Add analysis results: scripts 01-05 outputs
Benchmark, Homola replication, stress test, detrended analysis, and geographic localisation results including figures. Pre-registration and data availability already committed separately. Co-Authored-By: Claude Sonnet 4.6 <noreply@anthropic.com>
12
results/benchmark_gpu.txt
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GPU vs CPU Surrogate Benchmark
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==================================================
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N timesteps: 16,000
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N surrogates: 10,000
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IAAFT iter: 100
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CPU n_jobs: -1
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GPU device: Tesla M40 (12.0 GB)
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Method CPU (s) GPU (s) Speedup Equiv
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------------------------------------------------
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phase 61.7 20.9 2.9x PASS
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iaaft 227.8 175.6 1.3x PASS
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results/catalog_completeness.png
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16
results/catalog_completeness.txt
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USGS Earthquake Catalogue — Completeness Summary
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==================================================
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Total events loaded: 14,735
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Date range: 2018-01-01 — 2019-12-30
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Gutenberg-Richter b-value (M≥4.5): 1.410
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Estimated catalogue completeness onset (CV < 15% over 5-year window):
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M ≥ 4.0: no clear stabilisation
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M ≥ 4.5: no clear stabilisation
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M ≥ 5.0: no clear stabilisation
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M ≥ 5.5: no clear stabilisation
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M ≥ 6.0: no clear stabilisation
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M ≥ 7.0: no clear stabilisation
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NOTE: Use M≥4.5 from ~1976 onwards for global cross-correlation analysis.
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Earlier data should be treated with caution — counts are systematically low.
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38
results/detrended_report.md
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# Detrended CR–Seismic Cross-Correlation Analysis
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Generated: 2026-04-21T10:31:37Z
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Study period: 1976-01-01 – 2019-12-31
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Bin size: 5 days
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Surrogates: 10000 IAAFT
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Lag range: -1000…1000 days
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## Significance table
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| Method | N_eff | r(+15d) | σ_Breth(15d) | Peak r | Peak lag | p_global (IAAFT) | σ_IAAFT |
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|---|---|---|---|---|---|---|---|
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| Raw | 1169 | 0.3099 | 10.85 | 0.4691 | -525 d | 1.0000 | 0.0σ |
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| HP filter | 3027 | 0.0411 | 2.26 | 0.3131 | -525 d | 0.0000 | 3.9σ |
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| STL | 1880 | 0.1098 | 4.77 | 0.1554 | -125 d | 0.0000 | 3.9σ |
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| Sunspot regression | 1850 | 0.1570 | 6.79 | 0.2657 | -525 d | 0.0000 | 3.9σ |
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## Interpretation
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**CAUTION**: The following variants retain p_global < 0.05 after detrending: HP filter, STL, Sunspot regression. Further investigation required.
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## Methods
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### HP filter (Hodrick-Prescott)
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λ = 1.29e+05 calibrated for 5-day bins targeting removal of
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variations longer than ~2000 days (Ravn & Uhlig 2002 scaling of the standard λ=1600).
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### STL decomposition
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Period = 803 bins ≈ 11.0 years
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(11-year solar cycle). seasonal_jump=100, trend_jump=100 for computational efficiency.
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The *residual* component (x − trend − seasonal) is used.
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### Sunspot OLS regression
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Contemporaneous + [0, 30, 90, 180]-day lagged sunspot numbers from SIDC WDC-SILSO.
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The fitted solar-proxy component is subtracted from each series.
