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This book introduces systematically the concept of weakly-bound
complexes into the broad field of atmospheric sciences. To fill up
the gap between our rapidly expanding knowledge of the individual
properties of Van der Waals and hydrogen-bonded molecules, and our
understanding of their role in the atmospheric processes, an
ensemble of related topics are covered by a team of expert
co-authors. The general properties of the weakly bound molecular
complexes (or "clusters") are discussed, as well as their
distribution in the planetary atmospheres. Collision-induced and
dimeric absorption and emission are considered in the context of
atmospheric spectroscopy. The advanced experimental techniques
which enable us to study the spectroscopic features of molecular
complexes in the gas phase, or which are adsorbed, are reviewed.
The role of molecular complexes in the cometary atmosphere, the
Earth mesosphere, and the atmospheres of the giant planets and some
of their satellites are also discussed in detail.
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