The irradiance of the sun, or the amount of solar energy received per unit area, primarily depends on several factors:
-
The wavelength of the radiant energy it emits: The sun emits energy across a range of wavelengths, with the peak of this emission lying in the visible spectrum. The irradiance varies depending on these wavelengths due to the different efficiencies of energy transmission through the Earth's atmosphere.
-
The distance from the sun: The irradiance decreases with the square of the distance from the sun due to the inverse square law.
-
Solar activity: Factors such as the number of sunspots can indirectly affect irradiance, but this is a more complex relationship. Solar cycles can influence the total solar irradiance slightly.
-
Atmospheric conditions on Earth: Conditions such as cloud cover and air quality can affect the amount of solar irradiance that reaches the surface.
While energetic solar wind particles and the density of particles in the solar wind are important in understanding solar phenomena and space weather, they do not directly influence the irradiance of solar energy that reaches the Earth.
So, the correct and most relevant option regarding the irradiance of the sun would be the wavelength of the radiant energy it emits.