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Year 9 Magnetism summary sheet
Year 9 Magnetism summary sheet

... A north pole and a south pole attract each other. Two north poles or two south poles will repel each other. The space around a magnet where it has an effect is called its magnetic field. ...
Earth as a Magnet
Earth as a Magnet

... sun towards our planet. • Solar wind is a stream of charged particles moving at high speeds from the sun to the earth. • These solar winds give the magnetosphere its shape and is constantly reshaping it as the Earth orbits the sun and rotates on its axis. • Most particles from this wind cannot get t ...
High Speed, High Resolution Multi-Probe Magnetic Field Mapping
High Speed, High Resolution Multi-Probe Magnetic Field Mapping

Magnetism
Magnetism

Electromagnetic Forces
Electromagnetic Forces

L 28 Electricity and Magnetism [5]
L 28 Electricity and Magnetism [5]

Magnetism PowerPoint
Magnetism PowerPoint

... “magnetite.” They discovered that the stone always pointed in the same direction. Later, stones of magnetite called “lodestones” were used in navigation. ...
3 The Magnetosphere
3 The Magnetosphere

... with the lobe magnetic pressure. The plasma sheet has a clear boundary (plasma sheet boundary) due to the presence of X point at the magnetotail at approximately 120 Re (point of magnetic reconnection; Line 7 in Fig.3). The lobe magnetic field is open, allowing the outflow of solar wind plasma. In c ...
Magnets and Magnetism
Magnets and Magnetism

...  Magnetic Fields- area ...
Guided Reading: Magnetism
Guided Reading: Magnetism

... 21. Refer to Figure 36.8, copy the caption below: ...
Magnetism
Magnetism

... 21. Refer to Figure 36.8, copy the caption below: ...
Lecture_7_Magnets and Magnetism print
Lecture_7_Magnets and Magnetism print

File - Lanier Bureau of Investigation
File - Lanier Bureau of Investigation

magnetic field
magnetic field

Chapter 15
Chapter 15

Guided Reading 15.1
Guided Reading 15.1

"High density operation (SDC/IDB configuration) in LHD and its
"High density operation (SDC/IDB configuration) in LHD and its

... Results of High-b Experiments 5% plasma was maintained for more than 10tE, whereas 4.8 % one was for 85 tE ...
L 28 Electricity and Magnetism
L 28 Electricity and Magnetism

Chapter 19 - springsphysics
Chapter 19 - springsphysics

The Earth`s Magnetic Field
The Earth`s Magnetic Field

L 28 Electricity and Magnetism [5]
L 28 Electricity and Magnetism [5]

Chapter 15 - Cloudfront.net
Chapter 15 - Cloudfront.net

... http://www.windows.ucar.edu/tour/link=/physi cal_science/magnetism/bar_magnet_inter active.html ...
Magnetism Permanent magnetism Permanent magnets
Magnetism Permanent magnetism Permanent magnets

... • A compass needle is attracted to the earth’s north geographic pole • The earth’s magnetism is the magnetic north pole is due to currents flowing in inclined about 14° from the its molten core (not geographic north pole, or entirely understood!) ...
Magnets Notes
Magnets Notes

... Draw a picture modelling the behavior of magnetic poles when they are brought together. Like poles _______________ ...
L 28 Electricity and Magnetism [5]
L 28 Electricity and Magnetism [5]

... naturally magnetic • a piece of loadstone will attract bits of iron • a magnet produces a magnetic field in the space around it, just like the Sun produces a gravitational field that holds the planets in their orbits • the magnetic field can be ...
< 1 ... 31 32 33 34 35 36 37 38 39 ... 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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