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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?
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2.3.6 Identify shock accelerated particles
Created by
Yannis Zouganelis
, last modified on
25 Jun, 2017
Description of the objective:
Infer the rates of particle acceleration and the injection energies as a function of distance and along different parts of the shock.
mag/burst
mag/normal
metis/global
metis/cmeobs
epd/all
solohi/shock
solohi
solohi/synoptic
several-minutes
epd
rpw
radial
swa/triggered
swa/burst
mag
metis
swa
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{"serverDuration": 215, "requestCorrelationId": "3464809c7f1d585c"}