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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?
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2.3.2.4 Identify mechanisms that heat the thermal solar wind particle populations near shocks and determine their energy partition
Created by
Yannis Zouganelis
, last modified on
05 Feb, 2023
Description of the objective (to be written):
Relevant SOOPs:
L_FULL_HRES_HCAD_Coronal-Dynamics
mag/burst
mag/normal
solohi/shock
stereo
solohi
solohi/synoptic
several-minutes
epd
rpw
radial
swa/triggered
swa/burst
mag
swa
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{"serverDuration": 195, "requestCorrelationId": "4be8f8fe7d97eea0"}
