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Chapter 28 – Sources of Magnetic Field
Chapter 28 – Sources of Magnetic Field

... - Strong interactions between atomic magnetic moments cause them to align parallel to each other in regions (magnetic domains) even when no Bext is present. Ex: Fe, Co. - If no Bext  domain magnetizations are randomly ...
What is a magnet?
What is a magnet?

I Basic Spin Physics
I Basic Spin Physics

... out of atoms, which are made out of electrons orbiting a nucleus (made out of protons and neutrons). It is possible to further subdivide matter, but we shall stop at this level and treat the electron, proton and neutron as elementary point ...
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magnetic field

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Notes on Magnetism
Notes on Magnetism

... became important for us to measure pole strength, it is very much important for us to measure magnetic field because at different points the magnetic forces are different.The question how much is the field is more important than whether field exists or not. We quantify the magnetic field as follows: ...
Magnetic Properties Introduction
Magnetic Properties Introduction

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magnetism

... ©2010, The McGraw-Hill Companies, Inc. ...
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Chapter 22: Magnetism

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The Magnetic Field of a Permanent Magnet

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2.3 Gyromagnetic Ratio - McMaster Physics and Astronomy

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... material has the ability to create internal Dipole moment . For this reason this kinds of material present special type of properties. Some common characteristics of this material is … 1. attracting other magnetic material. 2. Inducing pole in this material . 3. The polarity of two pole are opposite ...
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Forces on Current Carrying Wires in Magnetic Fields

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MAGNETIC EFFECTS OF CURRENT & MAGNETISM (Important formulae & concepts)

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... On September 11, 1820 Ampere heard of H. C. Ørsted's discovery that a magnetic needle is acted on by a voltaic current. Only a week later, on September 18, he presented a paper containing a far more complete exposition of that and other phenomena. The SI unit of measurement of electric current, the ...
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Magnetic Resonance TOPIC 3

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6 - Enea Frascati

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5_2_Magnetism basics

... When a magnetic field H is applied, an electron can only flip its spin magnetic dipole from anti-parallel to parallel if the decrease in its magnetic energy (2βH) is sufficient to supply the extra kinetic energy required to raise it to an empty translational energy level. (RECALL: β is the Bohr magn ...
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Magnetism Review

... Explanation: A force is exerted on charged particles only when they move at an angle to magnetic field lines. The force is greatest when motion is at right angles to the magnetic field. ...
Magnetic coupling in the solar system
Magnetic coupling in the solar system

Answers for Student notes page
Answers for Student notes page

Subject: Teacher Grade Level Length of Lesson
Subject: Teacher Grade Level Length of Lesson

... electromagnet is directly related to the number of coils of wire wrapped around their nail. ...
< 1 ... 10 11 12 13 14 15 16 17 18 ... 42 >

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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