Study Notes on Atmospheric Heating and Cooling Concepts

Introduction to Atmospheric Concepts

  • Discussion on basic atmospheric processes based on normal conditions, not incorporating urban effects.
  • Future discussions will link atmospheric processes to urban areas.
  • Main focus areas for this video:
    • Heating and Cooling of the Earth.
    • Air Pressure.

Heating and Cooling of the Earth

  • Four main topics will be covered:
    1. Insolation (incoming solar radiation).
    2. Albedo.
    3. Evaporation.
    4. Differences in Heating and Cooling over land versus water.

Insolation

  • Definition: Incoming solar radiation; refers to solar energy received by the Earth.
  • Sensible vs. Non-sensible Heat:
    • We perceive heat as sensible heat, which is measurable using thermometers. This is generated when incoming shortwave radiation is absorbed and then re-emitted as longwave radiation.
    • Non-sensible heat refers to radiation that isn't captured by traditional temperature measures.
  • Heat Absorption Elements:
    • Various surfaces absorb insolation, including streets, roofs, vehicles, and clothing.
    • Upon reaching absorption capacity, surfaces release energy back into the atmosphere as long wave radiation.
  • Variation in Insolation:
    • Amount of insolation varies by latitude and time of year.
    • Higher levels of longwave radiation emission occur near the equator, leading to warmer temperatures compared to the poles.
    • Direct rays of the sun predominantly strike the equator during March and September, increasing insulation levels.

Albedo

  • Definition: Albedo measures an object's ability to reflect insolation.
  • High Albedo Surfaces:
    • Light-colored, smooth, or shiny surfaces (e.g., fresh snow).
    • Reflect substantial amounts of insulation, remaining cold despite sunny conditions.
  • Low Albedo Surfaces:
    • Darker or rougher surfaces are better at absorbing insulation (e.g., asphalt, sand).
    • Example of Snow: High albedo means it reflects more insulation, making it colder.
  • Water Bodies:
    • Variable albedo affected by factors such as clarity, depth, and solar angle.

Evaporation

  • Overview:
    • Evaporation cools the surroundings as water transitions from liquid to gas, requiring energy from the environment.
    • This absorbed energy is stored in vapor and cannot be felt (non-sensible).
  • Real-world Applications:
    • Misting fans and cooling towels demonstrate evaporation’s cooling effect; moisture evaporates, reducing local temperature.
  • Climate Variability in Evaporation:
    • Effective in dry climates (e.g., Southern California).
    • Inefficient in humid climates (e.g., Georgia, Florida) due to saturation of air with water vapor, which limits additional evaporation.

Differences in Heating and Cooling over Land vs. Water

  • Four Major Characteristics:
    1. Specific Heat
    • The amount of energy required to raise the temperature of a substance.
    • Water has a specific heat five times greater than land.
    • Example: Requires five times more energy to heat water by 1°C compared to sand.
    1. Transparency
    • Insolation penetrates water much deeper (up to several hundred feet in clear water).
    • In contrast, on land, insulation only penetrates a few centimeters.
    1. Mobility
    • Water’s mobility allows for circulation and upwelling, resulting in better heat absorption and distribution.
    • Land remains stagnant; shallow layers heat up quickly but cool down rapidly at night once heat is released.
    1. Evaporation
    • High evaporation over water surfaces promotes cooling effects.
    • Land surfaces, particularly dry areas, experience lower evaporation and can heat excessively.
  • Nighttime Temperature Differences:
    • Sandy beaches cool significantly overnight due to rapid heat loss, while water remains relatively warm due to heat retention.

Conclusion

  • Understanding these basic concepts provides foundational knowledge on atmospheric heating and cooling processes as well as the distinction between land and water interaction with solar radiation. Further concepts will build upon this foundational knowledge as we explore atmospheric dynamics in urban contexts.