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Magnetic dipole moment
Magnetic dipole moment

The Magnetic Field of a Permanent Magnet
The Magnetic Field of a Permanent Magnet

... 2. How well does the inverse-cube model fit your experimental data? From the comparison, does your magnet show the magnetic field pattern of a dipole? 3. The computer adjusted the parameter A so the equation’s curve comes as close as possible to your data points. Relating the parameter A to the fiel ...
Jovian Planets
Jovian Planets

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... – Due Wednesday, April 28 – Problem 5, HW 1 is a good starting point for the lab questions – Note typo in Question 3 - “Jupiter” => “Saturn” ...
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... compared the process to the drying of an apple. Lord Kelvin (19th C) suggested that contraction was due to cooling of the Earth. The problems with this mechanism: •Fossils are preserved in rocks that represent organisms that could not withstand the early temperatures. •Initial temperatures required ...
Continental drift: the history of an idea
Continental drift: the history of an idea

... compared the process to the drying of an apple. Lord Kelvin (19th C) suggested that contraction was due to cooling of the Earth. The problems with this mechanism: •Fossils are preserved in rocks that represent organisms that could not withstand the early temperatures. •Initial temperatures required ...
Continental Drift
Continental Drift

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ETPD: The Facts and The FAQs
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... What happens to my compass in the southern hemisphere? For a compass to work properly, the compass needle must be free to rotate and align with the magnetic field. The difference between compasses designed to work in the northern and southern hemispheres is simply the location of the “balance”, a we ...
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Magnetism - SchoolRack

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A brief review of double-pulsar system PSR J0737-3039
A brief review of double-pulsar system PSR J0737-3039

... Synchrotron absorption model Since A’s luminosity is about 3000 times greater than B, A’s pulsar wind likely blow away B’s magnetosphere. The bow shock compress magnetosheath wind plasma, leading to magnetopause a sharp jump in plasma density and temperature. → synchrotron absorption. A ...
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Rad 160 – Radiographic Physics Unit 4 Magnetism I. Magnetism A

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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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