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Space Weather Satellite Blasts Off

NASA's IMAGE satellite successfully flew into orbit from Vandenberg AFB this weekend

see captionMarch 27, 2000 -- NASA’s newest space weather probe lifted off March 25 from the Western Range at Vandenberg AFB, CA at 12:34 p.m. PST. The "Imager for Magnetopause-to-Aurora Global Exploration" (IMAGE) spacecraft separated from the Delta II third stage about 56 minutes after launch and is now in an elliptical orbit, ranging from 1,000 kilometers to 45,871 kilometers above Earth.

"The skies cleared, then our hearts lifted with the IMAGE spacecraft; on time, on budget, on the start of a new era in space physics at the Earth," said onlooker Dennis Gallagher, a plasma physicist from NASA's Marshall Space Flight Center, who attended the launch along with other members of the IMAGE science team.

Right: Dennis Gallagher (NASA/MSFC) snapped this picture of IMAGE soaring into space aboard a Delta rocket on March 25, 2000.

"The spacecraft appears to be healthy with all systems performing nominally," said IMAGE project manager Frank Volpe at NASA’s Goddard Space Flight Center, Greenbelt, Md. "We are looking forward to a great science mission."

Instruments onboard the IMAGE spacecraft will provide scientists with never-before-seen global images of the Earth’s magnetosphere -- an area of space around our planet that is controlled by Earth’s magnetic field. Scientists expect the mission to revolutionize their understanding of the magnetosphere and to greatly improve space weather forecasting.

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"[Now that it's in orbit] there will be a 40 day period while the antennas for the radio plasma imager are deployed," explained Gallagher. "They're 500 meters tip to tip. As we reel them out, we have to continuously respin the spacecraft because it's spin-stabilized."

After the 40 day setup period, IMAGE will begin using its trio of neutral atom imagers, a far-ultraviolet imaging system, an extreme ultraviolet imager and a radio plasma imager to make movies of the magnetosphere. This unique approach will allow scientists to view, for the first time, the ‘big picture’ rather than capturing limited, local measurements at far-flung points in space.

see captionStay tuned to Science@NASA for science updates from the IMAGE mission. Please see our earlier articles "Space Weather Mission Nears Launch." and "The RADAR Cop in Space." to learn more.

Right: An artist's concept of IMAGE in orbit. Click for IMAGE animations, courtesy of Goddard Space Flight Center.

IMAGE is NASA’s first Medium-class Explorer (MIDEX) mission under the Agency’s Explorer Program. The principal institution for IMAGE is the Southwest Research Institute in San Antonio, which has overall responsibility for IMAGE science, instrumentation, spacecraft operations and data analysis during its two-year science mission. SwRI's Jim Burch is the IMAGE Principle Investigator. Lockheed Martin Missiles and Space Division in Sunnyvale, Calif. built and tested the 1,089-pound (494-kilogram) spacecraft under a contract with SwRI.



Web Links

IMAGE home page - from NASA/GSFC.

IMAGE home page - from the Southwest Research Institute.

Instruments on IMAGE include:

  • The Radio Plasma Imager. The RPI will use radar echoes in the frequency range 3 kHz to 3 MHz to detect and monitor ionized gas (plasma) inside the magnetosphere.
  • Far Ultraviolet Imager. The FUI will take pictures and spectra of the entire Earth along with the auroral oval at ultraviolet wavelengths. The 3 instruments that combine to form the FUI instrument package (GEO, SI and WIC) will provide almost constant monitoring of auroral activity from above our planet. The Earth is surrounded by a cloud of neutral atoms and molecules that is largely invisible from the ground. The so-called 'geocorona' is an extension of Earth's atmosphere into space. It is mostly made up of hydrogen, because it's the lightest element. GEO will also be used to detect these neutral atoms, measure their energy and map their distribution.
  • Neutral Atom Imagers. The neutral atom cameras will detect neutral atoms created by ring current ions and escaping auroral ions that collide and exchange charge with the cold, geocoronal hydrogen gas. This will allow scientists to indirectly monitor and explore the ring current and auroral ion fountains.
  • Extreme Ultraviolet Imager. The EUVI will detect ultraviolet photons from the Sun that are scattered by helium ions in the plasmasphere, a torus of cold dense plasma surrounding the Earth in the inner magnetosphere. A sophisticated deconvolution technique will be used to translate the photon counts into images of the plasmasphere.


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For lesson plans and educational activities related to breaking science news, please visit Thursday's Classroom Production Editor: Dr. Tony Phillips
Author: Dr. Tony Phillips
Source: IMAGE Status Report #1

Curator: Bryan Walls
Media Relations: Steve Roy (MSFC), Susan Hendrix (GSFC)
Responsible NASA official: John M. Horack