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Chapter 5
Chapter 5

Forces on Moving Charges in Magnetic Fields Standards
Forces on Moving Charges in Magnetic Fields Standards

... Students should understand the force experienced by a charged particle in a magnetic field, so they can: 1) Calculate the magnitude and direction of the force in terms of q, v, and B and explain why the magnetic force can perform no work. 2) Deduce the direction of a magnetic field from information ...
Global distributions_ temperature
Global distributions_ temperature

EM Waves
EM Waves

The Earth`s Interior
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... The Earth’s Interior Introduction  For much of our history, we have been ignorant of the inside of the interior on which we live.  Only is recent years have we been able to develop an image of the interior of the earth.  Today, it is known that the earth’s interior is so hot that it should be in ...
Relating the solar activity to climate variations has a long
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Debris Belts Around Vega
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... icy Kuiper belt. ...
ESS 7 Lecture 14 October 31, 2008 Magnetic Storms
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Lesson 6 The Sun and its power source
Lesson 6 The Sun and its power source

$doc.title

... Introduction  to  Plasma  Physics  (PY5012)   Homework  1   Submit  solutions  at  lecture  on  Monday,  October  10,  2011   Note:  This  homework  is  worth  10%  of  total  module  mark   ...
Earth`s Structure notes 5/26/15 • Crust
Earth`s Structure notes 5/26/15 • Crust

... • Mantle- 80 % 0f the volume of the earth. – Upper mantle is rigid, below is the asthenosphere which is a plastic like layer on which the tectonic plates float. – There is a huge difference in temperature between the outer mantle and the inner mantle. – This difference in temperature sets up a conve ...
Unit 1
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Fun Facts about Earth`s Magnetism caused by the Dynamo Effect
Fun Facts about Earth`s Magnetism caused by the Dynamo Effect

... moves from the Earth’s spin axis. The magnetic North Pole keeps moving. Right now, the magnetic North Pole is very close to the Earth’s axis. One hundred years ago, it was in Arctic Canada. The magnetic South Pole also moves. The magnetosphere is the magnetic force that extends into space. This forc ...
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NGC 2014 POSTER Tectonic setting of basaltic dykes from the

Debris Belts Around Vega
Debris Belts Around Vega

... also has four giant planets orbiting between the rocky asteroid belt and the icy Kuiper belt. ...
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crust

... that pulls objects toward the center (core) of the Earth. Weight is a measure of the strength of this pull. • Unit of weight is a Newton (N) ...
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Earth`s magnetic field – what is it good for?

(EM) Radiation
(EM) Radiation

Comets, asteroids, and meteors
Comets, asteroids, and meteors

... spread out and remain in the original orbit around the Sun, these may cross paths with Earth’s orbit If they enter Earth’s atmosphere- due to how fast they are travelling, this causes friction which causes the meteoroid to completely vaporize. ...
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Van Allen radiation belt



A radiation belt is a layer of energetic charged particles that is held in place around a magnetized planet, such as the Earth, by the planet's magnetic field. The Earth has two such belts and sometimes others may be temporarily created. The discovery of the belts is credited to James Van Allen and as a result the Earth's belts bear his name. The main belts extend from an altitude of about 1,000 to 60,000 kilometers above the surface in which region radiation levels vary. Most of the particles that form the belts are thought to come from solar wind and other particles by cosmic rays. The belts are located in the inner region of the Earth's magnetosphere. The belts contain energetic electrons that form the outer belt and a combination of protons and electrons that form the inner belt. The radiation belts additionally contain less amounts of other nuclei, such as alpha particles. The belts endanger satellites, which must protect their sensitive components with adequate shielding if their orbit spends significant time in the radiation belts. In 2013, NASA reported that the Van Allen Probes had discovered a transient, third radiation belt, which was observed for four weeks until destroyed by a powerful, interplanetary shock wave from the Sun.
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