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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?
3.1.3 Relativistic electron acceleration
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3.1.3.1 How shocks can accelerate electrons to relativistic energies (never observed for shocks near 1 AU)?
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Created by
Yannis Zouganelis
, last modified on
Feb 05, 2023
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How shocks can accelerate electrons to relativistic energies (never observed for shocks near 1 AU)? Is a more energetic seed population necessary?
Relevant SOOPs:
I_DEFAULT
swa
swa/normal
several-hours
perihelion
rpw
mag
epd
epd/all
metis
metis/global
metis/cmeobs
mag/normal
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{"serverDuration": 112, "requestCorrelationId": "f7d6a7d403862efa"}