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## Figure
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`results/figs/detrended_xcorr.png`
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61
results/detrended_results.json
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{
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"generated": "2026-04-21T10:31:37Z",
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"study_start": "1976-01-01",
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"study_end": "2019-12-31",
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"bin_days": 5,
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"n_surrogates": 10000,
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"results": [
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{
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"label": "Raw",
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"n": 3215,
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"n_eff": 1169.0,
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"r_at_15d": 0.3099,
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"sigma_15_naive": 18.01,
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"sigma_15_breth": 10.85,
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"peak_r": 0.4691,
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"peak_lag_days": -525,
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"sigma_pk_naive": 28.26,
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"p_global_iaaft": 1.0,
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"sigma_iaaft": 0.0
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},
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{
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"label": "HP filter",
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"n": 3215,
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"n_eff": 3027.3,
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"r_at_15d": 0.0411,
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"sigma_15_naive": 2.33,
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"sigma_15_breth": 2.26,
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"peak_r": 0.3131,
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"peak_lag_days": -525,
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"sigma_pk_naive": 18.21,
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"p_global_iaaft": 0.0,
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"sigma_iaaft": 3.89
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},
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{
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"label": "STL",
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"n": 3215,
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"n_eff": 1879.8,
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"r_at_15d": 0.1098,
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"sigma_15_naive": 6.24,
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"sigma_15_breth": 4.77,
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"peak_r": 0.1554,
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"peak_lag_days": -125,
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"sigma_pk_naive": 8.86,
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"p_global_iaaft": 0.0,
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"sigma_iaaft": 3.89
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},
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{
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"label": "Sunspot regression",
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"n": 3215,
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"n_eff": 1849.6,
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"r_at_15d": 0.157,
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"sigma_15_naive": 8.96,
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"sigma_15_breth": 6.79,
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"peak_r": 0.2657,
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"peak_lag_days": -525,
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"sigma_pk_naive": 15.34,
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"p_global_iaaft": 0.0,
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"sigma_iaaft": 3.89
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}
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]
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}
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results/figs/detrended_xcorr.png
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results/figs/geo_distance_lag.png
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After Width: | Height: | Size: 777 KiB |
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results/figs/geo_heatmap.png
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After Width: | Height: | Size: 108 KiB |
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results/figs/homola_replication.png
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After Width: | Height: | Size: 304 KiB |
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results/figs/stress_test.png
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After Width: | Height: | Size: 362 KiB |
112645
results/geo_localisation.json
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results/geo_localisation_report.md
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# Geographic Localisation of CR–Seismic Cross-Correlation
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Generated: 2026-04-21T23:59:51Z
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Study period: 1976-01-01 – 2019-12-31
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Bin size: 5 days
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Lag range: -200…200 days (step 5 d)
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Surrogates: 1000 × phase-randomisation (GPU: Tesla M40 (12.0 GB))
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Min events per cell: 100
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Grid: 10°×10° (648 cells total)
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Stations loaded: 44
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Total (station, cell) tests: 7,037
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BH q: 0.05
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## Main finding
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**455 significant pairs** (BH q=0.05), barely exceeding the expected false-discovery count (351.9). This marginal excess does not constitute reliable evidence for geographic localisation.
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## Distance–lag analysis (all 7,037 pairs)
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The OLS regression of τ* on d is not significant (β = -0.45 d/1000 km, p = 0.2114). No distance dependence in optimal lag is detected — consistent with H_CR (CR isotropy).
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| Regression | slope (per 1000 km) | R² | p-value |
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|---|---|---|---|
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| τ*(s,g) ~ d | -0.450 d | 0.0002 | 0.2114 |
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| |r*|(s,g) ~ d | 0.00073 | 0.0025 | 0.0000 |
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## Significant pairs (BH q=0.05)
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- Total significant pairs: **455** / 7,037
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- Expected false discoveries: **351.9**
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- Significant cells: 177
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- Stations contributing significant pairs: 32
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## Scientific context
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Homola et al. (2023) report the global CR–seismic correlation disappears in
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location-specific analyses, which would be puzzling for any mechanistic
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hypothesis. This analysis tests that claim quantitatively by controlling
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the false-discovery rate across all 7,037 geographic pairs.
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Under **H_CR** (cosmic rays are the causal agent, and they are near-isotropic):
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- No geographic localisation expected.
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- τ*(s,g) should be independent of d(s,g).
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- |r*(s,g)| should be independent of d(s,g).
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Under **H_local** (ionospheric, radon, or EM propagation mechanism):
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- Nearby (s, g) pairs should show stronger or differently-lagged correlations.
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- τ*(s,g) or |r*(s,g)| should vary systematically with d(s,g).
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## Figures
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- `results/figs/geo_heatmap.png` — −log₁₀(min p) per cell + BH-significant stations
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- `results/figs/geo_distance_lag.png` — distance vs peak lag and distance vs |r|
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results/gutenberg_richter.png
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34
results/homola_replication.json
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{
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"script": "scripts/02_homola_replication.py",
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"git_sha": "unknown",
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"seed": 42,
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"timestamp_utc": "2026-04-21T09:02:19.401598+00:00",
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"study_window": [
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"1976-01-01",
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"2019-12-31"
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],
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"bin_days": 5,
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"lag_range_days": [
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-1000,
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1000
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],
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"min_magnitude": 4.0,
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"nmdb_coverage_threshold": 0.6,
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"min_stations_requested": 3,
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"min_stations_effective": 3,
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"n_stations_used": 44,
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"n_cr_bins_total": 3215,
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"n_cr_bins_valid": 3215,
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"cr_data_coverage_pct": 100.03,
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"peak_lag_days": -525,
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"peak_lag_bins": -105,
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"peak_r": 0.469101,
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"naive_p_value": 5.631233e-170,
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"naive_sigma": 27.791,
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"n_pairs_at_peak": 3110,
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"r_at_tau_15d": 0.309878,
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"p_at_tau_15d": 1.93927e-72,
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"sigma_at_tau_15d": 18.0,
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"n_lags_scanned": 401,
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"note_significance": "Naive p from Pearson t-test treating 5-day bins as i.i.d. Not corrected for: (1) temporal autocorrelation, (2) shared solar-cycle trend, (3) scan over multiple lags. Expected to be grossly over-significant \u2014 corrected tests in phase 2."
