Solar Irradiance Analysis
Long-term structure, a strong repeating cycle, and a long interval in the seventeenth century where the cycle is absent.
Long-term structure, a strong repeating cycle, and a long interval in the seventeenth century where the cycle is absent.
The series is best described by a periodic component with a period near eleven years, modulated by a changepoint structure that switches the cycle off during the Maunder minimum, over a slowly varying baseline.
Annual reconstructed total solar irradiance, 1610–2011, 402 observations. Reconstructions before the satellite era carry substantially more uncertainty than later values; this analysis treats the series as observed and does not propagate reconstruction error.
Sunspot-driven cyclic behaviour is visible across most of the record, with amplitude varying between cycles. The seventeenth-century interval is conspicuously flat.
| Component | Structure | Interpretation |
|---|---|---|
| 1 | PER | Approximately eleven-year cycle |
| 2 | CP × PER | Cycle suppressed during 1645–1715 |
| 3 | SE | Slow baseline variation |
| 4 | WN | Observation noise |
Fitting a single periodic component without the changepoint produces systematically poor residuals in the quiet interval and understates the amplitude elsewhere, because one variance has to cover both regimes. This is the clearest illustration in the classic examples of why a model needs permission to say that behaviour changed.
The reconstruction itself is a model output, not a direct measurement, for most of the record. Conclusions about absolute levels should be treated accordingly.
Periodic kernels, changepoint detection and the treatment of forecast uncertainty.