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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?
3.1 How and where are energetic particles accelerated at the Sun?
3.1.1 CME and shock associated SEP sources
3.1.1.2 Why are gradual SEP events so variable?
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3.1.1.2.3 Warped shock fronts
Created by
Yannis Zouganelis
, last modified on
05 Feb, 2023
Relevant SOOPs:
L_IS_SoloHI_STIX
mag/normal
epd/all
solohi/shock
solohi
solohi/synoptic
several-minutes
epd
rpw
radial
swa/triggered
swa/burst
mag
swa
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{"serverDuration": 240, "requestCorrelationId": "057824a777c1595d"}
