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The physics of the strongly driven m...

Merkine, Viatcheslav G.

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The physics of the strongly driven magnetosphere: Global MHD modeling.

Record Type:	Electronic resources : Monograph/item
Title/Author:	The physics of the strongly driven magnetosphere: Global MHD modeling./
Author:	Merkine, Viatcheslav G.
Description:	173 p.
Notes:	Source: Dissertation Abstracts International, Volume: 64-12, Section: B, page: 6139.
Contained By:	Dissertation Abstracts International64-12B.
Subject:	Physics, Fluid and Plasma. -
Online resource:	http://pqdd.sinica.edu.tw/twdaoapp/servlet/advanced?query=3114756
ISBN:	0496622455

The physics of the strongly driven magnetosphere: Global MHD modeling.
Merkine, Viatcheslav G.

The physics of the strongly driven magnetosphere: Global MHD modeling. - 173 p.

Source: Dissertation Abstracts International, Volume: 64-12, Section: B, page: 6139.

Thesis (Ph.D.)--University of Maryland, College Park, 2004.

This study examines the behavior of the earth's magnetosphere under extreme solar wind conditions using global magnetohydrodynamic (MHD) simulations. Particular emphasis is placed on the phenomenon of the cross polar cap potential (CPCP) saturat

ISBN: 0496622455Subjects--Topical Terms:

1018402
Physics, Fluid and Plasma.

The physics of the strongly driven magnetosphere: Global MHD modeling.
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020 $a 0496622455
035 $a (UnM)AAI3114756
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040 $a UnM $c UnM
100 1 $a Merkine, Viatcheslav G. $3 1933875
245 1 4 $a The physics of the strongly driven magnetosphere: Global MHD modeling.
300 $a 173 p.
500 $a Source: Dissertation Abstracts International, Volume: 64-12, Section: B, page: 6139.
500 $a Chair: Konstantinos (Dennis) Papadopoulos.
502 $a Thesis (Ph.D.)--University of Maryland, College Park, 2004.
520 $a This study examines the behavior of the earth's magnetosphere under extreme solar wind conditions using global magnetohydrodynamic (MHD) simulations. Particular emphasis is placed on the phenomenon of the cross polar cap potential (CPCP) saturat
520 $a Global MHD simulations are a natural tool to study the phenomenon of the CPCP saturation. Despite the lack of proper microscopic shock and reconnection physics, such models reproduce many global phenomena in the SW-M-I system and its geometry. A
520 $a A series of simulations with idealized solar wind and ionosphere was conducted to study the dependence of the CPCP on the IEF and ionospheric conductance in a wide range of values. The simulations confirmed the CPCP saturation, but the level of
520 $a As a result of these studies a phenomenological model of the CPCP saturation was formulated. The main building blocks of this model are the direct amplifying effect of the solar wind electric field and the adverse feedback of the ionospheric con
590 $a School code: 0117.
650 4 $a Physics, Fluid and Plasma. $3 1018402
650 4 $a Physics, Atmospheric Science. $3 1019431
650 4 $a Physics, Electricity and Magnetism. $3 1019535
690 $a 0759
690 $a 0608
690 $a 0607
710 2 0 $a University of Maryland, College Park. $3 657686
773 0 $t Dissertation Abstracts International $g 64-12B.
790 1 0 $a Papadopoulos, Konstantinos (Dennis), $e advisor
790 $a 0117
791 $a Ph.D.
792 $a 2004
856 4 0 $u http://pqdd.sinica.edu.tw/twdaoapp/servlet/advanced?query=3114756