Visualization of the radiation belts with confined charged particles (blue & yellow) and plasmapause boundary (blue-green surface). Credit: NASA\/Goddard <\/p>\n
Its a well-known fact that Earths ozone layer protects us from a great deal of the Suns ultra-violet radiation. Were it not for this protective barrier around our planet, chances are our surface would be similar to the rugged and lifeless landscape we observe on Mars. <\/p>\n
Beyond this barrier lies another a series of shields formed by a layer of energetic charged particles that are held in place by the Earths magnetic field. Known as the Van Allen radiation belts, this wall prevents the fastest, most energetic electrons from reaching Earth. <\/p>\n
And according to new research from NASAs Van Allen probes, it now appears that these belts may be nearly impenetrable, a finding which could have serious implications for future space exploration and research. <\/p>\n
The existence of a belt of charged particles trapped by the Earths magnetosphere has been the subject of research since the early 20th century. However, it was not until 1958 that the Explorer 1 and Explorer 3 spacecrafts confirmed the existence of the belt, which would then be mapped out by the Explorer 4, Pioneer 3, and Luna 1 missions. <\/p>\n
Two giant belts of radiation surround Earth. The inner belt is dominated by protons and the outer one by electrons. Credit: NASA <\/p>\n
Since that time, scientists have discovered much about this belt, including how it interacts with other fields around our planet to form a nearly-impenetrable barrier to incoming electrons. <\/p>\n
This discovery was made using NASAs Van Allen Probes, launched in August 2012 to study the region. According to the observations made by the probes, this region can wax and wane in response to incoming energy from the sun, sometimes swelling up enough to expose satellites in low-Earth orbit to damaging radiation. <\/p>\n
This barrier for the ultra-fast electrons is a remarkable feature of the belts, said Dan Baker, a space scientist at the University of Colorado in Boulder and first author of the paper. Were able to study it for the first time, because we never had such accurate measurements of these high-energy electrons before. <\/p>\n
Understanding what gives the radiation belts their shape and what can affect the way they swell or shrink helps scientists predict the onset of those changes. Such predictions can help scientists protect satellites in the area from the radiation. <\/p>\n
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NASAs Van Allen Probes Spot Impenetrable Radiation Barrier in Space<\/a><\/p>\n","protected":false},"excerpt":{"rendered":" Visualization of the radiation belts with confined charged particles (blue & yellow) and plasmapause boundary (blue-green surface). Credit: NASA\/Goddard Its a well-known fact that Earths ozone layer protects us from a great deal of the Suns ultra-violet radiation. Were it not for this protective barrier around our planet, chances are our surface would be similar to the rugged and lifeless landscape we observe on Mars. Continue reading