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E > 10 MeV ions observed in gradual solar energetic particle (SEP) events are attributed to acceleration at shocks driven by coronal mass ejections (CMEs), but it has been suggested that such SEPs may also result from acceleration in the magnetic reconnection of coronal arcades following CMEs. The arcade SEPs could escape the corona along open field lines, but those components of SEP events would be difficult to distinguish from shock SEPs. We examine large solar soft X-ray arcades and metricdoi:10.1086/308680 fatcat:hyg6gu7b6bbgrjrhc7zuqt3o3a