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The Ions

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Part of the Atmospheric Sciences Library book series (volume 5)

Abstract

Atmospheric atoms and molecules can be ionized either by short wavelength solar radiation (UV and x-rays), or by precipitating energetic particles:
$${\rm X}+{\rm h}\nu\rightarrow{\rm X}^{+}+{\rm e}$$
(6.1)
$${\rm X}+{\rm e}^{\ast}\rightarrow{\rm X}^{+}+2{\rm e}$$
(6.2)
where e* represents an energetic electron. These processes are the starting points for a series of reactions which determine the structure of the ionosphere. Several types of general reactions of importance in ion chemistry should be outlined in order to study the ionosphere. For example, different ions may be produced from the initial (also called primary) particles through charge exchange reactions with neutral molecules:
$${\rm X}^{+}+{\rm Y}\rightarrow{\rm Y}^{+}+{\rm X}$$
(6.3)
Negative ions can be formed by electron attachment on neutral species:
$${\rm e}+{\rm Z}+{\rm M}\rightarrow{\rm Z}^{-}+{\rm M}$$
(6.4)
Electrons can be released from negative ions, either by photodetachment or by collisional detachment:
$${\rm Z}^{-}+{\rm h}\nu\rightarrow{\rm Z}+{\rm e}$$
(6.5)
$${\rm Z}^{-}+{\rm M}\rightarrow{\rm Z}+{\rm M}+{\rm e}$$
(6.6)
Positively and negatively charged particles can recombine:
$${\rm X}^{+}+{\rm e}\rightarrow{\rm neutral}\ {\rm products}$$
(6.7)
$${\rm X}^{+}+{\rm Y}^{-}\rightarrow{\rm neutral}\ {\rm products}$$
(6.8)
We will examine the detailed chemistry of each of these processes below.

Keywords

Middle Atmosphere Lower Ionosphere Solar Proton Event Proton Hydrate Ionospheric Absorption 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

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© D. Reidel Publishing Company, Dordrecht, Holland 1986

Authors and Affiliations

  1. 1.Institut d’Aéronomie Spatiale and Université Libre de BruxellesBrusselsBelgium
  2. 2.Aeronomy LaboratoryNational Oceanic and Atmospheric AdministrationBoulderUSA

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