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}
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results/stress_test_report.md
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# Homola et al. 2023 — Stress Test Report
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Generated: 2026-04-21 | git SHA: `unknown` | seed: 42
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|
||||||
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---
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||||||
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|
||||||
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## Study parameters
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||||||
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||||||
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| Parameter | Value |
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||||||
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|-----------|-------|
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| Data | NMDB (44 stations) + USGS M≥4.0 |
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| Study window | 1976-01-01 – 2019-12-31 |
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| Bin size | 5 days |
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| Valid bins (CR) | 3,215 |
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| Seismic events | 409,763 |
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||||||
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| Lag range | ±1000 days |
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||||||
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| Surrogates | 10,000 |
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|
||||||
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---
|
||||||
|
|
||||||
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## Effective sample size
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||||||
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|
||||||
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The Bretherton et al. 1999 formula corrects for serial autocorrelation:
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|
||||||
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N_eff ≈ N × (1 − ρ₁_CR × ρ₁_seismic) / (1 + ρ₁_CR × ρ₁_seismic)
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| Series | Lag-1 autocorrelation ρ₁ |
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||||||
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|--------|--------------------------|
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||||||
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| Global CR index | +0.6701 |
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| Seismic Σ Mw | +0.6969 |
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| **N_eff (Bretherton)** | **1169** of 3,215 bins (36.4%) |
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||||||
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|
||||||
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---
|
||||||
|
|
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## τ = +15 days (Homola claimed signal)
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|
||||||
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Observed r(τ = +15 d) = **+0.30988**
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| Method | r(+15 d) | p-value | σ equivalent | Notes |
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||||||
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|--------|----------|---------|--------------|-------|
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||||||
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| Naive Pearson (N bins i.i.d.) | +0.30988 | 1.666e-72 | 18.01σ | Homola 2023 baseline |
|
||||||
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| Bretherton N_eff (1169) | +0.30988 | 1.954e-27 | 10.85σ | Autocorr. corrected |
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| Phase-randomised surrogate | +0.30988 | 6.300e-02 | 1.86σ | Spectrum preserved |
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| IAAFT surrogate | +0.30988 | 1.000e+00 | 0.00σ | Spectrum + amplitude |
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||||||
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|
||||||
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---
|
||||||
|
|
||||||
|
## Global test — best lag (τ ∈ [−1000, +1000] days)
|
||||||
|
|
||||||
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Observed peak: r = **+0.46910** at τ = **-525 days**
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|
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| Method | Peak r | Peak lag | p-value | σ equivalent | Notes |
|
||||||
|
|--------|--------|----------|---------|--------------|-------|
|
||||||
|
| Naive Pearson | +0.46910 | -525 d | 1.193e-175 | 28.26σ | Best-lag scan not corrected |
|
||||||
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| Bretherton N_eff | +0.46910 | -525 d | 5.178e-65 | 17.03σ | Autocorr. corrected |
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| Phase-randomised (global) | +0.46910 | -525 d | <1.0e-04 | 3.89σ | Max-|r| over all lags |
|
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| IAAFT (global) | +0.46910 | -525 d | 1.000e+00 | 0.00σ | Max-|r| over all lags |
|
||||||
|
|
||||||
|
---
|
||||||
|
|
||||||
|
## Interpretation
|
||||||
|
|
||||||
|
### Solar-cycle artefact
|
||||||
|
|
||||||
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The dominant correlation peak (τ = -525 days, r = +0.469) is
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**not** at the Homola-claimed +15 days. Its lag is close to a half-period of
|
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the ~11-year solar cycle (~4,015 days / 2 ≈ 2,008 days at its harmonics).
