The aim of our studies was to examine turbulent, wavy structures in noctilucent clouds taking into account the clouds dusty plasma nature.
However, the dusty plasma nature of noctilucent clouds has been neglected.
We consider a weakly ionized dusty plasma composed of electrons, singly charged ions, negatively charged dust grains and neutrals.
Dustier layers appear to be deposited during periods when the atmosphere is dustier.
The transitions and the self-gravitational effects on the surface dust-ionacoustic mode are investigated in semi-bounded magnetized dusty plasmas.
The study of dusty plasmas is of significant practical use and scientific interest.
The dusty plasma aspect has been widely neglected, so far.
However, they all neglect the dusty plasma aspect.
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