The twin Van Allen Probes orbit one behind the other, investigating clues in a way a single spacecraft never could. In this model, the trailing spacecraft saw an increase in injected oxygen particles (blue), which was unobserved by the first. The increase in particles was due to a geomagnetic storm front that moved across the path of the orbit after the first spacecraft passed.
Credit: NASA’s Goddard Space Flight Center/Mike Henderson/Joy Ng, Producer
High above Earth, two giant rings of energetic particles trapped by the planet’s magnetic field create a dynamic and harsh environment that holds many mysteries — and can affect spacecraft traveling around Earth. NASA’s Van Allen Probes act as space detectives, to help study the complex particle interactions that occur in these rings, known as the Van Allen radiation belts. Recently, the spacecraft were in just the right place, at just the right time, to catch an event caused by the fallout of a geomagnetic storm as it happened. They spotted a sudden rise in particles zooming in from the far side of the planet, improving our understanding of how particles travel in near-Earth space.
Scientists scoured the clues to figure out what was happening. With the help of computer models, they deduced that the particles had originated on the night side of Earth before being energized and accelerated through interactions with Earth’s magnetic field. As the particles journeyed around Earth, the lighter hydrogen particles were lost in collisions with the atmosphere, leaving an oxygen-rich plasma. The findings were presented in a recent paper in Geophysical Review Letters.
The unique double observations of the Van Allen Probes help untangle the complex workings of Earth’s magnetic environment. Such information has provided the very first view of these harsh belts from the inside — and it helps us better protect satellites and astronauts traveling through the region.
Source: NASA/Goddard Space Flight Center
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M. H. Denton, G. D. Reeves, M. F. Thomsen, M. G. Henderson, R. H. W. Friedel, B. Larsen, R. M. Skoug, H. O. Funsten, H. E. Spence, C. A. Kletzing. Geophysical Research Letters, Nature Geoscience2016; 43 (19): 10,059 DOI: 10.1002/2016GL070878