The 2012 July 23 Backside Eruption: An Extreme Energetic Particle Event?
Nat Gopalswamy, Seiji Yashiro, Neeharika Thakur, Pertti M\"akel\"a,, Hong Xie, Sachiko Akiyama

TL;DR
The 2012 July 23 backside CME produced an extremely intense solar energetic particle event with high-energy particles, hard spectra, and shock characteristics similar to ground level enhancement events, indicating an extreme space weather occurrence.
Contribution
This study provides a detailed analysis linking CME speed and SEP spectral hardness, confirming the event's extremity and its similarity to GLE events, which was not previously established.
Findings
The event had a >10 MeV proton flux peaking at ~5000 pfu.
Shock speed exceeded 2000 km/s, typical of GLE events.
Spectral hardness correlated with CME initial speed.
Abstract
The backside coronal mass ejection (CME) of 2012 July 23 had a short Sun to Earth shock transit time (18.5 hours). The associated solar energetic particle (SEP) event had a >10 MeV proton flux peaking at ~5000 pfu, and the energetic storm particle (ESP) event was an order of magnitude larger, making it the most intense event in the space era at these energies. By a detailed analysis of the CME, shock, and SEP characteristics, we find that the July 23 event is consistent with a high-energy SEP event (accelerating particles to GeV energies). The time of maximum and fluence spectra in the range 10-100 MeV were very hard, similar to those of ground level enhancement (GLE) events. We found a hierarchical relationship between the CME initial speeds and the fluence spectral indices: CMEs with low initial speeds had SEP events with the softest spectra, while those with highest initial speeds…
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