THE PHYSICS OF THE STRONGLY DRIVEN MAGNETOSPHERE: GLOBAL MHD MODELING

منو

" THE PHYSICS OF THE STRONGLY DRIVEN MAGNETOSPHERE: GLOBAL MHD MODELING "

Document Type	:	Latin Dissertation
Language of Document	:	English
Record Number	:	149816
Doc. No	:	ET21608
Main Entry	:	Viatcheslav G. Merkine
Title Proper	:	THE PHYSICS OF THE STRONGLY DRIVEN MAGNETOSPHERE: GLOBAL MHD MODELING
Note	:	This document is digital این مدرک بصورت الکترونیکی می باشد
Abstract	:	This study examines the behavior of the earthبs magnetosphere under extremesolar wind conditions using global magnetohydrodynamic (MHD) simulations.Particular emphasis is placed on the phenomenon of the cross polar cap potential(CPCP) saturation. The eض‍ect refers to the tendency of the potential to level oض‍instead of growing linearly as the interplanetary electric field (IEF) increases.The CPCP is an important indicator of the coupling in the solarwind-magnetosphere-ionosphere (SW-M-I) system since it is mapped along theequipotential magnetic field lines from the dayside reconnection line. Due to theCPCP saturation a large amount of the solar wind energy is prevented fromdirectly accessing the ionosphere which limits the ionospheric response to thesolar wind driver.tested for theQ1 PC1 bus cardBoth these projects mere sofixare des elopment efforts tonards contributing to dlfferentaspects of Roboucs and lZ1echatronics projects m the Controls and Roboucs Group..
Subject	:	Electericl tess
	:	برق
electronic file name	:	TL44783.pdf
Title and statement of responsibility and	:	THE PHYSICS OF THE STRONGLY DRIVEN MAGNETOSPHERE: GLOBAL MHD MODELING [Thesis]