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Solar Orbiter SOC Public
Science Activity Plan (SAP)
Solar Orbiter detailed science objectives
Objective 3: How do solar eruptions produce energetic particle radiation that fills the heliosphere?
3.1 How and where are energetic particles accelerated at the Sun?
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3.1.4 Other high sensitivity X-ray studies
Created by
Yannis Zouganelis
, last modified on
25 Jun, 2017
3.1.4.1 Hard X-ray emission of escaping electron beams (thin-target emission)
3.1.4.2 X-ray emission from electrons accelerated at CME shocks
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{"serverDuration": 193, "requestCorrelationId": "85fe449e4e0bde68"}
