Detection asymmetry in solar energetic particle events

We used a published dataset of 239 CMEs recorded between 2006 and 2017 that had source regions both on the Sun’s front and far sides as seen from Earth. We produced distributions of occurrences of in situ SEP intensity enhancements associated with the CME events versus ∆φ, the longitudinal separation between the source AR and the spacecraft magnetic footpoint based on the nominal Parker spiral. We focussed on protons of energy >10 MeV measured by STEREO A, STEREO B, and GOES at 1 au.

We also considered occurrences of 71–112 keV electron events detected by MESSENGER between 0.31 and 0.47 au. Results. We find an east-west asymmetry with respect to the best magnetic connection (∆φ = 0) in the detection of >10 MeV proton events and of 71–112 keV electron events.

For protons, observers for which the source AR is on the eastern side of the spacecraft footpoint and not well connected (−180◦ < ∆φ < −40◦ ) are 93% more likely to detect an SEP event compared to observers with +40◦ < ∆φ < +180◦ . The asymmetry may be a signature of the corotation of magnetic flux tubes with the Sun since, for events with ∆φ < 0, corotation sweeps particle-filled flux tubes towards the observing spacecraft, while for ∆φ > 0 it moves them away.

Alternatively, it may be related to asymmetric acceleration or propagation effects.