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- Solar Orbiter SOC Public
- Science Activity Plan (SAP)
- Solar Orbiter detailed science objectives
- Objective 2: How do solar transients drive heliospheric variability?
- 2.3 How and where do shocks form in the corona and in the heliosphere?
- 2.3.2 What are the properties and distribution of heliospheric shocks?
2.3.2.4 Identify mechanisms that heat the thermal solar wind particle populations near shocks and determine their energy partition
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