THE SOLAR SYSTEM

MAGNETIC FIELDS
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January 6-12, 2010
January 13-25, 2010
ORIGIN OF THE SOLAR SYSTEM
THE SUN
SOLAR FEATURES
EVOLUTION OF THE SUN
EARTH
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MERCURY
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DWARF PLANETS
KUIPER BELT
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LUNAR & PLANETARY PHASES
COMETS
ASTEROIDS
MAIN ASTEROID BELT
METEORS & METEORITES
AURORAS & MAGNETIC FIELDS
MAGNETIC FIELDS
KEPLER
NEWTON
PLANETARY MOTIONS
EFFECTS OF PLANETS & SATTELITES ON EACH OTHER
CHARACTERISTCS OF TERRESTRIAL AND GIANT PLANETS AND THEIR SATELLITES
GEOLOGIC ACTIVITIES OF PLANET AND SATELLITES
CONSTELLATIONS

The The magnetosphere is the Earth's magnetic environment. The Earth is a huge dipole (2-pole) magnet. The Earth's magnetic field is probably cause by its molten iron-nickel core. This magnetic field is aligned with the north and south poles, and has reversed many times during geologic history.

The Earth's magnetic field is about 0.32 Gauss at the equator and about 0.62 Gauss at the poles.

William Gilbert hypothesized that the Earth was a giant magnet in 1600. Thomas Gold proposed the name "magnetosphere" in 1959. The Earth's magnetosphere extends far into space and is influenced by the solar wind (ions and electrons emitted from the sun). It extends into space from 60 to 37,280 miles (100 to 60,000 km) towards the Sun, and over 186,500 miles (300,000 km) away from the Sun (nightward), forming the Earth's magnetotail.

The magnetopause is the boundary between the area in which the Earth's magnetic field dominates and the magnetic field of the rest of the Solar System dominates.

Auroras:
Charged particles become trapped on the field lines of the magnetosphere. Auroras appear when trapped particles from the solar wind spiral towards a pole. These beautiful arcs of lights in the near-polar sky are caused by gases that become excited after being hit by solar particles. Most auroras are 100 to 250 km above the ground (in the
ionosphere).

Earth has a magnetic field with north and south poles. The Earth's magnetic field reaches 36,000 miles into space.

The magnetic field of the Earth is surrounded in a region called the magnetosphere. The magnetosphere prevents most of the particles from the sun, carried in solar wind, from hitting the Earth.

Some particles from the solar wind can enters the magnetosphere. The particles that enter from the magnetotail travel toward the Earth and create the auroral oval light shows.

The Sun and other planets have magnetospheres, but the Earth has the strongest one of all the rocky planets. The Earth's north and south magnetic poles reverse at irregular intervals of hundreds of thousands of years.

Magnetosphere

A magnetosphere has many parts, such as the bow shock, magnetosheath, magnetotail, plasmasheet, lobes, plasmasphere, radiation belts and many electric currents. It is composed of charged particles and magnetic flux.

These particles are responsible for many wonderful natural phenomena such as the aurora and natural radio emissions such as lion roars and whistler waves.

The particles move and circulate about the magnetosphere and even generate storms. The magnetosphere changes constantly, even flipping its orientation every few thousand years.