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The Magnetosphere
Our Earth is a large magnet. The magnetic field lines extend out in space in
great arches form the North to the South pole. The magnetic poles of the earth
don't quite coincide with the North and South geographic poles, in fact they
tend to drift around a bit. As of 2005 the North Magnetic Pole lay near
Ellesmere Island in northern Canada
at 82.7° N 114.4° W.
The Earth's magnetic field protects us from cosmic rays and the Solar WInd
by deflecting particles around the Earth. This magnetic field is also important
in creating many of the Natural Radio sounds that we are able to hear.
The magnetosphere is the area around the Earth where the Earth's magnetic
field is dominant. Outside the magnetosphere the interplanetary magnetic field
is dominant.
The Ionosphere
Above the breatheable part of the atmosphere lies the ionosphere. From About
60 or 70 miles up the air thins out and the UV radiation from the Sun strips
electrons away form the atoms and forms an ionized plasma. The reflective
properties of the ionosphere bend radio waves of certain frequences that would
otherwise travel in straight lines out into space, and sends them back to
earth, thus allowing global shortwave communications.
The Plasmasphere
Above the Ionosphere is a region of the magnetosphere that contains plasma,
a highly ionized state of matter. The plasmasphere contains the Van Allen
radiation belts.
Whistler Mode Waves
Radio waves propagate through free space at 186,000 miles per second. In the
conductive plasmasphere, another type of propagation is possible. Whistler mode
wave propagate through plasma along magnetic field lines. Thes waves are
circularly polarixed as they spiral along the Earth's magnetic field lines.
Propagation is much slower than through free space.
Geomagnetic Storms
Coronal mass ejections and sometimes the solar wind
carry magnetic fields that can couple with the Earth's field and disrupt it
causing a geomagnetic storm. A severe geomagnetic storm may induce currents in
long power lines that will destroy equipment and cause power outages. Compasses
become useless and auroral displays may be seen in much lower latitudews than
normal. Geomagnetic storms also tend to generate VLF Emissions, Chorus and
other signals that are very interesting to Natural Radio listeners.
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