The Sunβs output is not constant; it varies over an approximately 11βyear magnetic cycle known as the solar cycle. During this cycle the number of sunspots, solar flares, and the overall magnetic activity rise and fall, leading to measurable changes in the total solar irradiance that reaches Earth.
Solar irradiance is typically expressed as the solar constant, about 1361β―Wβ―mβ»Β² at the top of the atmosphere during a quiet Sun. However, observations show that this value can increase by roughly 0.1β―% near solar maximum and decrease by a similar amount near solar minimum.
To estimate the irradiance for a given phase of the cycle, a simple linear model can be used: the base solar constant multiplied by a factor that accounts for the percentage variation associated with the chosen phase.
What is the solar constant?
How does solar irradiance vary over time?
What causes the solar cycle?
How does solar irradiance variation affect Earth?
What is the significance of sunspots in the solar cycle?
Can solar irradiance variation impact satellite operations?
How is total solar irradiance measured?
Results are for informational purposes only and do not constitute professional advice.
