EPOD - a service of USRA
The Earth Science Picture of the Day (EPOD) highlights the diverse processes and phenomena which shape our planet and our lives. EPOD will collect and archive photos, imagery, graphics, and artwork with short explanatory
captions and links exemplifying features within the Earth system. The
community is invited to contribute digital imagery, short captions and
relevant links.
Archive - Aurora Observed from Space Station
January 16, 2021
Iss006-e-47517_540
Every weekend we present a notable item from our archives. This EPOD
was originally published January 16, 2004.
Provided by: NASA Earth Observatory
Summary authors & editors: Earth Observatory; Jim Foster
According to Expedition 6 Science Officer Don Pettit, aboard the
International Space Station (ISS), being in orbit around the Earth
offers a unique perspective on auroras. He mentioned that when their
orbit coincided with local midnight at high latitudes, the lights were
turned down so that it was possible to peer out the windows at the
breathtaking views of the shimmering northern lights. The above photo
was taken from the ISS as it orbited over the Southern Hemisphere,
approximately 400 km above the Earth’s surface, on April 20, 2003.
Most of the auroral light is emitted by oxygen atoms excited from
bombardment by charged solar particles. Charged particles consisting of
atomic fragments released by the Sun stream through space and run into
Earth’s magnetic field. When a charged particle encounters our magnetic
field, a force perpendicular to the motion is created, which diverts
the particle into a spiral path until it collides with atoms in the
upper atmosphere. The collisions excite the atoms (oxygen and nitrogen)
into emitting light, in much the same way that electrons pumped inside
of a glass tube filled with neon gas create a neon light. Green light
is the color most commonly observed. It's emitted from excited oxygen,
centered around a wavelength in the electromagnetic spectrum of 558
nanometers. Red light, emitted about wavelengths in the 630 nanometer
region, is less infrequently observed. Green emissions extend from
about 100 km altitude to approximately 300 km, whereas the red
emissions lie on top of the green and extend to perhaps 500 km.
Related EPODs
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Germany Parisian Sky: Glaciating Virga Crepuscular Rays over
the Roof Tops of Manchester November Gales on Lake Michigan
More...
Atmospheric Effects Links
* Atmospheric Optics
* Color and Light in Nature
* The Colors of Twillight and Sunset
* Refraction Index
* Image Gallery: Atmospheric Effects
* What is a Rainbow?
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Space Research Association.
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