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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?
3.3 What are the seed populations for energetic particles?
3.3.1 What are the properties and distribution of suprathermal seed populations?
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3.3.1.1 Characterization of the suprathermal population
Created by
Yannis Zouganelis
, last modified on
25 Jun, 2017
Solar wind ions
Flare populations
Gradual SEP events
Pickup ions
Other particle populations
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{"serverDuration": 185, "requestCorrelationId": "0927222c627a8de2"}
