Distribution of Temperature
This section discusses the global distribution of temperature as influenced by a myriad of factors. The interaction of insolation (incoming solar radiation) with the atmosphere and Earth's surface results in temperatures that vary across the globe. Several factors contribute to temperature variation:
-
Latitude: Locations at different latitudes receive varying amounts of solar energy. The angle at which sunlight strikes the Earth impacts the concentration of energy received; hence, equatorial regions receive more direct sunlight compared to pole regions.
-
Altitude: Temperature generally decreases with elevation, commonly referred to as the normal lapse rate of about 6.5°C per 1,000 meters. Areas at sea level are typically warmer than higher altitudes.
-
Distance from the Sea: Water bodies tend to warm up and cool down more slowly than land, leading to milder temperature variations in coastal regions compared to inland areas.
-
Air Masses and Ocean Currents: The influence of warm or cold air masses and ocean currents affect local temperatures, creating zones of varying climatic conditions.
-
Seasonal Variations: The isotherms, or lines of equal temperature, shift between January and July due to the Earth's axial tilt, impacting temperature zones differently in each hemisphere. For example, the northern hemisphere experiences substantial temperature variation due to its larger landmasses compared to the southern hemisphere.
The section also covers how temperatures can vary drastically, for instance, the continental interior can see a larger range in temperature compared to coastal regions. Understanding these concepts not only aids in meteorological studies but also enhances our insight into climatic changes and patterns on Earth.