University of Minnesota-led experiment to fly on NASA mission to Earth's radiation belts

A University of Minnesota-led experiment is set for launch Friday, Aug. 24 aboard NASA's Radiation Belt Storm Probes (RBSP) mission, a probe of the forces that govern radiation in the Van Allen Radiation Belts. These two concentric, doughnut-shaped regions of space girdle the Earth and pose radiation danger to astronauts and spacecraft.

Data from RBSP will deepen scientists' understanding of how radiation belt particles become energized and aid the design of spacecraft to withstand the strongest radiation.

"We really are trying to understand these systems, because if we can't understand them, we can't send [astronauts] out there," said Mona Kessel, RBSP program scientist.

The two-year mission will send twin spacecraft into orbit through both Van Allen Belts, areas of strong radiation from protons, electrons and other subatomic particles trapped in Earth's . Forces originating with can intensify radiation in the belts; this mission marks the first time two spacecraft have explored the region of space where these acceleration processes occur.

The University of Minnesota-led experiment, the Electric Field and Waves Suite (EFW), will study the sizes, intensities and durations of electric fields that accelerate particles in the belts and how solar activity influences them. Such activity includes the , a stream of charged particles, or plasma, emanating from the sun at up to 2,000 kilometers per second (or more than 4 million miles per hour); and coronal mass ejections (CMEs), multibillion-ton bubbles of plasma hurled out from the sun's corona.

John Wygant, physics professor in the University of Minnesota's College of Science and Engineering and the principal investigator for EFW, also worked on the original Geospace Mission Design Team that conceived of RBSP. He described how particles from the sun can intensify radiation in the Van Allen Belts:

"CMEs that go faster than the solar wind—typically 1,000,000 kilometers per second—can produce interplanetary shock waves that deliver sharp impulses to the Van Allen Belts," Wygant said. "They can energize particles to relativistic speeds in 10 to 60 seconds. And if the solar wind is variable, it can jostle Earth's magnetic field, create variation in electric fields associated with it, and accelerate particles on magnetic field lines."

"On this mission, we're especially interested in periods when these acceleration processes are most powerful and the intensity of radiation increases by factors of 100 to 100,000," Wygant added.

The inner Van Allen Belt lies between about 100 and 10,000 kilometers altitude, the outer between about 13,000 and 60,000 kilometers. These fluid areas can change size and shape, meld into each other and even disappear temporarily. But the International Space Station and other satellites regularly pass through part of the inner belt and so require extra shielding.

The RBSP spacecraft will follow nine-hour orbits through both belts, venturing out as far as 39,000 kilometers and swooping as close as 580 kilometers to Earth. The EFW experiment will measure electric fields in 3-D by means of three pairs of probes, two on cables spanning 100 meters—longer than a football field.

Wygant and his University of Minnesota colleagues, including Professor Cynthia Cattell, three graduate students, several postdoctoral fellows and project manager Keith Goetz, will compare data from the two RBSP spacecraft and from other spacecraft, such as ones that detect interplanetary shock waves.

"We can tell when a shock wave goes by and correlate [our electric field measurements] with it and with changes in magnetic fields," Wygant said. "We can pick up the geometry of shock waves and electric fields."

By correlating data on electric fields and intensities (measured by other RBSP experiments), Wygant and his colleagues will get a handle on what kinds of electric fields help energize the particles in the belts. With two spacecraft, EFW can measure the sizes of electric field structures, even those thousands of kilometers wide.

RBSP will also investigate the forces that eject particles from the belts. Some are lost in Earth's upper atmosphere, where they cause auroras; others escape to the far reaches of Earth's magnetic field.

Many of the acceleration processes that occur in the inner regions of Earth's magnetic field are also believed to occur at other planets, at sudden releases of magnetic energy from the sun's surface (solar flares); and at more remote objects like ordinary stars; collapsed, rapidly spinning stars called pulsars; and black holes.

"Understanding the similarities and differences between how particles are accelerated at these different places is an ongoing effort for a wide range of scientists," Wygant said.

James Van Allen, a University of Iowa physicist, first discovered the inner belt in 1958 with a cosmic ray detector on the Explorer 1 spacecraft—NASA's first mission. The second was found a few months later, using data from Explorer 4 and Pioneer 3.

Working with the University of Minnesota on EFW are scientists from the University of California, Berkeley, and the University of Colorado. The twin spacecraft were built at the Johns Hopkins University Applied Physics Laboratory.

According to NASA, RBSP is scheduled to launch no earlier than 4:07 a.m. EDT Friday, Aug. 24 from Cape Canaveral Air Force Station in Florida. The twin probes will lift off on a United Launch Alliance Atlas V rocket.

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Citation: University of Minnesota-led experiment to fly on NASA mission to Earth's radiation belts (2012, August 23) retrieved 17 August 2019 from
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Aug 23, 2012
Those radiation belts are just part of the electric currents that connect the Earth with the Sun, until NASA has the ability to map all the electric current sheets and electric fields in addition to the related magnetic fields in the Earth-Sun relationship (as well as the other planets and heliosphere) there will be no way to accurately predict space weather. At least they are starting to investigate the undeniable aspects of our 'Electric/Plasma Universe'.

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