The case of the relativistic particles solved with NASA missions

The case of the relativistic particles solved with NASA missions

Encircling Earth are two enormous rings—called the Van Allen radiation belts—of highly energized ions and electrons. Various processes can accelerate these particles to relativistic speeds, which endanger spacecraft unlucky enough to enter these giant bands of damaging radiation. Scientists had previously identified certain factors that might cause particles in the belts to become highly energized, but they had not known which cause dominates.

Now, with new research from NASA's Van Allen Probes and Time History of Events and Macroscale Interactions during Substorms—THEMIS—missions, published in Geophysical Research Letters, the verdict is in. The main culprit is a process known as local acceleration, caused by electromagnetic waves called . Named after their characteristic rising tones, reminiscent of chirping birds, chorus waves speed up the particles pushing them along like a steady hand repeatedly pushing a swing. This process wasn't a widely accepted theory before the Van Allen Probes mission.

Establishing the main cause of the radiation belt enhancements provides key information for models that forecast space weather—and thus protect our technology in space.

"We've had studies in the past that look at individual events, so we knew local acceleration was going to be important for some of the events, but I think it was a surprise just how important local acceleration was," said Alex Boyd, lead author and researcher at New Mexico Consortium, Los Alamos, New Mexico. "The results finally address this main controversy we've been having about the radiation belts for a number of years."

In a background magnetic field, represented by the cyan arrows, two electrons are propagating to the right, executing identical gyromotion. A circularly polarized electromagnetic wave approaches the upper electron from the left. Credit: NASA

There are two main causes of particle energization in the Van Allen belts: radial diffusion and local acceleration. Radial diffusion, which often occurs during solar storms—giant influxes of particles, energy and magnetic fields from the Sun, which can alter our space environment—slowly and repeatedly nudges particles closer to Earth, where they gain energy from the magnetic fields they encounter. Many scientists had long thought this was the primary, or even only, cause of energization.

However, early on in its mission, the Van Allen Probes showed that local acceleration, which is caused by particles interacting with waves of fluctuating electric and magnetic fields can also provide energy to the particles. The new research, which looked at nearly a hundred events over almost five years, shows that these wave-particle interactions are responsible for energizing particles around Earth 87 percent of the time.

Chorus waves as heard by the EMFISIS instrument aboard NASA's Van Allen Probes as it passed around Earth. Credit: NASA/University of Iowa

The scientists knew that local acceleration was at work because they observed mountains of energetic growing in one place, as the local acceleration mechanism predicts, rather than sliding in Earthwards as diffusion would.

That's a large percentage for a process that wasn't perceived as a strong candidate even five years ago. "Radial diffusion is definitely important for the radiation belts, but wave-particle interactions are much more important than we realized," said Geoff Reeves, co-author at the New Mexico Consortium.


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More information: What Causes Radiation Belt Enhancements: A Survey of the Van Allen Probes Era, Geophysical Research Letters (2018). doi.org/10.1029/2018GL077699 , agupubs.onlinelibrary.wiley.co … 10.1029/2018GL077699
Journal information: Geophysical Research Letters

Citation: The case of the relativistic particles solved with NASA missions (2018, May 29) retrieved 16 November 2019 from https://phys.org/news/2018-05-case-relativistic-particles-nasa-missions.html
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