STEINERT Magnetic Drum
... drum going in the same direction, the flow is easy to handle and ferrous losses are small. Even when the material is large, small or mixed, the size of the particles usually determines the diameter of the drum. ...
... drum going in the same direction, the flow is easy to handle and ferrous losses are small. Even when the material is large, small or mixed, the size of the particles usually determines the diameter of the drum. ...
VIII. NUCLEAR MAGNETIC RESONANCE (NMR) SPECTROSCOPY
... F:\Attila\Osszesitett\WORD\Oktatas\Eloadasok\ElméletiKémiaI-Angol\Week6.docx ...
... F:\Attila\Osszesitett\WORD\Oktatas\Eloadasok\ElméletiKémiaI-Angol\Week6.docx ...
understanding electromagnetism: a new approach
... There are similarly several questions, to which the above concept of creation of magnetic fields due to the spin and orbital motions of the charge of electron give rise. These questions raise serious question mark over the truth of the above concept. The electron cannot have m s and a magnetic field ...
... There are similarly several questions, to which the above concept of creation of magnetic fields due to the spin and orbital motions of the charge of electron give rise. These questions raise serious question mark over the truth of the above concept. The electron cannot have m s and a magnetic field ...
Magnetism Magnetism
... Some materials can be made into permanent magnets Some substances, such as lodestones, are magnetic all the time. These types of magnets are called permanent magnets. You can change any piece of iron, such as a nail, into a permanent magnet by stroking it several times with a permanent magnet. A slo ...
... Some materials can be made into permanent magnets Some substances, such as lodestones, are magnetic all the time. These types of magnets are called permanent magnets. You can change any piece of iron, such as a nail, into a permanent magnet by stroking it several times with a permanent magnet. A slo ...
Magnet
... The Two Models for Magnets: Magnetic Poles and Atomic Currents Magnetic pole model. Although for many purposes it is convenient to think of a magnet as having distinct north and south magnetic poles, the concept of poles should not be taken literally: it is merely a way of referring to the two diffe ...
... The Two Models for Magnets: Magnetic Poles and Atomic Currents Magnetic pole model. Although for many purposes it is convenient to think of a magnet as having distinct north and south magnetic poles, the concept of poles should not be taken literally: it is merely a way of referring to the two diffe ...
Magnets and Magnetic Fields
... The importance of language can be demonstrated when talking about magnetic fields it is helpful for learners to realise that when they place their compass in a magnetic field the North Pole of that compass will experience a force of attraction. To help avoid the previously mentioned misconception th ...
... The importance of language can be demonstrated when talking about magnetic fields it is helpful for learners to realise that when they place their compass in a magnetic field the North Pole of that compass will experience a force of attraction. To help avoid the previously mentioned misconception th ...
Physics, Chapter 29: The Magnetic Field
... is given by the magnitude of the force on a unit north pole, and whose direction is the direction of the force on a north pole. Algebraically, it is conventional to represent a north pole as a positive pole and a south pole as a negative pole. In cgs emu the force is stated in dynes, the pole streng ...
... is given by the magnitude of the force on a unit north pole, and whose direction is the direction of the force on a north pole. Algebraically, it is conventional to represent a north pole as a positive pole and a south pole as a negative pole. In cgs emu the force is stated in dynes, the pole streng ...
Physics, Chapter 29: The Magnetic Field
... is given by the magnitude of the force on a unit north pole, and whose direction is the direction of the force on a north pole. Algebraically, it is conventional to represent a north pole as a positive pole and a south pole as a negative pole. In cgs emu the force is stated in dynes, the pole streng ...
... is given by the magnitude of the force on a unit north pole, and whose direction is the direction of the force on a north pole. Algebraically, it is conventional to represent a north pole as a positive pole and a south pole as a negative pole. In cgs emu the force is stated in dynes, the pole streng ...
Static Airgap Magnetic Field of Axial Flux Permanent Magnet Disk
... heat dissipation, high efficiency, obviously energy saving effect, high torque - inertia ratio and power density and so on [1, 2], especially the size and weight of which is about 50% of the ordinary permanent magnet motor, is especially suitable for occasions demanding small size, low weight the lo ...
... heat dissipation, high efficiency, obviously energy saving effect, high torque - inertia ratio and power density and so on [1, 2], especially the size and weight of which is about 50% of the ordinary permanent magnet motor, is especially suitable for occasions demanding small size, low weight the lo ...
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.