Here are the essential concepts you must grasp in order to answer the question correctly.
Stratospheric Chemistry
Stratospheric chemistry involves the study of chemical reactions that occur in the stratosphere, particularly those involving ozone (O3) and other atmospheric gases. The reactions can influence the concentration of ozone, which plays a crucial role in absorbing ultraviolet (UV) radiation from the sun, thereby affecting temperature and climate patterns.
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Photodissociation
Photodissociation is the process by which a chemical compound is broken down by photons, typically ultraviolet light. In the context of the stratosphere, the reaction O2(g) + hv → 2 O(g) illustrates how UV radiation can lead to the formation of reactive oxygen atoms, which can subsequently participate in other reactions that may affect temperature.
Ozone Formation and Depletion
Ozone formation and depletion are critical processes in the stratosphere that influence temperature. Reactions that produce ozone, such as O(g) + O2(g) → O3(g), can lead to warming as ozone absorbs UV radiation. Conversely, reactions that deplete ozone can lead to cooling effects, making it essential to understand these dynamics when analyzing temperature changes in the stratosphere.
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Formation Equations Example 1