Out the Window of the ISS
From the International Space Station, astronaut Don Pettit got a unique view
of colorful auroras that sometimes dance above Earth's polar regions. He saw
them on Earth's endless horizon. He looked down into them. He flew through them.
Auroras occur when elevated solar activity accelerates tiny, charged particles
to race along Earth's magnetic field lines toward the poles. These particles
excite molecules in the upper atmosphere, causing them to glow.
From Earth's surface, people at high latitudes sometimes witness the aurora
from below. Pettit, the science officer for Expedition Six, got an edge-on view
of the undulating, ephemeral phenomena, allowing him to estimate how high they
go.
Green
is the predominant auroral color, but reds are fairly common. Blue and yellow
sometimes show up. Oxygen is the primary fuel for the lights, and nitrogen is
involved, too.
Green emissions ranged from about 62 miles (100 kilometers) above the surface
to about 186 miles (300 kilometers), Pettit writes in an account published by
NASA last week. Red emissions danced always atop the green and extended up to
311 miles (500 kilometers).
Sometimes the orbiting outpost flies right through an auroral display (it orbits
at about 250 miles, or 400 kilometers, up). Pettit's reflections on one such
journey:
"We were in a dimly glowing fog of red. It was like we had been shrunk down
to some miniature dimension and inserted into the tube of a neon sign. And it
was just on the other side of the windowpane ... we wanted to reach out and
touch! Afterwards, I had to clean a nose print off of the window."
The photographs were taken by Pettit with a Kodak
DCS760 digital camera. More of his images and thoughts, as well as animations
of auroras, are available from NASA's Earth
Observatory web site. See also a host of
aurora
pictures from the ground.
-- Robert
Roy Britt
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