Total Solar Irradiance (TSI) represents the amount of solar energy received per unit area outside the Earth's atmosphere on a surface perpendicular to the sun's rays. It is essentially the sum of all types of solar radiation reaching the Earth's atmosphere. TSI is a fundamental measure, often referred to as the solar constant, with an approximate value of 1361 W/m².
While TSI is crucial for understanding the potential energy available from the sun, it should be noted that not all this energy reaches the Earth's surface unattenuated. During the path through the atmosphere, several factors such as absorption, scattering, and reflection can reduce the amount of solar energy available for practical use.
Important aspects of TSI include:
- TSI affects the Earth's climate by determining the amount of energy available to the planet's surface.
- It is an essential input for models predicting weather and climate patterns.
- The comparison of DNI and TSI helps illustrate the impact of atmospheric conditions on solar power viability.
Thus, comparing DNI with the total solar irradiance highlights the significant reduction in energy content due to atmospheric and environmental factors, as shown in our exercise.