|
The
Magnetosphere
Saturday, May 3, 2008
Credit: JHAPL / NASA
The Earth is a huge magnet, and
its magnetic influence extends far into space.
In our everyday environment,
magnetic forces are of no importance and a sensitive instrument,
the compass needle, is needed to detect them. That is because we,
the materials we encounter in everyday life, even the oxygen and
nitrogen which we breathe, are all electrically neutral. The
atoms of oxygen, for instance, contain electrons with negative
electric charges and protons which are positive, but the two
charges balance each other andthe electric and magnetic forces
cancel. Magnetic forces have almost no effect on neutral atoms.
However, 60 miles (100 km) or
more above the surface of the Earth, the natural environment is
quite different. The fringes of the atmosphere at these heights
are strongly heated by the Sun's x-rays and ultra-violet light
(and by other causes as well), causing negative electrons to be
torn off atoms and leaving the remainder of the atoms as
positively charged "ions". These electrified fragments
react strongly to the magnetic forces and can be steered and
trapped by them.
With a suitable input of
energy, such fragments can also be accelerated to high speeds,
can give rise to electic currents and emit a variety of
radio-type waves.
It can be shown that such free
electrons and ions will be guided by the magnetic field lines (or
"lines of force") which rise from near the southern
(magnetic) pole and enter the Earth again near the northern pole.
Electrons and ions tend to remain attached to field lines like
beads on wires, though unlike beads they also slowly migrate
("drift") to neighboring "wires."
It follows that the structure
of field lines near Earth determines much of the motion and
behavior of the free electrons and ions found there. Satellites
observing magnetic forces in space have found (figure on right)
that lines from most points on Earth are confined inside a fairly
well-defined cavity, the magnetosphere of the Earth. The space
outside it is dominated by the Sun, and by the fast "solar
wind" of free ions and electrons emitted by the Sun.
Source:
NASA

|
Scientific
Frontline®
RSS
Feeds
Scientific
Frontline®
The
Comm Center
The
E.A.R.®
World
News Report
SFL
Gallery
Cassini
Gallery
Mars
Gallery
Missions
Gallery
Exploration
Gallery
Space
Weather Alerts
Stellar
Nights®
Events
Directors
Chair
Scientific
Frontline®
Is
supported in part by “Readers Like You”
|