The Sunβs photosphere is dotted with dark, magnetically active regions called sunspots. Their number varies over an approximately 11βyear solar cycle, providing a key indicator of solar magnetic activity.
Because the raw monthly sunspot count can fluctuate sharply from month to month, solar physicists use a 13βmonth centered moving average, known as the **smoothed sunspot number**, to reveal the underlying trend of the solar cycle.
The smoothed value is calculated by weighting the current month and its six neighbours on each side, giving halfβweight to the outermost months and full weight to the inner ten months. This reduces shortβterm noise and highlights the longβterm evolution of solar activity.
What is the purpose of the smoothed sunspot number?
How is the smoothed sunspot number calculated?
Why do solar physicists use a 13-month moving average?
What does the smoothed sunspot number indicate?
How often does the sunspot number vary?
Can I use this calculator for any other purpose besides analyzing solar activity?
Where can I find the raw monthly sunspot data needed for this calculation?
Results are for informational purposes only and do not constitute professional advice.
