Pathfinding Experiment to Study Origins of Solar Energetic Particles

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A joint NASA-U.S. Naval Research Laboratory experiment dedicated to studying the origins of solar energetic particles — the Sun’s most dangerous form of radiation — is ready for launch.

A joint NASA-U.S. Naval Research Laboratory experiment dedicated to studying the origins of solar energetic particles — the Sun’s most dangerous form of radiation — is ready for launch.

UVSC Pathfinder — short for Ultraviolet Spectro-Coronagraph Pathfinder — will hitch a ride to space aboard STPSat-6, the primary spacecraft of the Space Test Program-3 (STP-3) mission for the Department of Defense. STP-3 is scheduled to lift off on a United Launch Alliance Atlas V 551 rocket no earlier than Nov. 22, from Cape Canaveral Space Force Station in Florida.

Solar energetic particles, or SEPs, are a type of space weather that pose a major challenge to space exploration. A solar particle storm, or SEP event, occurs when the Sun fires energetic particles into space at such high speeds that some reach Earth — 93 million miles away — in less than an hour. Flurries of the powerful particles can wreak havoc with spacecraft and expose astronauts to dangerous radiation.

UVSC Pathfinder will peer at the lowest regions of the Sun’s outer atmosphere, or corona, where SEPs are thought to originate. While the Sun releases eruptions almost daily when it is most active, there are only about 20 disruptive solar particle storms during any given 11-year solar cycle. Scientists can’t reliably predict which of these will produce SEPs, nor their intensity. Understanding and eventually predicting these solar storms are crucial for enabling future space exploration.

Read more at: NASA Goddard Space Flight Center