Scientists at the University of New Hampshire have unlocked one of the mysteries of how particles from flares on the sun accumulate at early stages in the energization of hazardous radiation that is harmful to astronauts, satellites and electronic equipment in space. Using data obtained by NASA’s Parker Solar Probe (PSP), researchers observed one of the largest events so far during the mission. These observations show how plasma that is released after a solar flare—a sudden flash of increased brightness—can accelerate and pile up energetic particles generating dangerous radiation conditions.
“We’re getting some of the earliest observations from this mission to the sun on how the coronal mass ejection—the sun’s release of plasma and energy—builds up particles released after solar flare events,” said Nathan Schwadron, professor of physics in UNH’s Space Science Center. “Because energetic particles are accelerated near the sun, by flying closer and getting a better look we are able to observe the beginning of the energization process and see them actually start to pile up like snow that piles up in front of a snowplow. Instead of an actual snowplow, it is the coronal mass ejections released from the sun that cause the buildup of this material in space.”
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Image: Using data from parker solar probe, UNH researchers observe sun’s plasma and energy build up particles released by solar flares - highlighting new phase of energizing process leading to radiation hazards. Credit: NASA