There are many problems yet to be resolved in this field.
If it is assumed that the major ions in sporadic E are NO+ and O+, then ionospheric studies and laboratory measurements suggest an appropriate value of α (the recombination coefficient) to be of order 10−7 cm3 sec−1 at room temperatures. This conflicts with the highest value of α tolerable to wind‐shear theory of about 3 × 10−8 cm3 sec−1. High electron temperatures in sporadic E clouds may reduce this discrepancy if a decreases with increase of temperature. In its present stage of development the windshear theory does not account for the high electron temperatures sometimes observed in association with sporadic E, nor does it account for the magnetic variation observed in association with sporadic E clouds.
The possibility of an airglow component caused by recombination in sporadic E clouds is discussed.
We conclude that measurements of ion composition, electron temperature, electric current, and VLF noise in sporadic E clouds should provide valuable clues in the further understanding of the phenomenon.