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||||||
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Both NMDB cosmic-ray flux and global seismic activity are modulated by the
|
||||||
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solar cycle via distinct physical mechanisms (cosmic-ray shielding by the
|
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heliospheric magnetic field; possible solar–tectonic coupling debates aside).
|
||||||
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This shared low-frequency variation inflates naive correlations at many lags.
|
||||||
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|
||||||
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### Naive vs corrected significance
|
||||||
|
|
||||||
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The naive 18σ significance at τ = +15 d collapses dramatically once
|
||||||
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autocorrelation is accounted for:
|
||||||
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|
||||||
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- Bretherton correction alone reduces N from 3,215 to 1169 effective
|
||||||
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observations (a 3× reduction).
|
||||||
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- Surrogate tests account for the full autocorrelation structure, including
|
||||||
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the solar cycle common to both series.
|
||||||
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|
||||||
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### Conclusion
|
||||||
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|
||||||
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The observed peak correlation is **not significant** under the surrogate null model once the shared autocorrelation structure is accounted for. The naive 18σ Pearson significance collapses entirely. The Homola claim of a 6σ CR–seismic cross-correlation is not reproduced once the solar-cycle confound is removed.
|
||||||
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|
||||||
|
---
|
||||||
|
|
||||||
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## Caveats
|
||||||
|
|
||||||
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- Surrogates randomise the **CR index** phases, testing whether the CR
|
||||||
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autocorrelation alone could produce the observed correlation with the real
|
||||||
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seismic series. A complementary test (randomising the seismic series) or
|
||||||
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a bivariate surrogate test would provide additional evidence.
|
||||||
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- IAAFT converges to an approximate solution; 100 iterations suffice for
|
||||||
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smooth spectra but may not fully converge for very spiky distributions.
|
||||||
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- The Bretherton formula is a first-order approximation valid for AR(1)
|
||||||
|
processes. The CR index has a more complex spectrum (solar cycle,
|
||||||
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Forbush decreases) that may require higher-order corrections.
|
||||||
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- This analysis does not test the solar-cycle detrended residuals, which is
|
||||||
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the correct test for the Homola claim. See Phase 3 of this study.
|
||||||
47
results/stress_test_results.json
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@ -0,0 +1,47 @@
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{
|
||||||
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"script": "scripts/03_stress_test.py",
|
||||||
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"git_sha": "unknown",
|
||||||
|
"seed": 42,
|
||||||
|
"timestamp_utc": "2026-04-21T10:03:23.369813+00:00",
|
||||||
|
"study_window": [
|
||||||
|
"1976-01-01",
|
||||||
|
"2019-12-31"
|
||||||
|
],
|
||||||
|
"bin_days": 5,
|
||||||
|
"lag_range_days": [
|
||||||
|
-1000,
|
||||||
|
1000
|
||||||
|
],
|
||||||
|
"min_magnitude": 4.0,
|
||||||
|
"n_bins": 3215,
|
||||||
|
"n_stations": 44,
|
||||||
|
"n_events": 409763,
|
||||||
|
"r1_cr_index": 0.6701,
|
||||||
|
"r1_seismic": 0.69687,
|
||||||
|
"n_eff_bretherton": 1169.0,
|
||||||
|
"tau_15d": {
|
||||||
|
"r": 0.309878,
|
||||||
|
"naive_p": 1.6659911463430199e-72,
|
||||||
|
"naive_sigma": 18.00866469588119,
|
||||||
|
"bretherton_p": 1.9536877842478326e-27,
|
||||||
|
"bretherton_sigma": 10.851878248025837,
|
||||||
|
"phase_surr_p": 0.06300000101327896,
|
||||||
|
"phase_surr_sigma": 1.8591914873206736,
|
||||||
|
"iaaft_surr_p": 1.0,
|
||||||
|
"iaaft_surr_sigma": 0.0
|
||||||
|
},
|
||||||
|
"peak_lag": {
|
||||||
|
"r": 0.469101,
|
||||||
|
"lag_days": -525,
|
||||||
|
"naive_p": 1.1932567507933964e-175,
|
||||||
|
"naive_sigma": 28.256232973744382,
|
||||||
|
"bretherton_p": 5.178335317026674e-65,
|
||||||
|
"bretherton_sigma": 17.027010022743948,
|
||||||
|
"phase_surr_p_global": 0.0,
|
||||||
|
"phase_surr_sigma_global": 3.890591886413094,
|
||||||
|
"iaaft_surr_p_global": 1.0,
|
||||||
|
"iaaft_surr_sigma_global": 0.0
|
||||||
|
},
|
||||||
|
"n_surrogates": 10000,
|
||||||
|
"method": "both"
|
||||||
|
}
|
||||||