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Magnets and Magnetism
Magnets and Magnetism

... All matter is made of atoms. Electrons are negatively charged particles of atoms. As an electron moves around, it makes, or induces, a magnetic field. The atom will then have a north and a south pole. In most materials, such as copper and aluminum, the magnetic fields of the individual atoms cancel ...
Magnetism Unit
Magnetism Unit

... 1. Define magnetism as a force that attracts iron, nickel or cobalt. 2. State that magnetic force is invisible. 3. Identify magnets as either bar or horseshoe based on shape. 4. Name the poles of magnets as north or south. 5. Given a drawing of a magnet, draw lines representing magnetic force lines. ...
The Earth`s Magnetic Field
The Earth`s Magnetic Field

2 Solar magnetic fields. - High Altitude Observatory
2 Solar magnetic fields. - High Altitude Observatory

... 1610. It was not until 1908 that Hale proved that the spots were concentrations of strong magnetic fields, but his discovery meant that spots could then be used to probe solar magnetism back to the early 1600s, the time of Galileo. Sunspots generally appear benign to the naked eye- so why should hum ...
Earth Communication
Earth Communication

Earth Communication
Earth Communication

PowerPoint - GeoWeb
PowerPoint - GeoWeb

bution of Solar Proton Events Affecting the Earth E
bution of Solar Proton Events Affecting the Earth E

contributed talk in splinter session
contributed talk in splinter session

Which of the following is a vector quantity?
Which of the following is a vector quantity?

... wire as shown. Recall that magnetic field lines point away from a north pole and toward a south pole. If the positive direction of the induced current I in the loop is as shown by the arrows on the loop, the variation of I with time as the bar magnet falls through the loop is illustrated qualitative ...
Electromagnetic Induction
Electromagnetic Induction

STELLAR ABLATION OF PLANETARY ATMOSPHERES
STELLAR ABLATION OF PLANETARY ATMOSPHERES

21.2 Electromagnetism
21.2 Electromagnetism

... fingers are oriented for a positive current and its magnetic field. Then, have students adapt the rule for positive charges moving in a magnetic field, as shown in Figure 8 (that is, the thumb points in the direction of the moving charge, the fingers extend in the direction of the magnetic field, an ...
Effect of the geomagnetic field on the intensity of sodium laser guide
Effect of the geomagnetic field on the intensity of sodium laser guide

Magnetism - WordPress.com
Magnetism - WordPress.com

... The initial story and description sets the discovery of lodestones which set the way for the modern term magnets as being derived from the area where lodestones were mined in Magnesia. The students should also know that here lodestones found their initial use as a compass, where travelers would take ...
360 Degree Angle Sensor Using Spin Valve
360 Degree Angle Sensor Using Spin Valve

Vlasov simulations of trapping and loss of auroral electrons
Vlasov simulations of trapping and loss of auroral electrons

... double layer position is possible when electrons are accelerated into a stronger magnetic field. Ergun et al. (2000b) used a static model to find solutions to the Vlasov–Poisson system over a distance of a few Earth radii along an auroral flux tube. The Vlasov equation was used in plasma physics by ...
Theory of pulsar winds and nebulae - Max-Planck
Theory of pulsar winds and nebulae - Max-Planck

... the wavelength of the radiation that would be emitted by the pulsar in vacuum is 2πrL . In the terminology of radiating systems, the region within the light cylinder is, therefore, the “near zone”, where the fields can be approximated as being in rigid corotation. Conventionally, this region is call ...
Lecture 12 ELEC 3105 NEW - Department of Electronics
Lecture 12 ELEC 3105 NEW - Department of Electronics

... A linear particle accelerator (often shortened to linac) is a type of particle accelerator that greatly increases the velocity of charged subatomic particles or ions by subjecting the charged particles to a series of oscillating electric potentials along a linear beamline; this method of particle ac ...
1 - UCLA IGPP
1 - UCLA IGPP

Ionization and Transport
Ionization and Transport

... As a result, FLUKA can correctly simulate electron backscattering even at very low energies and in most cases without switching off the condensed history transport (a real challenge for an algorithm based on Moliere theory!) The sophisticated treatment of boundaries allows also to deal successfully ...
A Rigid-Field Hydrodynamics approach to modelling the
A Rigid-Field Hydrodynamics approach to modelling the

... We introduce a new Rigid-Field Hydrodynamics approach to modelling the magnetospheres of massive stars in the limit of very strong magnetic fields. Treating the field lines as effectively rigid, we develop hydrodynamical equations describing the one-dimensional flow along each, subject to pressure, ...
Current can produce magnetism.
Current can produce magnetism.

... Page 93 shows how a simple motor works. The photograph at the top of the page shows a motor that turns the blades of a fan. The illustration in the middle of the page shows the main parts of a simple motor. Although they may look different from each other, all motors have similar parts and work in a ...
Plate Tectonics
Plate Tectonics

Ferromagnets and Electromagnets
Ferromagnets and Electromagnets

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Aurora



An aurora is a natural light display in the sky, predominantly seen in the high latitude (Arctic and Antarctic) regions. Auroras are produced when the magnetosphere is sufficiently disturbed by the solar wind that the trajectories of charged particles in both solar wind and magnetospheric plasma, mainly in the form of electrons and protons, precipitate them into the upper atmosphere (thermosphere/exosphere), where their energy is lost. The resulting ionization and excitation of atmospheric constituents emits light of varying colour and complexity. The form of the aurora, occurring within bands around both polar regions, is also dependent on the amount of acceleration imparted to the precipitating particles. Precipitating protons generally produce optical emissions as incident hydrogen atoms after gaining electrons from the atmosphere. Proton auroras are usually observed at lower latitudes. Different aspects of an aurora are elaborated in various sections below.
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