A NASA-funded study found a region between radiation belts surrounding the Earth is not as benign as once thought. The region was considered a safe zone for satellites in "Middle Earth" orbits, because of relatively small amounts of radiation.
The observations revealed the Van Allen Radiation Belt Slot, often considered a safe zone, filled with concentrated radiation during the ferocious solar storms of October and November 2003. The radiation surge was the most intense ever observed in this region, according to researchers.
"Space weather matters. We know that no matter what orbit we choose, there is the possibility a spacecraft could get blasted by a significant dose of radiation," said Daniel Baker, Director of the Laboratory for Atmospheric and Space Physics at the University of Colorado, Boulder, and lead author of the study. "We need to take space weather into account when designing spacecraft. We also need the ability to continuously monitor space weather, so satellite operators can take protective measures during solar storms," he said.
High radiation occasionally forms in the safe zone during solar storms. This radiation is usually not intense and dissipates in a few days. During the 2003 solar storms, billion-ton eruptions of electrified gas slammed into the Earth's magnetic field at millions of miles per hour. This generated powerful electric fields that forced much of the plasmasphere into interplanetary space. It was eroded to an unprecedented degree, to the point below the safe zone. Since the plasmasphere was below the safe zone, an intense radiation belt powered by the solar storms formed in the region.
If the Van Allen radiation belts were visible from space, they would resemble a pair of donuts around the Earth, one inside the other with the planet in the hole of the innermost one. The safe zone would appear as a gap between the inner and outer donut, beginning about 7,000 km (4,350 miles) and ending approximately 13,000 km (8,110 miles) above the Earth's surface. The belts are comprised of high-speed electrically charged electrons and atomic nuclei trapped in the Earth's magnetic field.
The Solar, Anomalous and Magnetospheric Particle Explorer (SAMPEX) satellite flies through these belts, taking measurements of the particle types, their energy and abundance. SAMPEX observed the formation of the new belt in the safe zone on October 31, 2003. The radiation remained intense for about two weeks, and then gradually dissipated.
NASA's Imager for Aurora to Magnetopause Global Exploration (IMAGE) satellite observed the loss of the plasmasphere during the solar storms. Since solar ultraviolet radiation energizes helium ions in the plasmasphere, causing them to glow in ultraviolet light, the Extreme Ultraviolet Imager instrument on IMAGE can record the extent of the plasmasphere by observing this glow.
IMAGE discovered the plasmasphere was at its lowest point on October 31, 2003. The plasmasphere slowly expanded past the safe zone, replenished by particles from Earth's upper atmosphere. After its expansion beyond the safe zone, SAMPEX observed the dissipation of the new radiation belt.
"We were surprised to see the radiation belt persist so long after the plasmasphere expanded past the safe zone," said Jerry Goldstein of the Southwest Research Institute (SwRI), San Antonio, a co-author of the paper. "Radiation in the safe zone remained strong for a few weeks, a lot longer than usual," he said.
The research used theory, modeling, and observations from work sponsored by the National Science Foundation and the National Oceanic and Atmospheric Administration. The research team included Drs. Shri Kanekal, Xinlin Li, and Steven Monk also of the University of Colorado and Dr. James Burch of SwRI.
The research data was presented today during the American Geophysical Union Fall meeting in San Francisco, and it appears tomorrow in the journal Nature. For more information about the research and images on the Web, visit:
http://www.nasa.gov/vision/universe/solarsystem/safe_zone.htmlFor information about NASA and agency research programs on the Web, visit:
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