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Updated: Mar 21, 2026

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Structural Design and Manufacturing of a Cruiser Class Solar Vehicle
Published on: January 30, 2019
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The Solar Cycle
1NASA Ames Research Center, Mail Stop: 258-5, Moffett Field, CA 94035 USA.
Summary
The solar cycle, an 11-year pattern of sunspot activity, influences various solar phenomena. This review examines solar cycle characteristics, variability, and prediction methods for solar cycles 23 and 24.
Area of Science:
- Solar physics
- Astronomy
Background:
- The 11-year solar cycle is a fundamental aspect of solar activity.
- Numerous indicators, including sunspots, radio flux, and geomagnetic activity, correlate with this cycle.
Approach:
- This review synthesizes information on the characteristics of individual solar cycles.
- It examines cycle-to-cycle and short-term variability, including phenomena like the Maunder Minimum and double-peaked maxima.
Key Points:
- Solar cycle characteristics include maxima, minima, amplitude, shape, and latitudinal drift of active regions.
- Variability encompasses long-term trends (Maunder Minimum, Gleissberg Cycle) and short-term fluctuations (154-day periodicity).
- Solar activity indicators such as sunspots, radio flux, irradiance, and geomagnetic activity are discussed in relation to the solar cycle.
Conclusions:
- Understanding solar cycle prediction techniques is crucial for space weather forecasting.
- The review provides insights into solar cycles 23 and 24, highlighting their specific features and prediction challenges.
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