— Ch. 1 · The 1958 Discovery —
Van Allen radiation belt.
~3 min read · Ch. 1 of 6
In early 1958, the Explorer 1 satellite sent back data that changed our understanding of space. James Van Allen from the University of Iowa published an article describing these belts later that year. Before this moment, scientists like Kristian Birkeland and Carl Størmer had theorized about trapped particles since 1895. The Soviet Union's Sputnik 2 carried detectors designed by Sergei Vernov to search for similar phenomena. Explorer 3 followed shortly after, confirming the existence of a radiation zone around Earth. These early missions mapped the trapped radiation using instruments on Explorer 4, Pioneer 3, and Luna 1. The term Van Allen belts now refers specifically to the radiation zones surrounding our planet.
Protons in the Inner Zone
The inner belt extends from an altitude of 0.2 to 2 Earth radii above the surface. It contains high concentrations of electrons ranging from hundreds of keV. Energetic protons with energies exceeding 100 MeV are also trapped here. Proton energies over 50 MeV result from beta decay of neutrons created by cosmic ray collisions. These neutrons form when cosmic rays strike nuclei in the upper atmosphere. Lower energy protons arrive through diffusion caused by changes in the magnetic field during geomagnetic storms. The South Atlantic Anomaly allows the inner boundary to drop to roughly 200 km above Earth. This region makes the closest approach to the surface due to the offset of the belts from Earth's geometric center.