The Oriented Scintillation Spectrometer Experiment onboard the Compton Gamm
a Ray Observatory observed a strong flux of neutrons from the behind-the-li
mb flare that occurred on 1991 June 1. This is surprising if the neutrons w
ere produced by thin-target interactions in the Sun's corona, as is suggest
ed by gamma-ray observations of this hare made by Granat/PHEBUS. We compare
neutron and gamma-ray observations of the June 1 hare with thick-target em
issions observed from a hare 3 days later, where the interactions took plac
e in the chromosphere and photosphere. A very hard spectrum for the acceler
ated particles is required to account for the number of neutrons observed o
n June 1 if they were produced by thin-target interactions in the corona.