The astronomers say that a small number of anti-protons lie between the Van Allen belts of trapped “normal” matter. The antiprotons were spotted by the Pamela satellite launched in 2006 to study the nature of high-energy particles from the Sun and from beyond our Solar System — so-called cosmic rays, the ‘BBC’ reported.
These cosmic ray particles can slam into molecules that make up the Earth’s atmosphere, creating showers of particles. Many of the cosmic ray particles or these “daughter” particles they create are caught in Van Allen belts, doughnut-shaped regions where Earth’s magnetic field traps them.
The new analysis shows that when Pamela passes through a region called the South Atlantic Anomaly, it sees thousands of times more anti-protons than are expected to come from normal particle decays, or from elsewhere in the cosmos. The astronomers say this is evidence that bands of anti-protons, analogous to Van Allen belts, hold anti-protons in place — at least until they encounter the normal matter of atmosphere, when they “annihiliate” in a flash of light.
The band is “the most abundant source of anti-protons near the Earth”, said Alessandro Bruno, team member.
“Trapped anti-protons can be lost in the interactions with atmospheric constituents, especially at low altitudes where the annihilation becomes the main loss mechanism. Above altitudes of several hundred kilometres, the loss rate is significantly lower,” he added. PTI
“Trapped anti-protons can be lost in the interactions with atmospheric constituents, especially at low altitudes where the annihilation becomes the main loss mechanism. Above altitudes of several hundred kilometres, the loss rate is significantly lower,” he added. PTI
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