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Continental Drift Continental Drift Continental Drift
Continental Drift Continental Drift Continental Drift

... freely-floating magnetic object will align with Earth’s magnetic field.  When lava cools to a temperature called the Curie point, magnetic minerals in the lava are frozen in a direction determined by Earth’s magnetic poles. – At the poles, the orientation of the minerals will be vertical – At the e ...
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... Alka could not believe her eyes that such a colorful display like the one during commonwealth games could be created by nature. She went to the library, but could not find the right book. So she consulted her teacher who guided her. Hence, Alka understood that during a solar flare, a large number of ...
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... 22. [2] Touch the ends of the rods together. The rod that doesn’t stick to either of the other rods is brass. As it is now identified, set it aside. The other two rods can be identified by touching the end of either rod to the center of the other. If there is a strong attraction, then the rod that w ...
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... What is Electromagnetism? • Electromagnetism is one of the four fundamental interactions of nature, along with strong interaction, weak interaction and gravitation. It is the force that causes the interaction between electrically charged particles; the areas in which this happens are called electro ...
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... flowing in it will create a magnetic field  The strength of the magnetic field depends on  The amount of current in a wire – More current means stronger magnetic field  The number of turns in the coil – More turns means stronger magnetic field  The material in the coil – Magnetic materials like ...
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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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