Large airglow enhancements produced via wave-plasma interactions in sporadic E

In the past there has been great interest in monitoring enhanced 557.7 nm O (S-1) emissions from the thermosphere in connection with high-power, high-f requency (HF) radio wave modification of the F region ionosphere. These emi ssions are considered to be evidence that the HF-modified electron distribu tion function is non-Maxwellian because a significant flux of similar to 5- 6 eV electrons is required to produce the airglow. The suprathermal tail is believed to develop as a result of nonlinear plasma processes. Past F regi on observations of 557.7 nm airglow at Arecibo Observatory, Puerto Rico hav e yielded only a few Rayleighs of enhanced emissions. Recently, airglow enh ancements were monitored in sporadic E above Arecibo. Surprisingly, these e xperiments yielded similar to 55 Rayleighs of enhanced 557.7 nm airglow and the first observations of emissions from the N-2 first positive molecular bands. The observations imply that a large flux of energetic (5-10 eV) elec trons is generated as part of the wave-plasma interaction in sporadic E.