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Paleomagnetics and Marine Oxygen Isotope
Paleomagnetics and Marine Oxygen Isotope

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Magnetism and Electricity

... when all the electrons spin in the same direction. When you bring two magnets together they exert a push or pull called a magnetic force. This force results from spinning electric charges of electrons in the magnet. The force can either push magnets apart, or pull them together. Magnetic force is on ...
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... Using a divertor the particles that leave the plasma flow along the magnetic field and hit the target plates These plates are far away from the plasma such that any impurity released at the plate has a smaller chance ending up in the plasma Furthermore, one can try to cool the plasma further through ...
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... Using a divertor the particles that leave the plasma flow along the magnetic field and hit the target plates These plates are far away from the plasma such that any impurity released at the plate has a smaller chance ending up in the plasma Furthermore, one can try to cool the plasma further through ...
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Chapter 64: The Magnetic Moment of the Electron

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Magnetism - Mr. Treon

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The Measurement of a Magnetic Field in Fundamental Units

... to the field while the sides are parallel to it only the end will be subject to a force from the field. We can measure the force on the end of the loop by balancing it with a known weight hung from the other end of the balance. In this lab, we wish to determine B, the magnetic field of the solenoid; ...
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Practice Quiz (Ch 24) 1) The source of all magnetism is A) tiny

... C) only an electric field. D) none of these Answer: A 3) If a steady magnetic field exerts a force on a moving charge, that force is directed A) in the direction of the field. B) opposite the direction of the field. C) at right angles to the direction of the field. Answer: C 4) Like kinds of magneti ...
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5H10.11 - Compass Needles and Magnet

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The Earth is a magnet

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Magnetosphere of Saturn



The magnetosphere of Saturn is the cavity created in the flow of the solar wind by the planet's internally generated magnetic field. Discovered in 1979 by the Pioneer 11 spacecraft, Saturn's magnetosphere is the second largest of any planet in the Solar System after Jupiter. The magnetopause, the boundary between Saturn's magnetosphere and the solar wind, is located at a distance of about 20 Saturn radii from the planet's center, while its magnetotail stretches hundreds of radii behind it.Saturn's magnetosphere is filled with plasmas originating from both the planet and its moons. The main source is the small moon Enceladus, which ejects as much as 1,000 kg/s of water vapor from the geysers on its south pole, a portion of which is ionized and forced to co-rotate with the Saturn’s magnetic field. This loads the field with as much as 100 kg of water group ions per second. This plasma gradually moves out from the inner magnetosphere via the interchange instability mechanism and then escapes through the magnetotail.The interaction between Saturn's magnetosphere and the solar wind generates bright oval aurorae around the planet's poles observed in visible, infrared and ultraviolet light. The aurorae are related to the powerful saturnian kilometric radiation (SKR), which spans the frequency interval between 100 kHz to 1300 kHz and was once thought to modulate with a period equal to the planet's rotation. However, later measurements showed that the periodicity of the SKR's modulation varies by as much as 1%, and so probably does not exactly coincide with Saturn’s true rotational period, which as of 2010 remains unknown. Inside the magnetosphere there are radiation belts, which house particles with energy as high as tens of megaelectronvolts. The energetic particles have significant influence on the surfaces of inner icy moons of Saturn.In 1980–1981 the magnetosphere of Saturn was studied by the Voyager spacecraft. As of 2010 it is a subject of the ongoing investigation by Cassini mission, which arrived in 2004.
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