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Image of HAARP
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In the Copper River Valley, near a small town called Gakona in
eastern Alaska, scientists are studying the airglow and aurora, and even creating their own. Although not as colorful
as the natural aurora that often paint the skies over Alaska, the
artificial airglow is proving very useful in understanding how the
Sun's radiation affects the Earth's atmosphere and what that means
for us.
Researchers at the High Frequency Active Auroral Research Program
(HAARP) are using powerful radio antennae to study and even mimic
what the Sun's energy does to the atmosphere. One reason understanding
the atmosphere is important is to keep track of how it might change
over time. We rely on the atmosphere for the air we breathe as well
as protection from the Sun's powerful energy, so it's something
we'd like to keep around. Different levels of the atmosphere are
also very useful for communication, so studying them can help us
communicate better.
Radio signals can be sent over great
distances through the ionosphere, which starts about 35 miles (56
km) above the Earth's surface and extends up to about 500 miles (805
km). Storms on the Sun that send lots of energetic particles to the
Earth and cause aurora can distort the ionosphere and interrupt our
communications. Scientists at HAARP recreate, on a small scale, what
happens when the atmosphere is excited by the Sun's energy.
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Image of Elizabeth with telescope
(courtesy Elizabeth Gerken)
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Artificial airglow
When HAARP was used to excite a section of the ionosphere on several
days in 2000, 2001, and 2002, researcher Elizabeth Gerken, a graduate
student at Stanford University in California, was there. She and
her fellow scientists watched the airglow created in the ionosphere
through a telescope that has a special electronic camera called
a charge-coupled device, or CCD. Red or green glass filters were
placed in front of the camera's lens to allow it to "see" only certain
types of light. The camera's shutter was kept open for 30 seconds
so it could image faint glows that are invisible to the human eye.
The camera sends digital pictures directly to a computer for processing
into images that Elizabeth can then analyze. By studying how the
ionosphere reacts to the experiments, scientists can begin to understand
how it behaves during natural airglow and aurora.
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Image of Sprite
(courtesy Elizabeth Gerken)
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Sprites and elves
Sprites and elves may sound like creatures you'd be looking for
low to the ground, maybe near some fairies or leprechauns. But you'll
need to look high in the sky to find the types of sprites and elves
hunted by Elizabeth. Sprites are flashes of light that sometimes
appear above thunderstorms at the same time lightning hits the ground
or another cloud. Sprites are difficult to spot with the human eye
because they are not very bright and because they last only a portion
of a second. If you divide a second into 100 pieces, a sprite would
be gone after just one or two! Sprites are also rare, only occuring
with about one percent (that's 1 out of 100) lightning strikes.
If you think you're fast enough to catch one, look under Resources
for viewing tips. Pancake-shaped elves are even more fleeting than
sprites, and appear slightly before them. Elizabeth and her fellow
scientists use telescopes and television cameras to look for and
record these phenomena (rare events). By studying the structures of sprites and elves,
and the direction in which they develop, Elizabeth hopes to learn
what causes them and to better understand the atmosphere.