Two bidirectional solar energetic particle events show sunward and anti-sunward proton streams with different release times and path lengths, attributed to shock and flare acceleration inside small-scale flux ropes.
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Bidirectional anisotropic solar energetic particle events observed by Solar Orbiter
Two bidirectional solar energetic particle events show sunward and anti-sunward proton streams with different release times and path lengths, attributed to shock and flare acceleration inside small-scale flux ropes.