with negative equivalent depths) are described in this article, where the main thermal drives for the durnal tide are described and the theory is then used to compute the atmosphere's response to the thermal drives.
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