May 09, 2002 -(date of web publication) EARTH'S SPACE STORM SHIELD OFFERS PROTECTION AT A PRICE
New observations from a NASA spacecraft reveal that a layer in the Earth's outer atmosphere acts like a heat shield by absorbing energy from space storms, which reduces their ability to heat the lower atmosphere. However, it imposes a heavy toll for its services by creating a billion-degree cloud of electrified gas, or plasma, that surrounds our planet. The plasma cloud is so ferociously hot, its particles act like radiation, occasionally disrupting satellites in mid to high orbits. This discovery from NASA's Imager for Magnetopause to Aurora Global Exploration (IMAGE) spacecraft confirms that the Earth actively participates in space storms.
Although past space missions gave provisional evidence for this behavior, IMAGE provides the first global picture of the active role Earth's ionosphere plays in space storms, which is very different from the earlier view that the solar wind itself supplied the energetic particles responsible for these storms.
The Earth's space storm shield is a tenuous layer of the outer atmosphere (outer ionosphere) between 180-620 miles (300-1,000 kilometers) high that includes electrically charged atoms. "Just as a heat shield sacrifices itself by allowing its outer layers to slough off during the fiery reentry of a spacecraft, Earth's shield absorbs space storm energy by throwing some of its charged particles into space," said Stephen Fuselier of the Lockheed-Martin Advanced Technology Center, Palo Alto, Calif., who is lead author of the first of two papers on this discovery to be published in the Journal of Geophysical Research.
"But this protection comes with a high price, because the expelled particles gain tremendous speed as they leave the atmosphere, become trapped by the Earth's magnetic field and ultimately encircle the Earth, where they form a hot plasma cloud around the planet," said Donald Mitchell of the Johns Hopkins Applied Physics Laboratory, Laurel, Md., who is lead author of the second paper. Approximately half of the energy deposited by space storms in our atmosphere is absorbed this way, according to the researchers.
The solar wind, a thin, high-velocity plasma, blows constantly from the Sun at an average speed of 250 miles per second (400 kilometers/sec). If the Earth had no global magnetic field, or magnetosphere, the solar wind would impact our atmosphere directly and gradually erode it away. Instead, the solar wind slams into the Earth's magnetosphere and is diverted around our planet. Buffeting of the magnetosphere is more intense during space storms, when explosive events on the Sun give the solar wind an unusually high velocity or density, or a particularly potent magnetic field configuration.
Although the magnetosphere does a good job staving off the solar wind, Earth is not home free. Since the solar wind plasma is comprised of electrically charged particles that are moving rapidly past the Earth's magnetic field, a multimillion amp electric current is generated, which flows down the Earth's invisible magnetic field lines and pumps up to a trillion watts of power into the magnetosphere, especially above the polar regions, where the aurora (northern and southern lights) form. Without the space storm shield, heat from these enormous electric currents would cause our lower atmosphere (lower ionosphere) to expand and increase orbit-disrupting drag on spacecraft.
The first result from IMAGE shows the Earth's shield in action as it absorbs a space storm's electric current and is ejected into space. Fuselier used the Low Energy Neutral Atom imager (LENA) instrument on IMAGE to discover that electrically charged oxygen atoms are ejected into space immediately in response to the bursts of heating of the ionosphere by the massive electric currents. The amount of ionosphere lost during a typical space storm is around a few hundred tons, about equal to the mass of the air in the Louisiana Superdome, according to the team.
The second IMAGE observation shows the price paid for the shield's protection. Because of their electric charge, the expelled oxygen ions feel magnetic forces and are trapped within the Earth's vast magnetosphere, where they follow magnetic field lines like cars on a highway. Scientists know that the magnetosphere distorts under the impact of the solar wind, like an umbrella in a windstorm. In particular, the region of the magnetosphere facing away from the Sun is stretched into a long, tail-like shape as the solar wind blows by. Because magnetic fields have tension, they resist stretching and behave like rubber bands. When the stretching becomes too great, the night-side magnetosphere snaps back towards Earth, carrying the ejected ions from the ionosphere with it like an enormous slingshot.
