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Wednesday, March 20, 2013

Magnetic hysteresis (2)

Theoretical model of magnetization m against magnetic field h. Starting at the origin, the upward curve is the initial magnetization curve. The downward curve after saturation, along with the lower return curve, form the main loop. The intercepts hc and mrs are the coercivity and saturation remanence.
When an external magnetic field is applied to a ferromagnet such as iron, the atomic dipoles align themselves with it. Even when the field is removed, part of the alignment will be retained: the material has become magnetized. Once magnetized, the magnet will stay magnetized indefinitely. To demagnetize it requires heat or a magnetic field in the opposite direction. This is the effect that provides the element of memory in a hard disk drive.
The relationship between field strength H and magnetization M is not linear in such materials. If a magnet is demagnetized (H=M=0) and the relationship between H and M is plotted for increasing levels of field strength, M follows the initial magnetization curve. This curve increases rapidly at first and then approaches an asymptote called magnetic saturation. If the magnetic field is now reduced monotonically,M follows a different curve. At zero field strength, the magnetization is offset from the origin by an amount called the remanence. If the H-M relationship is plotted for all strengths of applied magnetic field the result is a hysteresis loop called the main loop. The width of the middle section is twice the coercivity of the material.[16]
A closer look at a magnetization curve generally reveals a series of small, random jumps in magnetization called Barkhausen jumps. This effect is due to crystallographic defects such as dislocations.[17]
Magnetic hysteresis loops are not exclusive to materials with ferromagnetic ordering. Other magnetic orderings, such as spin glass ordering, also exhibit this phenomena.[18]



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Saturday, March 9, 2013

Reference Natural Events to GSHL (5)



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New High-Intensity Cosmic Explosion (Reference for GSHL Experiment)




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Nikola Tesla (Courtesy Of Hystory Channel)



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Nikola Tesla (Courtesy of History)



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Rotary magnetic fields



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Electromagnetic Rail Gun Simulation



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Simulations of Core Collapse Supernovae (Natural Events Reference for GSHL Experiment))



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Supernova Simulation (Cosmic Magnetic Events for Reference to GSHL Experiment))



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Type-II Supernova (Space Magnetic Events)



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A simulation of magnetic field outflows from active galactic nuclei (Space Magnetic Events)


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Wednesday, March 6, 2013

Lopez's Teragaussian Ejection Speed Calculation


Lopez´s Ejeccion Speed Calculation


Speed Ejection Constants:
Q(exp) :  4.2 x 10E15 [J]
T :  6.0 x 10E6   [K] or 0.5 [keV]
p : 3.14159264
µ : 4p x 10E-7 [TmA]
Insert Vehicle Weigh   [Kg]:
Insert Coil Helix Number   : 
Insert Coil Long [m] :           
Insert Conductor Cross Section Area [m2]: