Van Allen Probes circle radiation belts. This artist’s rendering of the Van Allen Probes mission shows the path of its two spacecraft through the radiation belts that surround Earth, which are made visible in false color.
The inner Van Allen belt has less radiation than previously believed, according to a recent study in the Journal of Geophysical Research. Observations from NASA’s Van Allen probes show the fastest, most energetic electrons in the inner radiation belt are actually much rarer and harder to find than scientists expected. This is good news for spacecraft that are orbiting in the region and can be damaged by high levels of radiation. The results will also help scientists better understand — and detect — effects from high-altitude nuclear explosions.
“Basically what we’re doing is detecting very small signals against very large backgrounds,” said Geoff Reeves, a space physicist at Los Alamos National Laboratory and co-author of the study. “Let’s say you have a few snowflakes in a rainstorm — but you’ve never seen snowflakes before. How do you ignore the rain so you can just see the snowflakes? That’s what we’ve done here: we ignored a whole lot of protons so we could see the electrons — and it turns out there aren’t as many as we thought.”
The Van Allen belts are two doughnut-shaped regions of charged particles encircling Earth. Past space missions have not been able to distinguish electrons from high-energy protons in the inner radiation belt. But by using a special instrument, the Magnetic Electron and Ion Spectrometer (MagEIS), on the Van Allen Probes, scientists could look at the particles separately for the first time. What they found was surprising: almost none of these super-fast electrons, known as relativistic electrons, are present in the inner belt.
Los Alamos National Laboratory has interest in the applications for space weather forecasting to protect satellites and also for monitoring the Nuclear Test Ban Treaty, which prohibits nuclear explosions in space. “A high-altitude nuclear explosion results in the creation of an artificial radiation belt,” said Reeves. “We can learn about the physics of an explosion by looking at these hard-to-detect relativistic electrons. If an artificial radiation belt were ever detected, these new observations would help us understand it better.”
Of the two radiation belts, scientists have long understood the outer belt to be the more active one. During intense geomagnetic storms, when charged particles from the sun hurtle across the solar system, the outer radiation belt pulsates dramatically, growing and shrinking in response to the pressure of the solar particles and magnetic field. Scientists thought that the inner belt maintains a steady position above Earth’s surface. The new results, however, show that’s not always true. For example, during a very strong geomagnetic storm in June 2015, relativistic electrons were pushed deep into the inner belt.
“When we carefully process the data and remove the contamination, we can see things that we’ve never been able to see before,” said Seth Claudepierre, lead author and Van Allen Probes scientist at the Aerospace Corporation in El Segundo, Calif. “These results are totally changing the way we think about the radiation belt at these energies.”
Given the rarity of the storms that can inject relativistic electrons into the inner belts, the scientists now understand that lower levels of radiation are typical there, a result that has implications for spacecraft flying in the region. Knowing exactly how much and what type of radiation is present in any given region of space may enable scientists and engineers to design lighter and cheaper satellites tailored to withstand the specific radiation levels they’ll encounter.
In addition to providing a new outlook on spacecraft design, the findings open a new realm for scientists to study next.
“This opens up the possibility of doing science that previously was not possible,” said Shri Kanekal, Van Allen Probes deputy mission scientist at NASA’s Goddard Space Flight Center in Greenbelt, Md., and not involved with the study. “For example, we can now investigate under what circumstances these electrons penetrate the inner region and see if more intense geomagnetic storms give electrons that are more intense or more energetic.”
S. G. Claudepierre, T. P. O’Brien, J. F. Fennell, J. B. Blake, J. H. Clemmons, M. D. Looper, J. E. Mazur, J. L. Roeder, D. L. Turner, G. D. Reeves, H. E. Spence. The hidden dynamics of relativistic electrons (0.7-1.5 MeV) in the inner zone and slot regionJournal of Geophysical Research: Space Physics, 2017; 095679761769136;DOI: 10.1002/2016JA023719