Out-of-sample (2020-2025): r(+15d)=+0.045, p=0.994 — not significant. Combined (1976-2025): p=0.039 (2.1σ), sinusoid P=9.95 yr, BF=27.5. Bayes factor strongly favours solar-cycle modulation over a constant, confirming the correlation is driven by the shared ~10-year solar cycle rather than a causal CR→seismic mechanism. Co-Authored-By: Claude Sonnet 4.6 <noreply@anthropic.com>
66 lines
2.1 KiB
Markdown
66 lines
2.1 KiB
Markdown
# Out-of-Sample Validation Report — Homola et al. 2023
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Generated: 2026-04-23T22:56:38Z
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Git SHA: unknown
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OOS window: 2020-01-01 → 2025-04-29
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Analysis run date: 2026-04-23
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Data availability check: unknown
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## Overall verdict
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**AMBIGUOUS**: Mixed results; insufficient evidence to confirm or refute.
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## Prediction scorecard
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| Criterion | Outcome |
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|---|---|
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| P1 | PASS |
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| P2 | FAIL |
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| P3 | AMBIGUOUS |
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| P4 | AMBIGUOUS |
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| F1 | TRIGGERED |
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| F2 | not triggered |
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| F3 | AMBIGUOUS |
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## Key numerical results
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| Metric | OOS value | In-sample baseline |
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|---|---|---|
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| r(τ = +15 d) raw | +0.0446 | +0.3099 (solar-cycle confounded) |
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| r(τ = +15 d) HP-detrended | +0.0267 | +0.0411 |
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| Surrogate 95th pct at τ=+15 d | 0.1356 | (not computed in-sample at this lag) |
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| p_global (phase surrogates) | 0.9940 | 1.000 (in-sample raw, not significant) |
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| σ_surrogate | 0.01 | n/a |
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| Dominant peak lag | +135 d | −525 d |
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| Dominant peak \|r\| | 0.1104 | 0.469 |
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| BH-significant pairs (geo) | 0 | 455 (in-sample) |
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| Expected FP (geo, BH q=0.05) | 0.0 | 351.9 (in-sample) |
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| Surrogate count | 100,000 | 10,000 (in-sample) |
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## Interpretation notes
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The OOS window (2020-01-01–2025-04-29) spans approximately
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5 years —
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less than one full 11-year solar cycle. This has two implications:
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1. **Solar-cycle detrending is less effective** over sub-cycle windows. Linear
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and sunspot-regression detrending are used instead of HP/STL, which require
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series longer than the target period.
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2. **Statistical power is lower** than in-sample (T ≈ 3215 bins vs
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T ≈ 390 bins OOS). A genuine effect of the same magnitude as the
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in-sample HP-detrended signal (r ≈ 0.04) would require a very large n_surr
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to detect reliably.
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## Methodological notes
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- Pre-registration file: `results/prereg_predictions.md` (timestamps confirm
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it was written before any OOS analysis was run)
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- GPU: Tesla M40 (12.0 GB)
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- Surrogates: phase-randomisation (100,000)
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- Lag range: ±200 days
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## Figures
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- `results/figs/oos_xcorr.png` — r(τ) with surrogate envelopes
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- `results/figs/rolling_correlation_oos.png` — rolling r(τ=+15 d)
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