Photochemical Smog Explained: Formation and Effects

Added:

Smog Basics
Smog Types
Reaction Chain
Cycle Impact

Smog Basics

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Playing Section
  • 1

    Defines smog as fog and smoke mixture in industrial cities.

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    Explains classical smog from fossil fuels in cool climates.

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    Notes London smog is reducing and occurs day or night.

Understanding the basic structure of the Earth's atmosphere, specifically the difference between the troposphere and the stratosphere.
Fundamental concepts of chemical reactions, specifically how solar radiation (UV light) can initiate photochemical reactions (photolysis).
The distinction between primary air pollutants (such as nitrogen oxides and volatile organic compounds) and secondary air pollutants (such as ground-level ozone).
Basic knowledge of fossil fuel combustion processes and how they generate vehicular and industrial emissions.
The role of meteorological phenomena, such as thermal inversions, in trapping and intensifying photochemical smog in urban basins.
Engineered solutions and technologies designed to mitigate precursor emissions, such as catalytic converters and vapor recovery systems.
Environmental policy frameworks and air quality standards, such as the Clean Air Act and Air Quality Index (AQI) monitoring.
The biochemical mechanisms of how ozone and PANs (peroxyacyl nitrates) cause oxidative stress in plant tissues and human respiratory systems.
133.4K views2.3Klikes8:20@KINETICSCHOOLOriginal Release: 2019-01-15

Photochemical smog is a brown haze formed when ultraviolet light reacts with nitrogen oxides (NOx) and volatile organic compounds (VOCs) from vehicle exhaust, industrial emissions, and other sources; the primary formation reactions involve N₂ + O₂ → 2NO, 2NO + O₂ → 2NO₂, NO₂ + hν → NO + O, and O + O₂ + M → O₃, with ozone being the main component; this oxidizing smog causes eye irritation, respiratory damage, and vegetation harm, and was first identified in Los Angeles in 1944.