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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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2.3.2.3 Study heating and dissipation mechanisms at shocks with radial distance
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Created by
Yannis Zouganelis
, last modified on
Feb 05, 2023
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Description of the objective (to be written):
Relevant SOOPs:
L_FULL_HRES_HCAD_Coronal-Dynamics
swa
swa/triggered
swa/burst
several-minutes
radial
rpw
mag
epd
solohi
solohi/shock
solohi/synoptic
stereo
mag/normal
mag/burst
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{"serverDuration": 61, "requestCorrelationId": "7191cfe1ebd256c6"}