Mitchell used the High Energy Neutral Atom imager (HENA) instrument on IMAGE to observe that these ions, now accelerated to enormous velocities (about 2,500 miles per second or 4,000 km/sec), appear immediately in the aurora and in the cloud of hot plasma that encircles the Earth during space storms. Earth contributes material and the solar wind supplies the energy which transforms this cool atmospheric material into a dangerously hot plasma cloud. If it were not for the Earth's own ionosphere supplying material, the hot plasma cloud would be very much diminished.
This new view is
helping scientists to better understand the effects of space
storms, which create moving plasma clouds that interfere with
navigation using Global Positioning System satellites.
RELATED LINKS AND IMAGES
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Movies of Images 1 - 4:
Caption for Images 1 - 4:
These images are taken from a computer animation illustrating the Earth's space storm shield in action. The solar wind, a thin, high-velocity electrified gas, or plasma, blows constantly from the Sun at an average speed of 250 miles per second (400 kilometers/sec). It is represented in Image 1 as a stream of yellow particles flowing from the Sun. The solar wind impacts the Earth's magnetic field, represented by the blue lines in Image 2. As the solar wind flows past the Earth's magnetic field, it generates enormous electric currents that heat Earth's space storm shield -- a layer in the Earth's electrically charged outer atmosphere (ionosphere) -- causing the shield to eject electrically charged oxygen atoms (oxygen ions) into space. The expelled oxygen ions are represented by the green particle streams in Image 3. The ejected oxygen ions gain tremendous speed as they leave the atmosphere, become trapped by the Earth's magnetic field and ultimately encircle the Earth, where they form a billion-degree plasma cloud around the planet, represented by the red cloud in Image 4. The blue doughnut shape in Image 4 represents the high-speed flow of these particles around the Earth. The red "ring of fire" around the Earth's polar regions represents the contribution of the particles to the aurora (the northern and southern lights).
Movie of Image 5:
Caption for Image 5:
The green areas in this image are the outflow of electrically charged oxygen atoms (oxygen ions) from the Earths ionosphere during a space storm as seen by the LENA instrument on board the IMAGE spacecraft.
Movie of Image 6:
Caption for Image 6:
This image shows the concentration of billion-degree plasma particles that surround the Earth during a space storm as seen by the HENA instrument on board the IMAGE spacecraft. Red represents the greatest density of particles; blue the least. The apparent size of the Earth, as seen from IMAGE's position in orbit, is represented by a white circle near the center of the image. The white loops represent the shape and size of the Earth's magnetic field at various positions.
Auroral Circuit movie:
The Aurora (Northern and Southern lights) are part of an enormous, multimillion-amp electric circuit powered by the interaction of the solar wind with the Earth's magnetic field. Electrically charged particles (electrons and ions) carry the current in this circuit. These particles move at high speed, and generate beautiful displays of light over the polar regions when they slam into particles in the Earth's upper atmosphere (ionosphere). This process is similar to the way a TV tube is illuminated by high-speed electrons impacting the phosphor on the back of the screen.
IMAGE Spacecraft movie:
This is a computer animation illustrating the IMAGE spacecraft in orbit as it explores the Earth's vast but invisible magnetic field.
Ion Flow movie:
This is a computer animation illustrating the flow of oxygen ions as they are expelled from the Earth's space storm shield and propelled back toward Earth. Because of their electric charge, the expelled oxygen ions feel magnetic forces and are trapped within the Earth's vast magnetosphere, where they follow magnetic field lines like cars on a highway. Scientists know that the magnetosphere distorts under the impact of the solar wind, like an umbrella in a windstorm. In particular, the region of the magnetosphere facing away from the Sun is stretched into a long, tail-like shape as the solar wind blows by. Because magnetic fields have tension, they resist stretching and behave like rubber bands. When the stretching becomes too great, the night-side magnetosphere snaps back towards Earth, carrying the ejected ions from the ionosphere with it like an enormous slingshot.