Particle scattering due to a Rosenbluth-Post convective loss-cone instability is calculated using a slab model. This collective contribution to the scattering rate is found to be the classical scattering rate increased by a factor ${({{T}ᵢ}{{T}ₑ})}3/2{({{m}ₑ}{{m}ᵢ})}1/2{(ln{Λ})}^{{-}1}×{}(energyamplificationoftheconvectiveinstabilityinthefiniteplasma)$.
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Baldwin et al. (1972) studied this question.
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