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Presentation - ScienceScene
Presentation - ScienceScene

... 2. Hold the laser 2 meters from the surface. Align the same square with one side and bottom. Determine the number of original squares it would take to fill the larger square. 3. Hold the laser 3 meters from the surface. Align the same square with one side and bottom. Determine the number of original ...
Magnetism
Magnetism

Supplement to Activity 9: A Soda Bottle Magnetometer
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... of automobiles on nearby road surfaces can perturb the local magnetic field in much the same way as a magnetic storm, although the time scale for the disturbance is very much shorter than for an actual storm. Metal detectors measure the same kinds of deviations caused by ferro-magnetic substances. W ...
Evolution of Rising Magnetic Cavities and UHECR acceleration
Evolution of Rising Magnetic Cavities and UHECR acceleration

magnet
magnet

Magnetism PowerPoint Template
Magnetism PowerPoint Template

... The Cause of Magnetism • As electrons in atoms move around, a magnetic field is generated. The atom will then have a north and south pole. • The atoms group together in tiny areas called domains. Each domain is like a tiny magnet. • In most materials, such as copper and aluminum, the magnetic field ...
Magnetism - Cobb Learning
Magnetism - Cobb Learning

... The Cause of Magnetism • As electrons in atoms move around, a magnetic field is generated. The atom will then have a north and south pole. • The atoms group together in tiny areas called domains. Each domain is like a tiny magnet. • In most materials, such as copper and aluminum, the magnetic field ...
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... Find the field at a point at distance r from the center of the toroid The toroid has N turns of wire ...
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Concerning long-term geomagnetic variations and space climatology

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Processing Electroceramics - Universiti Sains Malaysia

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Magnetic Modelling – basic concepts

... subjected to an applied magnetic field (in this case the applied field equals the earth magnetic field). Some rocks may, apart from the induced magnetization, also carry a “permanent” magnetization, termed remanence. The remanent magnetization is similar to a standard magnet and can be described by ...
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... interaction of a moving charged object or a magnet with other moving charged objects or another magnet. a. Magnetic dipoles have “north” and “south” polarity. b. The magnetic dipole moment of an object has the tail of the magnetic dipole moment vector at the south end of the object and the head of t ...
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Slide 1

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Summary Magnetic materials 2015. The magnetic susceptibility, i.e. 

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... widely studied. Observations(Feynman & Martin) suggest that the emerging flux has a strong connection with CMEs. As a interpretation to understand both of the results of the theories and the observations, we suggest that the dynamical motion such as a conversing one may be due to the emergence of th ...
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... A cross-sectional view of a coaxial cable is shown. The center conductor is surrounded by a rubber layer, which is surrounded by an outer conductor, which is surrounded by another rubber layer. In a particular application, the current in the inner conductor is 1.00 A out of the page and the current ...
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Adobe Acrobat file () - Wayne State University Physics and

Experimental studies on ion acceleration and stream line
Experimental studies on ion acceleration and stream line

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What is a magnet?

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Magnetosphere of Jupiter



The magnetosphere of Jupiter is the cavity created in the solar wind by the planet's magnetic field. Extending up to seven million kilometers in the Sun's direction and almost to the orbit of Saturn in the opposite direction, Jupiter's magnetosphere is the largest and most powerful of any planetary magnetosphere in the Solar System, and by volume the largest known continuous structure in the Solar System after the heliosphere. Wider and flatter than the Earth's magnetosphere, Jupiter's is stronger by an order of magnitude, while its magnetic moment is roughly 18,000 times larger. The existence of Jupiter's magnetic field was first inferred from observations of radio emissions at the end of the 1950s and was directly observed by the Pioneer 10 spacecraft in 1973.Jupiter's internal magnetic field is generated by electrical currents in the planet's outer core, which is composed of liquid metallic hydrogen. Volcanic eruptions on Jupiter's moon Io eject large amounts of sulfur dioxide gas into space, forming a large torus around the planet. Jupiter's magnetic field forces the torus to rotate with the same angular velocity and direction as the planet. The torus in turn loads the magnetic field with plasma, in the process stretching it into a pancake-like structure called a magnetodisk. In effect, Jupiter's magnetosphere is shaped by Io's plasma and its own rotation, rather than by the solar wind like Earth's magnetosphere. Strong currents in the magnetosphere generate permanent aurorae around the planet's poles and intense variable radio emissions, which means that Jupiter can be thought of as a very weak radio pulsar. Jupiter's aurorae have been observed in almost all parts of the electromagnetic spectrum, including infrared, visible, ultraviolet and soft X-rays.The action of the magnetosphere traps and accelerates particles, producing intense belts of radiation similar to Earth's Van Allen belts, but thousands of times stronger. The interaction of energetic particles with the surfaces of Jupiter's largest moons markedly affects their chemical and physical properties. Those same particles also affect and are affected by the motions of the particles within Jupiter's tenuous planetary ring system. Radiation belts present a significant hazard for spacecraft and potentially to human space travellers.
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